Space Math Problems Sorted by NASA Mission and Program
Advanced Composition Explorer (ACE)
Problem 81: The Pressure of a Solar Storm - Students will examine three mathematical models for determining how much pressure a solar storm produces as it affects Earth's magnetic field. They will learn that magnetism produces pressure, and that this accounts for many of the details seen in solar storms. [Grade level: 9-11 | Topics: Substituting numbers into equations; filling out missing table entries; data interpretation; mathematical models ]
Cassini - Huygens
Problem 461: Cassini Delivers Holiday Treats from Saturn
Students explore proportions and angular size using images of Saturn's moons Titan and Dione
[Grade: 7-9 | Topics: scale models; proportions]
(PDF)
Problem 335: Methane Lakes on Titan Students use a recent Cassini radar image of the surface of Titan to estimate how much methane is present in the lakes that fill the image, and compare the volume to that of the fresh water lake, Lake Tahoe. [Grade: 6-8 | Topics: estimating irregular areas; calculating volume from area x height; scaled images ]
Problem 315: The Mysterious Hexagon on Saturn A curious hexagon formed by the Saturn polar jet stream, and photographed by the Cassini spacecraft, is used to determine wind speed and acceleration. [Grade: 6-9 | Topics: Measuring; Metric Units; speed=distance/time]
Problem 154: Pan's Highway and Saturn's Rings Students use an image from the Cassini spacecraft to determine how large the satellite Pan is, and the scale of Saturn's rings using a millimeter ruler. [Grade: 4-6 | Topics:Finding the scale of an image; measurement; unit conversion]
Problem 135: How Big is It? - Io and Jupiter. Students work with an image taken by the Cassini spacecraft of Jupiter and its satellite Io. They determine the image scale, and calculate the sizes of various features in the image. [Grade: 4 - 7 | Topics:image scaling; multiply, divide, work with millimeter ruler]
Chandra X-Ray Observatory
Problem 511: Giant Gas Cloud in System NGC 6240
Students use scientific notation and volume of sphere to estimate the density of the gas cloud,
and the number of hydrogen atoms per cubic meter.
[Grade: 8-10 | Topics:Volume of a sphere; scientific notation; unit conversion ]
(PDF)
Problem 439: Chandra Sees a Distant Planet Evaporating
The planet CoRot2b is losing mass at a rate of 5 million tons per second. Students estimate how long it will
take for the planet to lose its atmosphere
[Grade: 6-8 | Topics: Scientific Notation; RAte = Amount/Time]
(PDF)
Problem 417: Estimating the Size and Mass of a Black Hole Students use a simple formula to estimate the size of a black hole located 3.8 billion light years from Earth, recently studied by NASA's Chandra and Swift satellites. [Grade: 8-10 | Topics: distance=speed x time] (PDF)
Problem 398: The Crab Nebula - Exploring a pulsar up close! Students work with a photograph to determine its scale and the time taken by light and matter to reach a specified distance. [Grade: 6-8 | Topics: Scale drawings; unit conversion; distance = speed x time] (PDF)
Problem 390: X-rays from hot gases near the black hole SN1979c Students use two functions to estimate the size of a black hole from the gas emitting x-rays which is flowing into it. [Grade: 8-10 | Topics: Functions; substitution; evaluation] (PDF)
Problem 389: Estimating the diameter of the SN1979c black hole Students use simple equations to learn about the various definitions for the sizes of black holes in terms of their event horizons, last photon orbit, and last stable particle orbit radii, and apply this to the recently discovered 'baby' black hole in the galaxy M-100 [Grade: 6-8 | Topics: evaluating linear functions; integer math; metric units] (PDF)
Problem 314: Chandra Studies an Expanding Supernova Shell Using a millimeter ruler and a sequence of images of a gaseous shell between 2000 and 2005, students calculate the speed of the material ejected by Supernova 1987A. [Grade: 6-9 | Topics: Measuring; Metric Units; speed=distance/time]
Problem 289: Chandra Spies the Longest Sound Wave in the Universe Students use an image of sound waves produced by a massive black hole to determine wavelength, and comparisons with musical scale to find how many octaves this sound wave is below the wavelength of middle-C. [Grade: 6-8 | Topics: metric measurement; scaling; Scientific Notation; exponents]
Problem 285: Chandra Sees the Most Distant Cluster in the Universe Students work with kinetic energy and escape velocity to determine the mass of a distant cluster of galaxies by using information about its x-ray light emissions. [Grade: 9-12 | Topics: Algebra I; Solving for X; Scientific notation]
Problem 283: Chandra Observatory Sees the Atmosphere of a Neutron Star Students determine the mass of the carbon atmosphere of the neutron star Cas-A. [Grade: 8-10 | Topics: Volume of spherical shell; mass = density x volume]
Problem 234: The Hand of Chandra Students use an image from the Chandra Observatory to measure a pulsar ejecting a cloud of gas. [Grade: 6-8 | Topics: Scientific Notation; proportions; angle measure]
Problem 144: Exploring Angular Size Students examine the concept of angular size and how it relates to the physical size of an object and its distance. A Chandra Satellite x-ray image of the star cluster NGC-6266 is used, along with its distance, to determine how far apart the stars are based on their angular separations. [Grade: 7 - 10 | Topics:Scientific Notation; degree measurement; physical size=distance x angular size.]
Dawn
Problem 434: Dawn Spacecraft Sees Asteroid Vesta Up-Close!
Students use an image of the asteroid to determine the diameters of craters
and mountains using a millimeter ruler and the scale of the image in meters per millimeter.
[Grade: 6-8 | Topics: scale, metric measurement]
(PDF)
Problem 210: The Mathematics of Ion Rocket Engines Students learn about the basic physics of ion engines, calculating speeds. [Grade: 9-12| Topics: Scientific Notation; Algebra II; evaluating formulae.]
Problem 202: The Dawn Mission - Ion Rockets and Spiral Orbits Students determine the shape of the trajectory taken by a spacecraft using a constant-thrust ion motor using differential and integral calculus for arc lengths. [Grade: 9-12| Topics: Calculus - Arc lengths.]
Deep Impact - EPOXI
Problem 387: A Mathematical Model of Water Loss from Comet Tempel-1 Students use data from the Deep Impact spacecraft to create a simple empirical model for predicting the rate of water loss from a comet based on actual data. [Grade: 8-10 | Topics: graphing; fitting a parabola to data; evaluating functions] (PDF)
Problem 383: Estimating the mass of Comet Hartley 2 using calculus.
Students use a recent image of the nucleus of Comet Hartley 2 taken by the Deep Impact/EPOXI camera and a shape function described
by a fourth-order polynomial to calculate the volume of the comet's head using integral calculus.
to estimate the volume of the comets nucleus, and its total mass,
[Grade: 12 | Topics: Volume integral using disk method; scale model; scientific notation; unit conversion]
(PDF)
Problem 382: Estimating the mass and volume of Comet Hartley 2.
Students use a recent image of the nucleus of Comet Hartley 2 taken by the Deep Impact/EPOXI camera and a simple geometric 'dumbell'
model based on a cylinder and two spheres, to estimate the volume of the comets nucleus, and its total mass.
[Grade: 8-10 | Topics: volume of a sphere and cylinder; scale model; scientific notation; unit conversion]
(PDF)
Problem 374: Deep Impact - Closing In on Comet 103P/Hartley 2
Students use the Tangent formula to figure out the angular size of the comet at closest approach, and the scale of the HRI camera image.
[Grade: 8-10 | Topics: Scaled images; trigonometry; angle measure]
(PDF)
Problem 324: Deep Impact Comet Flyby The Deep Impact spacecraft flew by the Comet Tempel-1 in 2005. Students determine the form of a function that predicts the changing apparent size of the comet as viewed from the spacecraft along its trajectory. [Grade: 9-12 | Topics: Algebra, geometry, differential calculus]
Problem 277: Deep Impact Comet Encounter Students learn about the Deep Impact experiment involving Comet Tempel-1, and how the path of an asteroid can be changed by using the Law of Conservation of Momentum. [Grade: 10-12 | Topics: Algebra; Scientific Notation; distance = speedxtime]
Problem 275: Water on the Moon! Students estimate the amount of water on the moon using data from Deep Impact/EPOXI and NASA's Moon Minerology Mapper experiment on the Chandrayaan-1 spacecraft. [Grade: 8-10 | Topics: Geometry, Spherical volumes and surface areas, Scientific notation]
Problem 255: Tempel-1 - Closeup of a Comet Students examine an image of the Comet Tempel-1 taken by the Deep Impact spacecraft to determine feature sizes and other details. [Grade: 6-8 | Topics: scales, proportions ]
Fermi Gamma-Ray Observatory
Problem 513: The Remarkable Gamma Ray Burst GRB 130427A
Students work with the surface area of a sphere, metric conversions and scientific
notation to calculate the total power of this distant supernova event.
[Grade: 8-10 | Topics: surface area of sphere; scientific notation]
(PDF)
Problem 503: The Origin of Cosmic Rays
Students explore the Fermi Gamma-Ray Observatory's confirmation of the idea that supernova are the sources of cosmic rays in the Milky Way. They use a simple model to estimate how many supernova are needed to account for the current number of cosmic rays in the galaxy.
[Grade: 8-10 | Topics: percercentages, scientific notation; volume of a disk]
(PDF)
Problem 460: Fermi Explores the High-Energy Universe
Students work with percentages to explore the identities of the 1873 gamma-ray sources detected by NASAs Fermi Observatory
[Grade: 6-8 | Topics: percentages; pie graphs]
(PDF)
Problem 330: Fermi Detects Gamma-rays from the Galaxy Messier-82 Based on a recent press release, students work with a log-log plot to show that straight lines on this plot represent power-law functions. They use this fact to determine, by interpolation, the strength of the gamma-rays from this galaxy. [Grade: 10-12 | Topics: power-laws; log-log graphing; linear regression]
Problem 288: Fermi Observatory Measures the Lumps in Space Students use timing data obtained by the Fermi Observatory of a powerful gamma-ray burst 10 billion light years away, to determine how lumpy space is based on travel time delays between the lowest and highest-energy gamma-rays. [Grade: 9-12 | Topics: Scientific Notation; Evaluating an equation with multiple factors]
Galaxy Evolution Explorer (GALEX)
Problem 111: A Star Sheds a Comet Tail! The GALEX satellite captured a spectacular image of the star Mira shedding a tail of gas and dust nearly 13 light years long. Students use the GALEX image to determine the speed of the star, and to translate the tail structures into a timeline extending to 30,000 years ago. [Grade: 8-10 | Topics:Image scaling; Unit conversion; Calculating speed from distance and time]
Grail Ebb and Flo - Mapping lunar gravity
Problem 509:Gail Spacecraft Creates a New Crater on the Moon
Students work with images of the Grail impact sites to estimate the diameter of the crater created
after the spacecraft impacted the moon.
[Grade: 6-8 | Topics: scale and proportion; volume of cylinder; mass=DensityxVolume]
(PDF)
Problem 504: Grail Satellites Create a Gravity Map of the Moon
Students explore the gravity field of the moon, and the behavior of simple pendulum clocks in places on the moon where the local gravity is slightly different.
[Grade: 9-12 | Topics: square-roots; evaluating equations]
(PDF)
Problem 478: The Grail and LRO Encounter in Lunar Orbit
Students explore the May 31, 2012 encounter between NASA's Grail and LRO spacecraft in orbit around the moon. Will the Grail/Ebb spacecraft be able to photograph the LRO spacecraft as it passes-by?
[Grade: 9-12 | Topics: formula for an ellipse; semi-major and minor axis]
(PDF)
Gravity Probe - B (GP-B)
Problem 421: The Lense-Thirring Effect Near the Sun and a Neutron Star Students work with a formula for the Lense-Thirring Effect and estimate how large it will be in orbit around our sun, and in the intense gravitational field of a dense neutron star. [Grade: 9-12 | Topics: algebra; scientific notation, angular measure] (PDF)
Problem 420: Gravity Probe B: Testing Einstein again! Students learn about the Lense-Thirring Effect, and calculate its magnitude near Earth's orbit using an algebraic equation with integer and fractional exponents. [Grade: 9-12 | Topics: algebra; scientific notation, angular measure] (PDF)
Hinode Solar Observatory
Problem 362: Hinode Discovers the Origin of White Light Flares
A study of the magnetic energy of a flare[Grade: 9-12 | Topics: Image scale; Algebra; Scientific Notation]
(PDF)
Problem 105: The Transit of Mercury As seen from Earth, the planet Mercury occasionally passes across the face of the sun; an event that astronomers call a transit. From images taken by the Hinode satellite, students will create a model of the solar disk to the same scale as the image, and calculate the distance to the sun. [Grade: 9-11 | Topics:image scales; angular measure; degrees, minutes and seconds]
Problem 104: Loopy Sunspots! Students will analyze data from the Hinode satellite to determine the volume and mass of a magnetic loop above a sunspot. From the calculated volume, based on the formula for the volume of a cylinder, they will use the density of the plasma determined by the Hinode satellite to determine the mass in tons of the magnetically trapped material. [Grade: 9-11 | Topics:image scales; cylinder volume calculation; scientific notation; unit conversions]
Problem 103: The Mysterious Solar Micro-Flares! Students will analyze an image taken by the Hinode solar satellite to determine the scale of the image in kilometers per millimeter, then use this to determine the sizes of solar micro-flares. From the number of micro-flares that they count in the image, the area of the image in square kilometers, and the surface area of a spherical sun, they will calculate the total number of micro-flares on the solar surface. [Grade: 6-9 | Topics:image scales; area calculation; unit conversions]
Problem 102: How fast does the sun rotate? Students will analyze consecutive images taken by the Hinode satellite to determine the sun's speed of rotation, and the approximate length of its 'day'. [Grade: 6-9 | Topics:image scales; time calculations; speed calculations, unit conversions]
Problem 99: The Hinode Satellite Views the Sun Students will use a full-sun image from the new Hinode satellite to sketch the locations of magnetic fields on the sun's surface using information in the introductory article as a guide. [Grade level: 6-8 | Topics:image interpretation; eye-hand coordination; reading to be informed]
Problem 97: Hinode - Closeup of a Sunspot Students will determine the sizes of sunspots and solar granulation cells from a recent image taken by the Hinode solar observatory. [Grade level: 6-8 | Topics:image scales, metric units, unit conversion]
Problem 96: Hinode Satellite Power Students will study the design of the Hinode solar satellite and calculate how much power it can generate from its solar panels. [Grade level: 6-8 | Topics:area of rectangle,area of cylinder, unit conversion]
Problem 85: The Solar Tsunami! Recent data from the Hinode satellite is used to measure the speed of a solar explosion on the surface of the sun using a series of images taken by the satellite at three different times. Students calculate the speed of the blast between the first pair and last pair of images, and determine if the blast wave was accelerating or decellerating in time. [Grade level: 5-8 | Topics: Finding image scale; calculating time differences; calculating speed from distance and time]
Hubble Space Telescope
Problem 501: Exploring the Most Distant Galaxies with Hubble
Students use recent Hubble Extreme Deep Field data and a polynomial to determine the light travel time between distant galaxies and Earth.
[Grade: 11-12 | Topics: polynomials; linearization]
(PDF)
Problem 490: LL Pegasi - A Perfect Spiral in Space
The star LL Persei is ejecting gas like a sprinkler on a lawn. Every 800 years the gas makes one complete
orbit, and over time forms a spiral patteri in space. Students explore the timing of this pattern and estimate the size and age of this gas.
[Grade: 6-8 | Topics: Distance = speed x time; unit conversions; evaluating formulas ]
(PDF)
Problem 487: The Hubble eXtreme Deep Field
Students use the Hubble XDF to estimate the number of galaxies in the visible universe.
[Grade: 6-8 | Topics: Counting, areas, proportions ]
(PDF)
Problem 481: Pluto's Fifth Moon
Students explore Kepler's Third Law and estimate the orbit period of a hypothetical sixth moon using the distance:period law.
They also determine the mass of Pluto using the orbit data, including the recently discovered fifth moon (P5) of Pluto by the Hubble Space Telescope.
[Grade: 9-12 | Topics: Power functions; integer exponents; Scientific Notation; tabular data]
(PDF)
Problem 480: The Expanding Gas Shell of U Camelopardalis
Students explore the expanding U Camelopardalis gas shell imaged by the Hubble Space Telescope, to determine its age and the density of its gas.
[Grade: 6-8 | Topics: Scientific Notation; distance = speed x time; density=mass/volume ]
(PDF)
Problem 399: A Galactic City in the Far Reaches of the Universe Students work with an image of a distant cluster of galaxies to determine its scale compared to nearby galaxies. [Grade: 6-8 | Topics: Scale; proportion; metric measurement; unit conversion] (PDF)
Problem 395: Death Stars Some stars create super-flares that are capable of eliminating life on planets that orbit close to the star. Students learn about these flares on common red-dwarf stars and compare them to flares on our own sun [Grade: 6-9 | Topics: Scientific Notation; percentages; rates of change] (PDF)
Problem 388: Hubble Detects More Dark Matter
Students learn about how astronomers estimate the amount of invisible dark matter in a cluster of galaxies by comparing its visible mass against the speeds of the galaxies to 'weigh' the cluster'
[Grade: 8-10 | Topics: evaluating functions; Scientific notation]
(PDF)
Problem 364: The Cometary Planet HD209458b
Problem 363: Celestial Fireworks Near NGC3603
Problem 344: Hubble Spies an Asteroid - Yes it does move!
Problem 333: Hubble: Seeing a Dwarf Planet Clearly Based on a recent press release, students use the published photos to determine the sizes of the smallest discernible features and compare them to the sizes of the 48-states in the USA.
They also estimate the density of Pluto and compare this to densities of familiar substances to create a 'model' of Pluto's composition.
A supplementary Inquiry Problem asks students to model the interior in terms of two
components and estimate what fraction of Pluto is composed of rock or ice.
[Grade: 8-12 | Topics: scales and ratios; volume of sphere; density=mass/volume]
Problem 332: Hubble: The Changing Atmosphere of Pluto Based on a recent press release, students determine the aphelion and perihelion of Pluto's elliptical orbit using the properties of ellipses, then
calculate the temperature of Pluto at these distances to estimate the thickness of Pluto's atmosphere and its changes during its orbit around the sun.
[Grade: 10-12 | Topics: properties of ellipses; evaluating an algebraic function ]
Problem 329: WISE and Hubble: Power Functions: A question of magnitude Students explore the function F(x) = 10^-ax and learn about the stellar magnitude scale used by astronomers to rank the brightness of stars.
[Grade: 10-12 | Topics: base-10, evaluating power functions ]
Problem 326: Hubble Spies Colliding Asteroids Based on a recent press release, students calculate how often asteroids collide in the Asteroid belt using a simple formula. Students
estimate belt volume, and asteroid speeds to determine the number of years between collisions. They also investigate how
the collision time depends on the particular assumptions they made. An 'extra' integration problem is also provided for calculus students.
[Grade: 8-12 | Topics: Volume of a thin disk; Algebra 1; Evaluating a definite integral; power-law]
Problem 316: Counting Craters on the Hubble Space Telescope Students count craters on a piece of the Wide Field Planetary
Camera recovered from the Hubble Space Telescope in 2009. They determine the cratering rate and use this to predict
how many impacts the solar panels on the International Space Station experiences each day.
[Grade: 6-9 | Topics: Counting; Area; density]
Problem 295: Details from an Exploding Star Students work with an image from the Hubble Space Telescope of the Crab Nebula to calculate scales and sizes of various features.
[Grade: 6-9 | Topics: Scale; measurement; metric units]
Problem 240: The Eagle Nebula Close-up Students measure a Hubble image of the famous Eagle Nebula 'Pillars of Creation' to determine the sizes of
arious features compared to our solar system
[Grade: 8-10 | Topics: scale, proportion, angle measure]
Problem 239: Counting Galaxies with the Hubble Space Telescope Students use an image of a small area of the sky to estimate the total number of galaxies in the universe visible from Earth.
[Grade: 8-10 | Topics: area, angular measure]
Problem 238: Satellite Drag and the Hubble Space Telescope Satellite experience drag with the atmosphere, which eventually causes them to burn up in the atmosphere. Students study
various forecasts of the altitude of the Hubble Space Telescope to estimate its re-entry year.
[Grade: 8-10 | Topics: interpreting graphical data; predicting trends]
Problem 197: Hubble Sees a Distant Planet Students study an image of the dust disk around the star Fomalhaut and determine the orbit period and distance of a newly-discoveblack planet orbiting this young star.
[Grade: 6-10| Topics: Calculating image scales; Circle circumferences; Unit conversions; distance-speed-time]
Problem 122: XZ Tauri's Super CME!
Ordinarily, the SOHO satellite and NASA's STEREO mission spot coronal
mass ejections (CMEs) but the Hubble Space Telescope has also spotted a few of its own...on distant stars! Students will
examine a sequence of images of the young star XZ Tauri, and measure the average
speed and density of this star's CME event between 1955 and 2000.
[Grade: 8-10 | Topics:Calculate image scale; speed
from distance and time; mass:volume:density]
Problem 49: A Spiral Galaxy Up Close.
Astronomers can learn a lot from studying photographs of galaxies. In
this activity, students will compute the image scale (light years per millimeter) in a
photograph of a nearby spiral galaxy, and explore the sizes of the features found in the image. They
will also use the internet or other resources to fill-in the missing background information about this galaxy.
[Grade level: 6-8 | Topics: Online research; Finding the scale of an image; metric measurement; decimal math]
Problem 274: IBEX Uses Fast-moving Particles to Map the Sky! Students learn about Kinetic Energy and how particle energies and speeds are related to each other in a simple formula,
which they use to derive the speed of the particles detected by the IBEX satellite.
[Grade: 8-10 | Topics: Algebra I, Scientific notation]
Problem 273: IBEX Creates an Unusual Image of the Sky Students create an image of the sky by using a Bingo-like technique of tallying particles in
various sky directions using a simple 5x5 grid.
[Grade: 6-8 | Topics: Counting, tallying]
Problem 114: The Heliopause...a question of balance
Students will learn about the concept of pressure equilibrium
by studying a simple mathematical model
for the sun's heliopause located beyond the orbit of Pluto. They will calculate the distance to the
heliopause by solving for 'R' and then using an Excel spreadsheet
to examine how changes in solar wind density, speed and interstellar gas density relate to
the values for R.
[Grade: 8-10 | Topics: Formulas with two variables; scientific notation; spreadsheet programming]
Problem 41: Solar Energy in Space Students will calculate the area of a satellite's surface
being used for solar cells from an actual photo of the IMAGE satellite.
They will calculate the electrical power provided by this one panel. Students
will have to calculate the area of an irregular region using nested rectangles.
[Grade level: 7-10 | Topics: Area of an irregular polygon; decimal math]
Problem 35: Exploring the Plasmasphere Students use an image of the plasmasphere obtained
by the IMAGE satellite to calculate how fast it orbits the Earth. They
will use this to determine whether gravity or Earth's magnetic field
provides the forces responsible for its movement through space.
[Grade: 7 - 9 | Topics: Geometry; ratios; decimal math; time arithmetic]
Problem 25: The Distance to Earth's Magnetopause Students use an algebraic formula and some real
data, to calculate the distance from Earth to the magnetopause, where
solar wind and magnetosphere pressure are in balance.
[Grade: 8 - 10 | Topics: Evaluating a function with two variables; completing tabular entries]
Problem 22: The Auroral Oval Students learn that the aurora are observed as two
'halos' of light encircling the North and South Poles. Students use
measurements made from two satellite images of the 'auroral ovals' to
determine the diameter of the rings, and their approximate geographic
centers - which are not at the geographic poles!
[Grade: 5 - 7 | Topics: Finding the scale of an image; measurement; decimal math]
Problem 21: Exploring the Plasmasphere Students learn that the Pythagorean Theorem is more
than a geometric concept. Scientists use a photograph taklen by the IMAGE
satellite to measure the size of Earth's plasmasphere region using a ruler
and protractor.
[Grade: 7 - 9 | Topics: Finding the scale of an image; decimal math; measurement]
Problem 15: Radio Plasma Imaging with IMAGE Students use the Distance=VelocityxTime relationship
to determine the distances to plasma clouds seen by the IMAGE satellite.
[Grade: 6 - 8 | Topics: Polar graphs; time = distance x speed; decimal math]
Problem 13: Plasma Clouds
Students use a simple 'square-root' relationship to learn how scientists
with the IMAGE satellite measure the density of clouds of plasma in space.
[Grade: 7 - 9 | Topics: Square-root; solving for X; evaluating a function]
Problem 12: The Ring Current Students use the formula for a disk to calculate the
mass of the ring current surrounding Earth.
[Grade: 7 - 9 | Topics: Volume of a disk; scientific notation; mass = density x volume]
Problem 527:Exploring a Possible InSight Landing Area on Mars
Problem 526:Comparing the InSight Landing Area to a City Block!
Problem 525:Exploring Marsquake Energy with the Moment Magnitude Scale
Problem 524:Exploring Logarithms and the Richter Magnitude Scale
Problem 523:The Distance to the Martian Horizon
Problem 522:Exploring the Interior of Mars with Spheres and Shells
Problem 521:Exploring the Mass of Mars
Problem 520:Exploring Impacts and Quakes on Mars
Problem 519:Comparing the Heat Output of Mars and Earth
Problem 518:Exploring Heat Flow and Insulation
Problem 517:Exploring Temperature Change in Earth’s Outer Crust
Problem 516:Exploring the InSight Lander Telemetry Data Flow
Problem 515:Seeing the Martian Surface with IDC
Problem 514:Telling Time on Mars - Earth Days and Mars Sols
Problem 513:Radio Communications with Earth – The Earth-Sun Angle
Problem 512:Estimating the Mass of a Martian Dust Devil!
Problem 511:The Work Area In Front of the Lander
Problem 510:Scheduling Events in Time for Launch
Problem 509:The InSight Seismographic Station Solar Power System
Problem 508: The InSight Seismographic Station - Wave arrival times
Problem 472: Investigating Juno's Elliptical Transfer Orbit
Problem 471: Investigating the Launch of the Juno Spacecraft
Problem 470: The Launch of the Juno Spacecraft - Ascent to orbit
Problem 469: Solar Energy and the Distance of Juno from the Sun
Problem 465: Comparing Planets Orbiting other Stars
Problem 458: Playing Baseball on the Earth-like Planet Kepler-22b!
Problem 444: Predicting the Transits of the Stars Kepler-16A and 16B from Tatooine - II
Problem 443: Predicting the Transits of the Stars Kepler-16A and 16B from Tatooine - I
Problem 441: Exploring the new planet Kepler 16b called 'Tatooine'
Problem 416: Kepler probes the interior of red giant stars
Students use the properties of circular arcs to explore sound waves inside stars.
[Grade: 8-10 | Topics: geometry of circles and arcs; distance=speed x time]
(PDF)
Problem 403: The Goldilocks Planets - Not too hot or cold
Students use a table of the planets discovered by the Kepler satellite, and estimate the number of planets in our Milky Way galaxy that are about the same size as Earth and located in their Habitable Zones.
They estimate the average temperature of the planets, and study their tabulated properties using histograms.
[Grade: 6-8 | Topics: Averaging; histogramming]
(PDF)
Problem 402: Kepler- Earth-like planets by the score! II
Students use recent Kepler satellite data summarized in tabular form to estimate the number of planets in the Milky Way galaxy
that are about the same size as our Earth, and located in their Habitable Zones were liquid water may exist.
[Grade: 6-8 | Topics: Percentage; re-scaling sample sizes]
(PDF)
Problem 401: Kepler - Earth-like planets by the score! I
Students use recent Kepler satellite data to estimate the number of Earth-like planets in the Milky Way galaxy.
[Grade: 6-8 | Topics: Percentage; histograms; Re-scaling sample sizes]
(PDF)
Problem 400: The Most Distant Objects in the Universe
Students use a tabels of the most distant known events and objects in the universe to create a timeline of the universe soon after the Big Bang.
[Grade: 6-8 | Topics: Working with millions and billions; elapsed time]
(PDF)
Problem 396: Kepler 10b - A matter of gravity
Students use the measured properties of the Earth-like planet Kepler 10b to estimate the weight of a human on its surface.
[Grade: 8-10 | Topics: Evaluating formulas; mass = density x volume; volume of a sphere; scientific notation]
(PDF)
Problem 360: Kepler's First Look at 700 Transiting Planets
Problem 325: Kepler Spies Five New Planets Students count squares on a Bizarro Star to study the transit of a planet, and determine the diameter of the planet.
This demonstrates the basic principle used by NASA's Kepler satellite to search for Earth-sized planets orbiting distant stars.
[Grade: 4-6 | Topics: Counting; graphing; area of a square]
Problem 225: Areas Under Curves; An astronomical perspective Students work with a bar graph of the number of planet discoveries since 1995 to evaluate the total
discoveries, as areas under the graph, for various combinations of time periods.
[Grade: 6-8 | Topics: Adding areas in bar graphs.]
Problem 213: Kepler: The hunt for Earth-like planets Students compare the area of a star with the area of a planet to determine how the star's light
is dimmed when the planet passes across the star as viewed from Earth. This is the basis for the 'transit'
method used by NASA's Kepler satellite to detect new planets.
[Grade: 6-8 | Topics: Area of circle; ratios; percents.]
Problem 512: New NASA Satellite Takes Pictures of Salton Sea
Problem 484: Exploring Water Use in Kansas
Problem 129: How Big is It? - The Moon up close.
Students work with an image taken by the Lunar Orbiter III spacecraft
to determine image scale, and search for the smallest things seen in a photograph.
[Grade: 4 - 7 | Topics:image scaling; multiply, divide, work with millimeter ruler]
Problem 127: How Big is It? - The Moon up close.
Students work with an image taken by the Lunar Orbiter IV spacecraft
to determine image scale, and search for the smallest things seen in a photograph.
[Grade: 4 - 7 | Topics:image scaling; multiply, divide, work with millimeter ruler]
Problem 445: LRO - The relative ages of lunar surfaces
Problem 440: LRO explores the Apollo 12 landing area on the moon
Problem 378: LRO Makes a Temperature Map of the Lunar South Pole
Problem 372: LRO Determines Lunar Cratering History
Problem 321: Lunar Crater Frequency Distributions Students use an image from the LRO satellite of the Apollo-11 landing area, along with a power-law
model of cratering, to determine what fraction of the landin garea was safe to land upon.
[Grade: 11-12 | Topics: Integral calculus]
Problem 290: The Apollo-11 Landing Area at High Resolution Students use recent images made by the LRO satellite to estimate distances, crater sizes, and how many tons of
TNT were needed to create some of the craters by meteor impact.
[Grade: 9-12 | Topics: metric measurement; scaling; A = B/C]
Problem 287: LCROSS Sees Water on the Moon Students use information about the plume created by the LCROSS impactor to estimate the (lower-limit) concentration of
water in the lunar regolith in a shadowed crater.
[Grade: 9-12 | Topics: Geometry; volumes; mass=density x volume]
Problem 262: LRO Explores Lunar Surface Cratering Students count the number of craters in various size ranges from a high-resolution image of the lunar surface.
[Grade: 6-8 | Topics: scale, proportion, ratio, area, density]
Problem 261: LRO - Searching for Lunar Boulders Students use a recent image of the Apollo-11 landing area to search for large lunar boulders.
[Grade: 6-8 | Topics: scale, ratio, proportion]
Problem 259: Mare Nubium And Las Vegas Students compare two satellite images taken at the same resolution to appreciate how large lunar features ae compared to more familiar objects.
[Grade: 8-10 | Topics: scale, proportion, ratio]
Problem 258: LRO's First Image of Mare Nubium Students examine the first image of this lunar region using the high-resolution camera image provided by the Lunar Reconnaissance Orbiter.
[Grade: 6-8 | Topics: scale, ratio, proportion]
Problem 257: LRO and the Apollo-11 Landing Site Students examine a map of the Apollo-11 landing area and determine how well various features
will be visible to the Lunar Reconnaissance Orbiter high-resolution camera.
[Grade: 6-8 | Topics: scale, proportion, ratios]
Problem 236: LRO Sees Apollo-11 on the Moon! Students use the latest image from the Lunar Reconnaissance Orbiter of the Apollo-11 landing
site to explore lunar features at 1-meter resolution, and determine the solar elevation angle.
[Grade: 6-8 | Topics: scale; ratios; angle measure; right triangles]
Problem 507: Exploring the Launch of the Falcon 9
Problem 476: SpaceX launches the First Commercial Rocket to the ISS
Problem 459: A piece of history - space shuttle thermal tiles
Problem 438: The Last Flight of the Space Shuttle Endeavor
Problem 437: Saturn V Rocket Launch Speed and Height
Problem 436: Space Shuttle Challenger Deploys the INSAT-1B Satellite
Problem 435: Apollo-17 Launch from Lunar Surface
Problem 433: Space Shuttle Atlantis - Plume Speed
Problem 432: Space Shuttle Atlantis - Exhaust Speed
Problem 431: Space Shuttle Atlantis - Launch Speed
Problem 430: Space Shuttle Atlantis - Ascent to Orbit
Problem 419: The Space Shuttle: Fly me to the moon?
Students discuss the popular misconception that the Space Shuttle can travel to the moon by examining the required orbit speed change and the capacity of the Shuttle engines to provide the necessary speed changes.
[Grade: 6-8 | Topics: amount = rate x time ]
(PDF)
Problem 394: Apollo: Probing the lunar core using seismology
Students learn about the geometry needed to determine the diameter of the lunar core using a simplified model.
[Grade: 9-10 | Topics: Geometry; Properties of Inscribed Arcs]
(PDF)
Problem 346: The International Space Station and a Sunspot: Exploring angular scales
Problem 282: Exploring the Ares 1-X Launch: The Hard Climb to Orbit Students learn about the energy required to send a payload into orbit by studying the Ares 1-X rocket launch.
[Grade: 8-10 | Topics: Algebra II]
Problem 281: Exploring the Ares 1-X Launch: Energy Changes Students learn about kinetic and potential energy while studying the Ares 1-X rocket launch.
[Grade: 8-10 | Topics: Algebra II]
Problem 280: Exploring the Ares 1-X Launch: Parametrics Students learn about parametric equations to determine the path of the Ares 1-X rocket.
[Grade: 8-10 | Topics: Algebra II; Parametric Equations]
Problem 279: Exploring the Ares 1-X Launch: Downrange Distance Students learn about the path of the Ares 1-X test launch and calculate its downrange landing distance in the Atlantic Ocean.
[Grade: 8-10 | Topics: Algebra; Significant Figures; Metric to English Conversion]
Problem 276: Solid Rocket Boosters and Thrust Students learn how solid rocket boosters work, and calculate the SRB Thrust Curve using a simple geometric model
and 'counting squares'..
[Grade: 8-10 | Topics: Geometry, Cylindrical volumes and surface areas, Graphing data]
Problem 266: The Ares-V Cargo Rocket Students work with the equations for thrust and fuel loss to determine the acceleration curve of the Ares-v during launch.
[Grade: 11-12 | Topics: Algebra II, properties of functions, differential calculus, Excel Spreadsheet]
Problem 245: Solid Rocket Boosters Students learn how SRBs actually create thrust, and study the Ares-V booster to estimate its thrust.
[Grade: 8-10 | Topics: volume, area, unit conversions]
Problem 243: ISS - Orbit Altitude Changes Students read an essay describing the increases and decreases in the International Space Station orbit, and
calculate the final orbit altitude after all the changes are applied.
[Grade: 8-10 | Topics: combining positive and negative mixed numbers; fractions]
Problem 196: Angular Size and velocity Students study a spectacular photo of the ISS passing across the face of the sun, and work out the angular sizes and speeds of the transit to figure out how long the event took in order to photograph it.
[Grade: 8-10| Topics: Geometry; Angle measurement]
Problem 185: The International Space Station: Follow that graph! Students use a plot of the orbit altitude of the ISS to pblackict its re-entry year after the peak of the next solar activity cycle.
[Grade: 6-8| Topics: extrapolating a simple graph; estimation; forecasting]
Problem 125: How Big is It? - Washington DC up close.
Students work with an image taken by ISS astronauts to determine image scale, and search for the smallest things seen in a photograph.
[Grade: 4 - 7 | Topics:image scaling; multiply, divide, work with millimeter ruler]
Problem 95: A Study on Astronaut Radiation Dosages in Space
Students will examine a graph of the astronaut radiation dosages for Space Shuttle flights, and estimate the
total dosages for astronauts working on the International Space Station.
[Grade level: 9-11 | Topics:Graph analysis, interpolation, unit conversion]
Problem 36: The Space Station Orbit Decay and Space
Weather Students will learn about
the continued decay of the orbit of the International Space Station by
studying a graph of the Station's altitude versus time. They will
calculate the orbit decay rates, and investigate why this might be
happening. [Grade: 5 - 8 | Topics: Interpreting graphical data; decimal math]
Problem 113: NASA Juggles Four Satellites at Once!
Students will learn about NASA's Magnetospheric Multi-Scale (MMS) satellite mission, and how
it will use four satellites flying in formation to investigate the mysterious process
called Magnetic Reconnection that causes changes in Earth's magnetic field. These changes
lead to the production of
the Northern and Southern Lights and other phenomena. From the volume formula for a tetrahedron, they will calculate the volume of several satellite configurations
and estimate the magnetic energy and travel times for the particles being studied by MMS.
[Grade: 8-10 | Topics: Formulas with two variables; scientific notation]
Problem 500: Curiosity Uses X-Ray DIffraction to Identify Minerals on Mars
Problem 491: The Curiosity Rover on the Move.
Problem 485: Curiosity Discovers Ancient Mars River
Problem 479: Exploring Gale Crater with the Curiosity Rover
Problem 457: The Interplanetary Voyage of MSL
Problem 456: The Launch of the Mars Science Laboratory (MSL) in 2011
Problem 393: Taking a stroll around a martian crater!
Students use a recent photograph of a crater on Mars to estimate its circumference and the time it will take NASAs Opportunity Rover to travel once around its edge.
[Grade: 6-8 | Topics: scale model; distance = speedxtime; metric measure]
(PDF)
Problem 237: The Martian Dust Devils Students determine the speed and acceleration of a martian dust devil from time laps images and information about the scale of the image.
[Grade: 6-8 | Topics: scales; Determining speed from sequential images; V = D/T
Problem 139: How Big Is It? - Mars
Students use an image of a crater wall on mars to investigate ancient
water gullies discovered in 2008 by the Mars Orbiter.
[Grade: 4 - 7 | Topics:image scales; metric measurement; division and multiplication; decimals]
Problem 133: How Big is It? - The Mars Rover.
Students work with an image taken by the Mars Orbiter
satellite of the Spirit landing site. They
determine the image scale, and calculate the sizes of various surface features from the image.
[Grade: 4 - 7 | Topics:image scaling; multiply, divide, work with millimeter ruler]
Problem 126: How Big is It? - A Martian Avalanche!
Students work with a Mars reconnissance Orbiter image to determine image scale, and search for
the smallest things seen in a photograph.This avalanche was caught as it occurred on February 19, 2008!
[Grade: 4 - 7 | Topics:image scaling; multiply, divide, work with millimeter ruler]
Problem 74: A Hot Time on Mars
The NASA Mars Radiation Environment (MARIE) experiment has created a map of the surface of mars, and measu black the ground-level radiation background that astronauts would be exposed to.
This math problem lets students examine the total radiation dosage that these explorers would receive on a series of 1000 km journeys across the martian
surface. The students will compare this dosage to typical background conditions on earth and in the International Space Station to get a sense of perspective
[Grade level: 6-8 | Topics: decimals, unit conversion, graphing and analysis ]
Problem 70: Calculating Total Radiation Dosages at Mars
This problem uses data from the Mars Radiation Environment Experiment (MARIE) which is orbiting Mars, and measures the daily radiation dosage
that an astronaut would experience in orbit around Mars. Students will use actual plotted data to calculate the total dosage by adding up the areas under the data curve. This
requires knowledge of the area of a rectangle, and an appreciation of the fact that the product of a rate (rems per day) times the time duration (days) gives a total dose (Rems), much like the product of speed times time gives distance.
Both represent the areas under their appropriate curves. Students will calculate the dosages for cosmic radiation and solar proton flares, and decide which component produces the most severe radiation problem.
[Grade level: 6-8 | Topics: decimals, area of rectangle, graph analysis]
Problem 474: MESSENGER Explores the Interior of Mercury
Problem 473: MESSENGER Explores the Mass of Mercury
Problem 415: Mercury and the Moon - Similar but different
Students explore the mass and volume of mercury compared to the moon by using the formula for a sphere and scale changes.
[Grade: 8-10 | Topics: scale; volume of a sphere; mass = density x volume]
(PDF)
Problem 121: Ice on Mercury?
Since the 1990's, radio astronomers have mapped Mercury.
An outstanding curiosity
is that in the polar regions, some craters appear to have 'anomalous reflectivity' in
the shadowed areas of these craters. One interpretation is that this is caused by
sub-surface ice. The MESSENGER spacecraft hopes to explore this issue in the next few years.
In this activity, students
will measure the surface areas of these potential ice deposits an calculate the
volume of water that they imply.
[Grade: 8-10 | Topics:Area of a circle; volume, density, unit conversion]
Problem 143: So..How big is it? - Asteroid Eros surface
Students calculate the scale of an image of the surface of the asteroid Eros
from the NEAR mission, and
determine how big rocks and boulders are on its surface.
[Grade: 4 - 7 | Topics: Scaling; multiplication, division; metric measure]
Problem 506: A New Belt for the Van Allen Belts
Problem 489: RBSP and the location of Dawn Chorus - III
Problem 488: RBSP and the Location of Dawn Chorus - II
Problem 486: RBSP Hears Dawn Chorus - I
Problem 485: - Estimating the total mass of the van Allen Belts
Students work with the density and volume of the van Allen Belts to estimate their mass
[Grade: 9-12| Topics: mass = density x volume; scientific notation]
Problem 484: - Exploring the donuit-shaped van Allen belts
Students determine the volume of the van Allen belts by using the volume formula for a torus. They compare this volume to that of a spherical earth.
[Grade: 9-12| Topics: Volume of a sphere and torus; scientific notation]
Problem 483: - How to use the RBSP spacecraft to measure the mass of Earth!
Students work with Keplers Third Law to determine the mass of earth by using the orbital data for the RBSP spacecraft.
[Grade: 9-12| Topics: Algebra 1; Re-writing equations;scientific notation ]
Problem 482: - Radiation Belt Storm Probes - Telemetry math
Students work with units of megabytes and gigabytes to determine how much data will be produced by the RBSP spacecraft.
[Grade: 6-8| Topics: giga and mega units; decimal math]
Problem 481: - The RBSP Satellite: Working with octagons
Students determine the surface area of the octagonal spacecraft body.
[Grade: 6-8| Topics: algebra 1; arease of rectangles and triangles; metric math]
Problem 480: - Working with areas of rectangles and circles
Students determine the area of a panel from a spacecraft by subtracting the areas of various holes
from the original panel area, and determine the remaining mass of the panel.
[Grade: 6-8| Topics: areas of rectangles and circles; mass = density x volume]
Problem 479: - Electricity from sunlight: The RBSP solar panels
Students work with a scaled drawing of the RBSP spacecraft to determine the area of its solar panels and how many watts of electricity they can produce.
[Grade: 6-8| Topics: area of rectangles; metric math; decimals]
Problem 204: The Mass of the Van Allen Radiation Belts- Students graph some magnetic field lines in polar coordinates, then estimate the volume and mass of the Belts using the formula for a torus.
[Grade: 9-12| Topics: Algebra II.]
Problem 93 An Introduction to Radiation Shielding -
Students calculate how much shielding a new satellite needs
to replace the ISO research satellite. Students use a graph of the wall thickness versus
dosage, and determine
how thick the walls of a hollow cubical satellite have to be to blackuce the
radiation exposure of its
electronics. Students calculate the mass of the satellite and
the cost savings by using different
shielding.
[Grade level: 9-11 | Topics: Algebra; Volume of a hollow cube; unit conversion]
Problem 71 Are the Van Allen Belts Really Deadly? -
This problem explores the radiation dosages that astronauts would receive as they travel
through the van Allen Belts enroute to the Moon. Students will use data to calculate the duration of the trip through the belts, and the total received dosage, and compare this to a lethal dosage to
confront a misconception that Apollo astronauts would have instantly died on their trip to the Moon.
[Grade level: 8-10 | Topics: decimals, area of rectangle, graph analysis]
Problem 101: Super-Fast Solar Flares!!
Students will analyze consecutive images taken of an erupting solar flare, and use
the information provided to calculate the speed of the flare.
[Grade level: 6-9 | Topics:image scales; time calculations; speed calculations]
Problem 299: Changing Perspectives on the Sun's Diameter Students compare two images of the sun taken by the SOHO satellite to measure the apparent diameter
change from different earth obit locations in the winter and summer.
[Grade: 6-8 | Topics: measurement; parallax; metric units; percentage change]
Problem 244: Solar Storms - Fractions and Percentages Students create a Venn Diagram to summarize data on a series of solar storms, and determine how often solar flares occur
when a solar plasma eruption happens.
[Grade: 4-7 | Topics: precentages; Venn Diagramming]
Problem 176: Solar Storms: Sequences and Probabilities I Students continue their study of a stormy week on the sun by working out the probabilities for joint events.
[Grade: 4-7| Topics: probability; numerating possible outcomes]
Problem 175: Solar Storms: Sequences and Probabilities II Students work out the probabilities for various combinations of solar storms during a given week.
[Grade: 4-7| Topics: probability; numerating possible outcomes]
Problem 117: CME Kinetic Energy and Mass
Coronal Mass Ejections (CMEs) are giant clouds of plasma
released by the sun at millions of kilometers per hour. In this activity, students
calculate the kinetic energy and mass of several CMEs to determine typical mass
ranges and speeds. Students will use the formula for kinetic energy to fill-in
the missing entries
in a table. They will then use the completed table to answer some basic questions
about CMEs.
[Grade: 8-10 | Topics:time calculation; Evaluating a simple equation; solving for variables]
Problem 94 : Solar Storms: Odds, Fractions and Percentages
Students will use actual data on solar storms to learn
about the
different kinds of storms and how common they are. This is a basic science activity that
professionals do in order to look for relationships between different kinds of events
that might
lead to clues about what causes them. Can your students come up with something new that
noone has thought about before? The Venn Diagramming activity is a key element of the activity and is reasonably challenging!
[Grade level: 6-8 | Topics: Averaging; fractions; percentages; odds; Arithmetic Operations; Venn Diagrams]
Problem 80 : Data Corruption by High Energy Particles
Students will see how solar flares can corrupt satellite data, and
create a timeline for a spectacular episode of data loss recorded by the SOHO satellite using
images obtained by the satellite. Students will also calculate the
speed of the event as particles are ejected from the sun and streak towards earth.
[Grade level: 6-8 | Topics: Time and speed calculations; interpreting scientific data ]
Problem 43: An Interplanetary Shock Wave On November 8, 2000 the sun released a coronal mass ejection that traveled to Earth, and its effects were
detected on Jupiter and Saturn several weeks later. In this problem, students will use
data from this storm to track its speed and acceleration as it traveled across
the solar system. [Grade level: 6-10 | Topics: Time calculations; distance = speed x time ]
Problem 7: Solar Flares, CME's and Aurora Some articles about the Northern Lights imply that
solar flares cause them. Students will use data to construct a simple Venn
Diagram, and answer an important question about whether solar flares cause
CME's and Aurora. [Grade: 5 - 7 | Topics: Venn Diagramming]
Problem 5: The November 8, 2004 solar storm Students calculate the speed of a CME, and describe
their aurora observations through writing and drawing.
[Grade: 6 - 8 | Topics: Time calculations; distance = speed x time]
Problem 505: SDO Sees Coronal Rain - Estimating Plasma Speeds
Problem 467: Estimating Magnetic Field Speeds on the Sun
Problem 337: SDO Reveals Details on the Surface of the Sun Students use a spectacular colored image of the Sun to calculate the scale of the image in kilometers per millimeter, and then
search for the smallest features relative to the size of Earth.
[Grade: 6-8 | Topics: image scales; proportions]
Problem 336: SDO: Measuring the Speed of an Eruptive Prominence Students use recent First Light images of the Sun from SDO to calculate the speed of a prominence using a sequence of scaled images
and computing position shift over the time interval of the images.
[Grade: 6-8 | Topics: image scales; speed=distane/time ]
Problem 334: Solar Dynamics Observatory: Working with Giga,
Tera, Peta and Exabytes The recent launch of SDO will bring 'high definition TV' to the study of the sun's surface details. This also means a HUGE amount of data
will have to be processed every day to handle the torrent of information. This activity works with the prefixes
giga, tera, peta and exa to familiarize students with how to interpret these quantities in a practical setting. Students already know about 'gigabytes', but
the SDO data stream represents terabytes per day, and petabytes per year in data storage demands.
[Grade: 8-12 | Topics: powers of ten; time conversion: seconds, minutes, days, years]
Problem 235: Scientific Data: The gift that keeps on giving! Students learn about gigabytes and terrabytes of data and the rates of data
generation by NASA missions and how to store it.
[Grade: 6-8 | Topics: metric units; rates; money]
Problem 373: Solar Probe Plus - Having a hot time near the sun!
Problem 278: Spitzer Studies the Distant Planet Osiris Students learn about the density of the planet HD209458b, also called Osiris, and compare it to that of Jupiter.
[Grade: 8-10 | Topics: Spherical volumes; density; Scientific Notation;]
Problem 272: Spitzer Telescope Discovers New Ring of Saturn! Students calculate the volume of the ring and compare it to the volume of Earth to check a news release figure that
claims 1 billion Earths could fit inside the new ring.
[Grade: 8-9 | Topics: Geometry, Algebra, volumn, scientific notation]
Problem 148 Exploring a Dying Star
Students use data from the Spitzer satellite to calculate the mass of a planetary nebula from a dying star.
[Grade: 9 - 11 | Topics:Scientific Notation; unit conversions; volume of a sphere ]
Problem 141: Exploring a Dusty Young Star
Students use Spitzer satellite data to learn about how dust emits infrared light and
calculate the mass of dust grains from a young star in the nebula NGC-7129.
[Grade: 4 - 7 | Topics: Algebra I; multiplication, division; scientific notation]
Problem 56: The Sombrero Galaxy Close-up
The Sombrero Galaxy in Virgo is a dazzling galaxy through the telescope,
and has been observed in detail by both the Hubble Space Telescope and the Spitzer Infrared Observatory.
This exercise lets students explore the dimensions of this galaxy as well as its finest details, using simple
image scaling calculations.
[Grade level: 9-11 | Topics: Finding the scale of an image; measurement; decimal math]
Problem 455: The Night Launch of STEREO in 2006
Problem 404: STEREO Spacecraft give 360-degree Solar View
Students use STEREO satellite images to determine which features can be seen from Earth and which cannot. They learn about the locations and changing positions of the satellites with respect to Earth's orbit.
[Grade: 6-8 | Topics: angular measure, extrapolation; distance = speed x time]
(PDF)
Problem 298: Seeing Solar Storms in STEREO - II Students explore the geometry of stereo viewing by studying a solar storm viewed from two satellites.
[Grade: 10-12 | Topics: Geometry; Trigonometry]
Problem 286: STEREO Watches the Sun Kick Up a Storm Students use images from the STEREO observation of a 'solar tsunami' to estimate its speed and kinetic energy.
[Grade: 9-12 | Topics: metric measurement; scaling; Scientific Notation; unit conversion; evaluating
a simple 2-variable formula for kinetic energy ]
Problem 248: Seeing Solar Storms in STEREO - I Students work out the details of stereoscopic vision using elementary properties of triangles and the Law of Cosines
to determine the distance from earth of a solar storm cloud.
[Grade: 8-10 | Topics: geometry, Law of Cosines, V = D/T]
Problem 207: The STEREO Mission: getting the message across Students learn about how the transmission of data is affected by how far away a satellite is for the two satellites in the STEREO constellation.
[Grade: 6-8| Topics: multiplication; division; decimal numbers.]
Problem 206: Can You Hear me now? Students learn about how the transmission of data is affected by how far away a satellite is, for a variety of spacecraft in the solar system
[Grade: 6-8| Topics: multiplication; division; decimal numbers.]
Problem 118: An Application of the Parallax Effect
The STEREO mission views the sun from two different locations in space. By combining this data, the parallax
effect can be used to determine how far above the solar surface various active regions are located. Students use the Pythagorean Theorem, a bit of
geometry, and some actual STEREO data to estimate the height of Active Region AR-978.
[Grade: 8-10 | Topics:Pythagorean Theorem; square-root; solving for variables]
Problem 116: The Comet Encke Tail Disruption Event
On April 20, 2007 NASA's STEREO satellite captured a rare
impact between a comet and the fast-moving gas in a solar coronal mass ejection. In this problem, students
analyze a STEREO satellite image to determine the speed of the tail disruption event.
[Grade: 8-10 | Topics:time calculation; finding image scale; calculating speed from distance and time]
Problem 92: A Lunar Transit of the Sun from Space
One of the STEREO satellites observed the disk of the moon pass across the sun. Students will use simple geometry to determine how far
the satellite was from the moon and Earth at the time the photograph was taken.
[Grade level: 9-11 | Topics: Geometry; parallax; arithmetic]
Problem 442: Modeling the Atmospheric Re-entry of UARS
Problem 406: Growing Grapes in the Middle of the Desert
Students use a dramatic Earth Observatory-1 satellite image of agriculture in Namibia to estimate the total cultivated
area and water needs of grape growing under desert conditions
[Grade: 6-8 | Topics: areas of irregular regions; unit conversion]
(PDF)
Problem 375: Terra Satellite Measures Dangerous Dust
Problem 339: Terra Satellite Spies the Great Gulf Oil Catastrophe of 2010 Students use a Terra satellite image of the oil slick in the Gulf of Mexico to calculate its area, mass and thickness.
[Grade: 6-8 | Topics: image scales; area of a circle; metric conversions ]
Problem 201: Fly Me To the Moon! Students learn some basic principles and terminology about how spacecraft change their orbits to get to the moon.
[Grade: 6-8| Topics: speed = distance/time; Pythagorean Theorem]
Problem 194: A Magnetic Case for 'What Came First?' Students create a timeline for events based on several data plots from the THEMIS program, and use their timeline to answer questions about the causes of magnetic storms.
[Grade: 6-8| Topics: Time calculations]
Problem 108: A Problem in Satellite Synchrony
The THEMIS program uses five satellites in five different
orbits to study Earth's magnetic field
and its changes during a storm. This problem asks students to use the periods of the
five satellites to figure out
when all 5 satellites will be lined-up
as seen from Earth. They will do this by finding the Greatest Common Multiple of the
five orbit periods, first for the case of 2 or 3 satellites, which can be easily
diagrammed with concentric circles,
then the case for all five satellites together.
[Grade: 5-9 | Topics:multiplication; Greatest Common Multiple]
Problem 3: Magnetic Storms II Students learn about the Kp index using a bar graph.
They use the graph to answer simple questions about maxima and time.
[Grade: 6 - 8 | Topics: Interpreting bar graphs; time calculations]
Problem 1: Magnetic Storms I Students learn about magnetic storms using real data
in the form of a line graph. They answer simple questions about data
range, maximum, and minimum. [Grade: 7 - 9 | Topics: Interpreting a graph; time calculations]
Problem 175: Solar Storms: Sequences and Probabilities II - Students work out the probabilities for various combinations of solar storms during a given week.
[Grade: 4-7| Topics: probability; numerating possible outcomes]
Problem 104: Loopy Sunspots!
Students will analyze data from the Hinode satellite to determine the volume and mass of a
magnetic loop above a sunspot. From the calculated volume, based on the formula for the volume of a cylinder, they will use the density of the plasma determined by
the Hinode satellite to determine the mass in tons of the magnetically trapped material.
[Grade: 9-11 | Topics:image scales; cylinder volume
calculation; scientific notation; unit conversions]
Problem 422: Supercomputers: Getting the job done FAST!
Students use a simple counting problem to explore how much faster a supercomputer is compared to as hand-calculation.
[Grade: 6-8 | Topics: algebra]
(PDF)
Problem 418: Supercomputers: Modeling colliding neutron stars!
Students use a series of time-lapse images calculated using a supercomputer to determine the speed of collision of two neutron stars, and whether they will form a black hole afterwards.
[Grade: 8-10 | Topics: distance=speed x time; scale model; triangle and circle geometry; circumference]
(PDF)
Problem 407: Cryo-testing the Webb Space Telecope ISIM
Students explore scaling by creating an enlarged geometric model of the ISIM to better
appreciate the small changes due to expansion and contraction
[Grade: 6-8 | Topics: scale models; proportions; unit conversion]
(PDF)
Problem 381: The Cosmological Redshift - Changing the light from a galaxy.
Problem 380: Seeing the Distant Universe Clearly
Problem 379: Exploring the Cosmos with Supercomputers
Problem 370: 6-fold Symmetry and the Webb Space Telescope Mirror
Problem 369: Scaling Up the Webb Space Telescope Mirror
Problem 368: The Hexagonal Tiles in the Webb Space Telescope Mirror
Problem 331: Webb Space Telescope: Detecting dwarf planets The 'JWST' will be launched some time in 2014. One of its research goals will be to detect new dwarf planets beyond the orbit of Pluto.
In this problem, students use three functions to predict how far from the sun a body such as Pluto could be detected, by calculating
its temperature and the amount of infrared light it emits.
[Grade: 9-12 | Topics: Evaluating square-roots and base-e exponentials]
Problem 329: WISE and Hubble: Power Functions: A question of magnitude Students explore the function F(x) = 10^-ax and learn about the stellar magnitude scale used by astronomers to rank the brightness of stars.
[Grade: 10-12 | Topics: base-10, evaluating power functions ]
Problem 328: WISE: F(x)G(x): A Tale of Two Functions Students use WISE satellite data to study a practical application of the product of two finctions by graphing them individually, and their product.
A calculus-level problem is included for advanced students.
[Grade: 10-12 | Topics: Power-law functions; domain and range; graphing; areas under curves; integration]
Problem 327: WISE: Exploring Power-law Functions Using WISE Data Based on a recent press release of the 'First Light' image taken with NASA's new WISE satellite,
students explore a practical application of a power law function to count the number of stars in the sky.
An additional calculus-level problem is included for advanced students.
[Grade: 10-12 | Topics: areas; functions; histograms; unit conversion; power-laws; integration]
Problem 510: Planck Mission Sees the Ancient Universe Clearly
Problem 233: The Milky Way: A mere cloud in the cosmos- Students compare the average density of the Milky Way with the density of the universe.
[Grade: 8-10 | Topics: Volume of disk, density, scientific notation]
Problem 192: The Big Bang - Cosmic Expansion - Students explore the expansion of the universe predicted by Big Bang cosmology
[Grade: 10-12| Topics: Algebra, Integral Calculus]
Problem 136 : Energy Generation near Black Holes
Students explore how much energy is generated by stars
and gas falling into black holes. The event horizon radius is calculated from a
simple equation, R = 2.95 M, and energy is estimated from E = mc^2.
[Grade: 7 - 10 | Topics:Scientific Notation; Working with equations in one variable to first and second power.]
Astronomers using NASA's Hubble Space Telescope have confirmed that this gas giant
planet is orbiting so close to its star its heated atmosphere is escaping into space.
[Grade: 9-12 | Topics: Scientific Notation; volume of a sphere; density; rates]
(PDF)
This young star cluster, barely one million years old, is furiously evaporating the clouds
of interstellar gas and dust from which it formed.
[Grade: 9-12 | Topics: Scientific Notation; evaluating functions; density]
(PDF)
The track of an asteroid in a Hubble image of a cluster of galaxies is analyzed to determine speed of the asteroid.[Grade: 6-8 | Topics: Scaling; unit conversion; speed=distance/time]
(PDF)
Interstellar Boundary Explorer (IBEX)
Imager for Magnetosphere to Auroral Global Exploration (IMAGE)
InSight Seismographic Station on Mars
Students work with latitude and longitude and scaled images of mars to locate the InSight proposed
landing area, and describe the terrain of the landing area.
[Grade: 6-8 | Topics: degree measure; latitude and longitude; working with scaled images; metric measure]
(PDF)
Students use scaled images of a proposed InSIght landing area and a scaled image of an urban neighborhood on Earth to compare the sizes
of familiar things with the unfamiliar martian landscape.
[Grade: 6-8 | Topics: scale; proportion; metric measurement]
(PDF)
Students are introduced to the Moment Magnitude marsquake scale which gives a logarithmic index for marsquakes of differing energies. They
calculate two examples of marsquakes and meteor impacts and compare their Moment Magnitude.
[Grade: 8-10 | Topics: logarithms; scientific notation; algebra ]
(PDF)
Students work with a logarithmic scale to estimate how much ground movement occurs for earthquakes of different strengths.
[Grade: 8-10 | Topics: logarithms; base-ten exponents]
(PDF)
Students devive a basic equation for the distance to the horizon on a spherical body using the Pythagorean Theorem
and a bit of algebra. The estimate the number of cell towers needed to cover Mars.
[Grade: 8-10 | Topics: Pythagorean Theorem, Algebra; scientific notation; areas of spheres and circles ]
(PDF)
Students use the volume properties of spheres and shells along with the
relationship mass=densityxvolume to create a model of the interior of mars.
[Grade: 8-10 | Topics: formula for volume of spheres and spherical shells; mass=densityxvolume; scientific notation ]
(PDF)
Students calculate the mass of mars by using satellite data and Keplers Third Law.
[Grade: 8-10 | Topics: Algebra; scientific notation ]
(PDF)
Students work with logarithmic scales to explore the relationship between the energy of an marsquake and its logarithmic index, which is
similar to the Richter Scale used for earthquakes.
[Grade: 8-10 | Topics: Logarithmic scales; scientific notation ]
(PDF)
Students learn about the heat flow formula and use it to explore the properties of Earth and Mars in terms of their crust composition.
[Grade: 8-10 | Topics: Algebra; temperature gradients]
(PDF)
Students explore how insulation works to reduce heat flow. They convert a verbal description of a formula expressed in proportions, and use it to calculate why aluminum pots heat faster than steel pots, and how we can determine the
properties of martian sooil from heat flow and temperature changes.
[Grade: 8-10 | Topics: algebra; rates of change ]
(PDF)
Students explore the rate of temperature change in the crust of Earth and Mars and learn about units expressed as degrees C/km. They calculate how hot the ground will be at various depths, and how
gold miners must deal with extreme heat.
[Grade: 6-8 | Topics: fahrenheit and celsius degrees; rates of change]
(PDF)
Students explore how long it takes to transmit digital data using examples from downloading songs from their computer to their ipod.
[Grade: 6-8 | Topics: working with kilo, mega and rates of data transfer in bytes/sec. ]
(PDF)
Students learn about the IDC camera and calculate resolution and how many images are needed to map the InSight landing area.
[Grade: 6-8 | Topics: ANgular measurfe, degrees and seconds; image scal; tiling an area with overlap. ]
(PDF)
Students work with two clocks on Earth and Mars and learn about earth and mars time given that a day on Mars is 40 minutes longer than an Earth day.
[Grade: 6-8 | Topics: time calculations, hours, minutes, seconds; length of day ]
(PDF)
The earth-sun angle is given in tabular form in degrees. Students graph the data and find the dates when transmissions to Earth cannot occur.
[Grade: 8-10 | Topics: Interpreting tabular data; rates and slopes ]
(PDF)
Students estimate the mass of a martian dust devil using the approximation that it is a cylinder with a fixed
density of dust. [Grade: 8-10 | Topics: Volume of a cylinder; mass = density x volume ]
(PDF)
Students estimate the area in front of the InSight lander where experiments will be conducted and
instruments moved with a single robotic arm. [Grade: 6-8 | Topics: Area of a circle segment; Area
common to two intersecting circles]
(PDF)
Students learn about scheduling many events along a timeline (breakfast, packing, driving, etc )
by planning a family trip where the family members have to arrive at the airport for a flight that
leaves at a specific date and time. [Grade: 5-7 | Topics: working with time units; creating a timeline]
(PDF)
Students explore the properties of decagons to determine the area of the solar panels used on the
InSight lander. [Grade: 7-9 | Topics: area of regular polygons; estimating areas of non-square shapes]
(PDF)
Students work with the circumference of Mars and the speed of shock waves in the martian crust to estimate the arrival times of the waves at the InSight Lander.
[Grade: 6-8 | Topics: speed=distance/time; Time calculations; circumference of a circle]
(PDF)
Juno to Jupiter
Students use the Standard Formula for an ellipse to study the elliptical orbit of the Juno spacecraft, and relate specific properties of the
ellipse to features of the spacecrafts trajectory such as aphelion, perihelion, and ellipticity.
[Grade: 9-12 | Topics: formula for an ellipse; semi-major and minor axis]
(PDF)
Students use a series of images from a launch video to determine the scale of each image and
determine the speed of the rocket as it leaves the gantry.
[Grade: 6-8 | Topics: scale models; speed = distance/times]
(PDF)
Students use tabulated altitude and range data following the launch of the Juno mission, to determine the speed of the rocket as it travels to arth orbit.
[Grade: 6-8 | Topics: scale models; speed = distance/time]
(PDF)
Students use the formula for an ellipse, along with the inverse-square law to create a mathemartical model that predicts
the declining solar power produced by Junos solar panels as the spacecraft travels from Earth to Jupiter.
[Grade: 9-12 | Topics: algebra; trigonometry; distance formula]
(PDF)
Kepler Exoplanet Transit Explorer
Students use simple fraction arithmetic to determine the relative sizes of several new planets recently discovered by the Kepler mission,
and compare these sizes to that of Jupiter and Earth.
[Grade: 3-5 | Topics: scale models; proportions; fractions]
(PDF)
The recently-confirmed Earth-like planet Kepler-22b by the Kepler Observatory is a massive planet orbiting its star in the temperature zone suitable for liquid water. This problem explores the gravity and mass of this planet, and some implications for playing baseball on its surface!
[Grade: 8-10 | Topics: scale models; proportions; scientific notation; metric math; Evaluating equations]
(PDF)
Students determine how often the two stars Kepler 16 A and B will line up with Tatooine on
the same day of the year. [Grade: 6-8 | Topics: comparing two sequences of numbers; patterns, Least Common Multiple]
(PDF)
Students explore the orbit speeds of Tatooine and Kepler-16B and predict how often the two stars line up with the planet
to create an 'eclipse'. [Grade: 6-9 | Topics: angle measure; angular speed]
(PDF)
Using the tangent function, students estimate the angular diameter and separation of the two stars in the Kepler 16 binary system as
viewed from the planet's surface...if it had one!! [Grade: 8-10 | Topics: angle measure; tangent]
(PDF)
A statistical study of the 700 transits seen during the first 43 days of the mission. [Grade: 6-8 | Topics: Percentages; area of circle]
(PDF)
Landsat
Students work with image of agricultural area to estimate the percentage of area cultivated and the total rainfall in gallons per year.
[Grade: 6-8 | Topics: area of square and rectangle; metric units; unit conversion]
(PDF)
Students use Landsat imagery from 1972 and 2011 to determine how much additional water is being used for irrigation in a small region of Kansas.
[Grade: 6-8 | Topics: Area of a circle; unit conversions ]
(PDF)
Lunar Orbiter
Lunar Reconnissance Orbiter (LRO)
Students examine two Apollo landing areas using images from the LRO spacecraft to estimate the relative ages of the two regions using
crater counting. [Grade: 6-8 | Topics: scale; histogramming]
(PDF)
Students use a recent image obtained by the LRO spacecraft to estimate how far astronauts walked to get to various points in the
landing area.
They also estimate how many craters are in this area and the average impact time between crater events.
[Grade: 6-8 | Topics: image scale; metric measurement]
(PDF)
Students use the published LRO temperature map to study the scale of the south polar region, the sizes of its craters,
and estimate the volume of water-ice that may be present in the Shackleton Crater.
[Grade: 7-9 | Topics: Volume of a circular disk; scale models]
(PDF)
Students count large craters on an LRO coded image of the lunar surface to estimate whether the impacting asteroids
that produced the largest
craters were from the same population of asteroids during the two different epocs of impacts.
[Grade: 8-10 | Topics: Scaled images; histograming; inference]
(PDF)
Manned Space Programs - Apollo, ISS, Shuttle, Ares, SpaceX
Students use data from the launch of the Falcon 9 booster to determine its speed and acceleration.
[Grade: 6-8 | Topics: speed=distance/time; Time calculations]
(PDF)
Students detemine the volume of the Dragon capsule using the volume formula for a cone.
[Grade: 9-12 | Topics: Volumes of 3-d objects; cones; evaluating functions]
(PDF)
Students explore volume density and mass using the Space Shuttle thermal tiles. Get your own free tile from NASA too!
[Grade: 6-8 | Topics: mass = density x volume; metric conversion]
(PDF)
Students use tabular data and graphing to determine the launch speed and acceleration of the Space Shuttle from the launch pad. [Grade: 6-8 | Topics: tabular data, graphing, metric measurement, speed=distance/time]
(PDF)
Students tabular data to determine the launch speed of the Saturn V rocket from the launch pad.
[Grade: 6-8 | Topics: tabular data, graphing, metric measurement, speed=distance/time]
(PDF)
Students use a sequence of images to determine the launch speed of the satellite from the Space Shuttle cargo bay.
[Grade: 6-8 | Topics: scale, metric measurement, speed=distance/time]
(PDF)
Students use a sequence of images to determine the speed of ascent of the Apollo-17 capsule from the lunar surface.
[Grade: 6-8 | Topics: scale, metric measurement, speed=distance/time]
(PDF)
Students use a sequence of images from a video of the launch to determine speed from the time
interval between the images, and the scale of each image.
[Grade: 6-8 | Topics: scale, metric measurement, speed=distance/time]
(PDF)
Students use a sequence of images from a video of the launch to determine speed from the time
interval between the images, and the scale of each image.
[Grade: 6-8 | Topics: scale, metric measurement, speed=distance/time]
(PDF)
Students use a sequence of images from a video of the launch to determine speed from the time
interval between the images, and the scale of each image.
[Grade: 6-8 | Topics: scale, metric measurement, speed=distance/time]
(PDF)
Students use a sequence of images from a video of the launch to determine speed from the time
interval between the images, and the scale of each image.
[Grade: 6-8 | Topics: scale, metric measurement, speed=distance/time]
(PDF)
An amateur photograph of the International Space Station crossing in front of the sun is analyzed to determine the scales of sunspots. [Grade: 9-12 | Topics: Similar triangles; angular measure]
(PDF)
Magnetosphere Multi-Scale Mission (MMS)
Mars Science Lab and Curiosity Rover
Students learn about diffraction geometry and then estimate the distance between crystal planes in a mars rock sample.
[Grade: 10-12 | Topics: geometry; trigonometry]
(PDF)
Students plot the position of the Curiosity Rover on a cartesian grid covering the satellite image of the landing area. They use the 2-point distance formula to determine how far the rover
traveled between stops, and determine it speed.
[Grade: 6-8 | Topics: Cartseian graphs; ordered pairs and coordinates; distance = speed x time; metric measure ]
(PDF)
Students estimate the speed of an ancient mars river using images from the CUriosity rover.
[Grade: 9-12 | Topics: Algebra; trigonometry; evaluating functions ]
(PDF)
Students explore the Gale Crater landing area and calculate rover distances to
various way stations to determine the round trip distance and travel time.
[Grade: 9-12 | Topics: Pythagorean Distance Formula; Coordinate geometry ]
(PDF)
Students use the properties of ellipses to determine the formula for the Hohmann Transfer Orbit taking the Mars Science Laboratory to Mars in 2012
[Grade: 10-11 | Topics: time=distance/speed; scale models; metric math; properties of ellipses]
(PDF)
Students use a sequence of launch images to determine the Atlas V's launch speed and acceleration. By determining the scale of each image, they estimate average speeds during the first 4 seconds after lift-off.
[Grade: 8-10 | Topics: time=distance/speed; scale models; metric math]
(PDF)
Mars Rovers, Orbiters, etc.
Mercury Surface, Space Environment, Geochemistry, and Ranging (MESSENGER)
Students work with a simple spherical core and shell model to determine the interior structure of mercury and the size of its dense iron core.
[Grade: 9-12 | Topics: working with volumes of speheres; mass = density x volume]
(PDF)
Students use the orbit of NASA's MESSENGER spacecraft to determine the mass of Mercury.
[Grade: 9-12 | Topics: working with equations with integer powers and solving for specified values; scientific notation]
(PDF)
Near Earth Asteroid Rendezvous (NEAR)
Radiation Belt Storm Probe (RBSP)
Students use a model of the orbit of the van Allen Belts Probes and simulated data to draw the locations of the three van Allen Belts in space.
[Grade: 3-5 | Topics: Interpreting Tabular Data]
(PDF)
The location of the Chorus signal from each of the RBSP spacecraft is given by a linear equation that represents the direction along which the signal is detected by each spacecraft. Students solve the two linear equations for the common intersection point representing the location of the Chorus signal in space. This can be done graphically by plotting each linear equation, or solved algebraically.
[Grade: 6-8 | Topics: Linear equations; solving systems of equations; graphical solutions ]
(PDF)
Students use hypothetical information from the twin RBSP spacecraft to triangulate the location of the Chorus signal near Earth using angle measurements, graphing and protractors to identify the intersection point of the CHorus signals.
[Grade: 6-8 | Topics: Angles; graphing; protractors ]
(PDF)
Students explore the method of triangulation and how it might be used by the RBSP spacecraft to find the origin of the Chorus signals.
[Grade: 6-8 | Topics: Graphing on the Cartesian plane; distances between points. ]
(PDF)
Ramaty High Energy Solar Spectroscopic Imager (RHESSI)
Solar and Heliospheric Observatory (SOHO)
Solar Dynamics Observatory (SDO)
Students estimate the speed of plasma streamers near the solar surface using images from a Solar Dynamics Observatory.
[Grade: 6-8 | Topics: scale models; speed=distance/time; proportions]
(PDF)
Students use two images from the Solar Dynamics Observatory to estimate the speed of the X-class solar flare on March 6, 2012.
[Grade: 6-8 | Topics: speed=distance/time; scale model; metric measurement]
(PDF)
Solar Probe Plus
Students use a simple equation to estimate the temperature reached by the Solar Probe Plus spacecraft as it gets close to the sun.
[Grade: 8-10 | Topics: Evaluating a function; square roots and forth roots]
(PDF)
Students use the tangent formula to determine the angular diameter of the sun as seen by the
Solar Probe Plus spacecraft as it approaches the sun.
[Grade: 8-10 | Topics: angular measure; tangent formula; angular size]
(PDF)
Spitzer Space Telescope
Solar Terrestrial Relations Observatory (STEREO)
An example of old news seen in a different way! Students use a spectacular time-lapse photo of the launch of the STEREO mission obtained by photographer Dominic Agostini in 2006 to study parabolic curves.
[Grade: 8-10 | Topics: time=distance/speed; scale models; metric math; equation of a parabola; curve fitting]
(PDF)
Terra, Landsat, UARS, Earth Observatory
Students graph the altitude of the UARS satellite in the weeks before re-enrty to explore the accelerating
effects of atmospheric drag. They create a mathematical model that fits the data, and use this to make their own
prediction of the re-entry date. [Grade: 8 - 11 | Topics: graphing data; linear equations; exponential and power functions]
(PDF)
Students determine the number of dust particles inhaled by using a satellite map of the dust concentration and a
calculation of the mass of a typical dust grain.
[Grade: 8-10 | Topics: unit conversion; scientific notation; mass=densityxvolume]
(PDF)
Time History of Events and Macroscale Interactions during Substorms (THEMIS)
Transition Region and Coronal Explorer (TRACE)
Webb Space Telescope
Students learn about the redshift unit of measurement in astronomy, and solve a simple linear equation to explore
how the light from very distant galaxies is reddened compared to nearby galaxies.
[Grade: 8-10 | Topics: solving a simple equation for X]
(PDF)
Students calculate the angular sizes and scales of distant objects to study how different sized
telescopes see details with varying degrees of clarity.
[Grade: 7-9 | Topics: solving a simple equation for X; angular measure; Scientific Notation]
(PDF)
Students use two images created by a supercomputer calculation to explore the size and accuracy of computer models of the distanct universe.
[Grade: 7-9 | Topics: scale model; proportions; Scientific Notation]
(PDF)
Students learn about the Webb Space Telescopes segmented mirror and its rotational 6-fold symmetry due to tiling with hexagons.
They identify groups of tiles that have identical optical properties
[Grade: 8-10 | Topics: Properties of Hexagons; rotation symmetry; counting; tiling]
(PDF)
Students learn about the Webb Space Telescopes segmented mirror and determine the area of the mirror along with scaled up
versions of this mirror using the formula for the area of a hexagon, and the properties of tiling a surface with hexagons.
[Grade: 8-10 | Topics: Properties of Hexagons and triangles; counting; evaluating a formula; tiling]
(PDF)
Students learn about the Webb Space Telescopes segmented mirror by studying the geometry of hexagons.
[Grade: 8-10 | Topics: Properties of Hexagons and triangles; counting]
(PDF)
Wide-Field Infrared Survey Explorer (WISE)
Wilkinson Microwave Anisotropy Probe (WMAP) and Planck
Students work with an image of the universe when it was 370,000 years old and determine from simple scaling and
proportions the sizes of the features seen in the image compared to the Milky Way.
[Grade: 6-8 | Topics: scale and proportion; angular measure]
(PDF)
X-ray Multi-Mirror mission (XMM)


