Goddard Space Flight Center

Problem 669: Exploring Two Nearby Stars to the Sun. Students explore two nearby stars Ross 128 and Gliese 445 and determine when they will be the nearest stars to our sun by working with quadratic equations that model their distances. [Grade: 9-12 | Topics: Working with quadratic equations; intersection points of quadratic functions] [Click here]

Problem 665: Kepler - Keplers Latest Count on Goldilocks Planets Students examine the statistics of the latest candidate planets beyond our solar system, work with poercentages and a bar graph, and estimate the number of earth-like planets in our Milky Way. [Grade: 6-8 | Topics: percentages, bar graphs, estimation] [Click here]

Problem 664: HST - The Suns Nearest Companions at least for now! Students study a graph that models the distances from the sun of seven nearby stars over a 100,000 year time span. They determine the minimum distances and a timeline of which star will be the suns new closest neighbor in space in the next 80,000 years. [Grade: 6-8 | Topics: Graphical data; finding minimum from a plotted curve] [Click here]

Problem 608: Constellations in 3D Students create a 3-d model of the constellation Orion and explore how stars are located in space and how this perspective changes from different vantage points. [Grade: 6-8 | Topics: geometry; scale] [Click here]

Problem 564:Exploring the Stars in Orion - Light Year Madness Students explore the light year and its relationship to light travel time for observing events in different parts of space. When would colonists at different locations observe the star Betelgeuse become a supernova? [Grade: 6-8 | Topics: time lines; time intervalcalculations; time = distance/speed ] [Click here]

Problem 561:Exploring the Evaporating Exoplanet HD189733b Students estimate how quickly this planet will lose its atmosphere and evaporate at its present loss rate of 6 million tons/second [Grade: 6-8 | Topics:mass=densityx volume; rates; volume of a sphere ] [Click here]

Problem 517: A Distant Supernova Remnant Discovered Students work with proportions and scaling to discover the size of the supernova remnant compared to the distance from the Sun to the nearest star Alpha Centauri. The also work with time and speed calculations to estimate the speed of the supernova compared to the International Space Station. [Grade: 6-8 | Topics: proportions; speed=distance/time] [Click here]

Problem 494: The Close Encounter to the Sun of Barnards Star Students use parametric equations and calculus to determine the linear equation for the path of Barnards Star, and then determine when the minimum distance to the sun occurs [Grade: 12 | Topics: Derivitives and minimization] [Click here] 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 pattern 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 ] [Click here]

Problem 483: The Radioactive Dating of a Star in the Milky Way! Students explore Cayrel's Star, whose age has been dated to 12 billion years using a radioisotope dating technique involving the decay of uranium-238. [Grade: 9-12 | Topics: half-life; exponential functions; scientific notation] [Click here]

Problem 482: Exploring Density, Mass and Volume Across the Universe Students calculate the density of various astronomical objects and convert them into hydrogen atoms per cubic meter in order to compare how astronomical objects differ enormously in their densities. [Grade: 9-12 | Topics: Density=mass/volume; scientific notation; unit conversion; metric math ] [Click here]

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 ] [Click here]

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] [Click here]

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] [Click here]

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 from the pulsar. [Grade: 6-8 | Topics: Scale drawings; unit conversion; distance = speed x time] [Click here]

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 ] [Click here]

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] [Click here]

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] [Click here]

Problem 322: Rotation Velocity of a Galaxy Students examine a simple model of the rotation of a galaxy to investigate how fast stars orbit the centers of galaxies in systems such as the Milky Way and Messier-101. [Grade: 10-12 | Topics: Algebra, limiting form of functions; derivitives] [Click here]

Problem 320: Star Light...Star Bright A simple polynomial function is used to determine the temperature of a star from its brightness at two different visible wavelengths. [Grade: 10-12 | Topics: Algebra II; Polynomials; maxima and minima] [Click here]

Problem 319: How Many Stars Are In the Sky? A simple polynomial is used to determine how many stars are in the sky. [Grade: 10-12 | Topics: Log Functions; Polynomials] [Click here]

Problem 318: The Internal Density and Mass of the Sun Students use a simple, spherically symmetric, density profile to determine the mass of the sun using integral calculus. [Grade: 11-12 | Topics: Algebra II; Polynomials; integral calculus] [Click here]

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] [Click here]

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] [Click here]

Problem 294: Star Cluster math A simple counting exercise involving star classes lets students work with percentages and ratios. [Grade: 4-6 | Topics: Counting; percentage; scaling] [Click here]

Problem 284: Calculating the Thickness of a Neutron Star Atmosphere Students determine the thickness of the carbon atmosphere of the neutron star Cas-A using Earth's atmosphere and a set of scaling relationships. [Grade: 9-12 | Topics: Algebra I; Exponential functions; graphing; Scientific notation] [Click here]

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] [Click here]

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;] [Click here]

Problem 269: Parts Per Hundred (pph) Students work with a common unit to describe the number of objects in a population. Other related quantities are the part-per-thousand, part-per-million and part-per-billion. [Grade: 3-5 | Topics: counting, unit conversion] [Click here]

Problem 241: Angular Size and Similar Triangles A critical concept in astronomy is angular size, measured in degrees, minutes or arc-seconds. This is a review of the basic properties of similar triangles for a fixed angle. [Grade: 8-10 | Topics: geometry, similar triangles, proportions] [Click here]

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 various features compared to our solar system [Grade: 8-10 | Topics: scale, proportion, angle measure] [Click here]

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] [Click here]

Problem 232: Star Circles- Students use a photograph of star trails around the North Star Polaris to determine the duration of the timed exposure based on star arc lengths. [Grade: 8-9 | Topics: Lengths of arcs of circles; angular measure.] [Click here]

Problem 231: Star Magnitudes and Decimals- Students work with the stellar magnitude scale to determine the brightness differences between stars. [Grade: 5-8 | Topics: Multiplying decimals.] [Click here]

Problem 224: Perimeters; Which constellation is the longest?- Students use tabulated data for the angular distances between stars in the Big Dipper and Orion to determine which constellation has the longest perimeter, and the average star separations. [Grade: 3-5 | Topics: perimeter of a curve; basic fractions; mixed numbers.] [Click here]

Problem 221: Pulsars and Simple Equations- Students work with linear equations describing the rotation period of a pulsar, and evaluate the equations for various conditions. Students use the equations to predict intersection points in time. [Grade: 6-8 | Topics: Evaluating simple one-variable equations] [Click here]

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.] [Click here]

Problem 212: Finding Mass in the Cosmos- Students derive a simple formula, then use it to determine the masses of objects in the universe from the orbit periods and distances of their satellites. [Grade: 9-12| Topics: Scientific Notation; Algebra II; parametric equations] [Click here]

Problem 211: Where Did All the Stars Go?- Students learn why NASA photos often don't show stars because of the way that cameras take pictures of bright and faint objects. [Grade: 6-8| Topics: multiplication; division; decimal numbers.] [Click here]

Problem 209: How to make faint things stand out in a bright world!- Students learn that adding images together often enhances faint things not seen in only one image; the power of averaging data. [Grade: 6-8| Topics: multiplication; division; decimal numbers.] [Click here]

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] [Click here]

Problem 191: Why are hot things red? - Students explore the Planck Function using graphing skills, and calculus for experts, to determine the relationship between temperature and peak wavelength. [Grade: 10-12| Topics: Algebra, graphing, differential calculus] [Click here]

Problem 190: Modeling a Planetary Nebula - Students use calculus to create a mathematical model of a planetary nebula [Grade: 10-12| Topics: Algebra, Integral calculus] [Click here]

Problem 189: Stellar Temperature, Size and Power- Students work with a basic equation to explore the relationship between temperature, surface area and power for a selection of stars. [Grade: 8-10| Topics: Algebra] [Click here]

Problem 186: Collapsing Gas Clouds and Stability- Students use the derivative to find an extremum of an equation governing the pressure balance of an interstellar cloud. [Grade: 11-12| Topics: differentiation; finding extrema; partial derivitives] [Click here]

Problem 182: Our Neighborhood in the Milky Way- Students create a scale model of the local Milky Way and estimate distances and travel times for a series of voyages. [Grade: 6-8| Topics: scale models; speed-distance-time] [Click here]

Problem 172: The Stellar Magnitude Scale- Students learn about positive and negative numbers using a popular brightness scale used by astronomers. [Grade: 3-6| Topics: number relationships; decimals; negative and positive numbers] [Click here]

Problem 170: Measuring Star Temperatures- Students use a simple formula to determine the temperatures of stars, and to use a template curve to analyze data for a specific star to estimate its temperature. [Grade: 6-8 | Topics: algebra, graph analysis] [Click here]

Problem 160: The Relative Sizes of the Sun and Stars- Students work through a series of comparisons of the relative sizes of the sun compared to other stars, to create a scale model of stellar sizes using simple fractional relationships. ( e.g if Star A is 6 times larger than Star B, and Star C is 1/2 the size of Star B, how big is Star C in terms of Star A?) [Grade: 4-6 | Topics: working with fractions; scale models] [Click here]

Problem 158: The Solar Neighborhod within 17 Light Years - Students create a scale model of the local solar neighborhood and determine the shortest travel distances to several stars. [Grade: 6-8 | Topics: Plotting polar coordinates using a ruler and compass; decimal math] [Click here]

Problem 156: Spectral Classification of Stars- Students use actual star spectra to classify them into specific spectral types according to a standard ruberic. [Grade: 5-8 | Topics: Working with patterns in data; simple sorting logic] [Click here]

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 ] [Click here]

Problem 147 Black hole - fade out Students calculate how long it takes light to fade away as an object falls into a black hole. [Grade: 9 - 11 | Topics: Scientific Notation; exponential functions] [Click here]

Problem 146 Black Hole Power Students calculate how much power is produced as matter falls into a rotating and a non-rotating black hole including solar and supermassive black holes. [Grade: 9 - 11 | Topics:Scientific Notation; Spherical shells; density; power] [Click here]

Problem 145 Black Holes - What's Inside? Students work with the Pythagorean Theorem for black holes and investigate what happens to space and time on the other side of an Event Horizon. [Grade:9 - 11 | Topics: Scientific Notation; distance; time calculations; algebra] [Click here]

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.] [Click here]

Problem 142 Black Holes---Part VIII Matter that falls into a black hole heats up in an accretion disk, which can emit x-rays and even gamma rays visible from Earth. In this problem, students use a simple algebraic formula to calculate the temperature at various places in an accretion disk. [Grade: 7 - 10 | Topics:Scientific Notation; Working with equations in one variable to first and second power.] [Click here]

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] [Click here]

Problem 140 Black Holes---Part VII If you fell into a black hole, how fast would you be traveling? Students use a simple equation to calculate the free-fall speed as they pass through the event horizon. [Grade: 7 - 10 | Topics:Scientific Notation; Working with equations in one variable to first and second power.] [Click here]

Problem 138 Black Holes---Part VI Tidal forces are an important gravity phenomenon, but they can be lethal to humans in the vicinity of black holes. This exercise lets students calculate the tidal acceleration between your head and feet while standing on the surface of Earth...and falling into a black hole. [Grade: 7 - 10 | Topics:Scientific Notation; Working with equations in one variable to first and second power.] [Click here]

Problem 137 Black Holes---Part V Students explore how Kepler's Third Law can be used to determine the mass of a black hole, or the mass of the North Star: Polaris. [Grade: 7 - 10 | Topics:Scientific Notation; Working with equations in one variable to first and second power.] [Click here]

Problem 136 Black Holes---Part IV 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.] [Click here]

Problem 132 Black Holes - III Students learn about how gravity distorts time near a black hole and other massive bodies. [Grade: 8 - 12 | Topics:Simple linear equations; scientific notation] [Click here]

Problem 131 How Big is It? - Las Vegas up close. Students work with an image taken by the QuickBird imaging satellite of downtown Las Vegas, Nevada. They determine the image scale, and calculate the sizes of streets, cars and buildings from the image. [Grade: 4 - 7 | Topics:image scaling; multiply, divide, work with millimeter ruler] [Click here]

Problem 130 Black Holes - II Students learn about how gravity distorts time and causes problems even for the Global Positioning System satellites and their timing signals. [Grade: 8 - 12 | Topics:Simple linear equations; scientific notation] [Click here]

Problem 128 Black Holes - I Students learn about the most basic component to a black hole - the event horizon. Using a simple formula, and scientific notation, they examine the sizes of various kinds of black holes. [Grade: 8 - 12 | Topics:Simple linear equations; scientific notation] [Click here]

Problem 115 A Mathematical Model of the Sun Students will use the formula for a sphere and a shell to calculate the mass of the sun for various choices of its density. The goal is to reproduce the measured mass and radius of the sun by a careful selection of its density in a core region and a shell region. Students will manipulate the values for density and shell size to achieve the correct total mass. This can be done by hand, or by programming an Excel spreadsheet. [Grade: 8-10 | Topics: scientific notation; volume of a sphere and a spherical shell; density, mass and volume.] [Click here]

Problem 62 Star light...Star bright - A question of magnitude! - Since the time of the ancient Greek astronomer Hipparchus, astronomers have measured and cataloged the brightness of stars according to the 'apparent magnitude scale'. This activity lets students experience this peculiar numbering system where bright stars have small numbers (even negative: our sun is a -26 magnitude!) and faint stars have large numbers (faintest stars are +29 magnitudes). Students will calculate the brightness differences between stars using multiplication and division. Working with the number line will be a big help and math review! [Grade level: 4-6 | Topics: Positive and negative numbers; decimal math] [Click here]

Problem 61 Drake's Equation and the Search for Life...sort of! - In the 1960's astronomer Frank Drake invented an equation that helps us estimate how much life, especially the intelligent kind, might exist in our Milky Way. It has been a lively topic of discussion in thousands of college astronomy courses for the last 30 years. In this simplified version, your students will get to review what we now know about the planetary universe, and come up with their own estimates. The real fun is in doing the research to track down plausible values (or their ranges) for the factors that enter into the equation, and then write a defense for the values that they choose. Lots of opportunity to summarize basic astronomical knowledge towards the end of an astronomy course, or chapter. [Grade level: 6-8 | Topics: decimal math; evaluating functions for given values of variables] [Click here]

Problem 58 How many stars are there? - For thousands of years, astronomers have counted the stars to determine just how vast the heavens are. Since the 19th century, 'star gauging' has been an important tool for astronomers to assess how the various populations of stars are distributed within the Milky Way. In this activity, students will get their first taste of star counting by using a star atlas reproduction and bar-graph the numbers of stars in each magnitude interval. They will then calculate the number of similar stars in the sky by scaling up their counts to the full sky area. [Grade level: 6-8 | Topics: Positive and negative numbers; histogramming; extrapolating data] [Click here]

Problem 53 Astronomy: A Moving Experience! - Objects in space move. To figure out how fast they move, astronomers use many different techniques depending on what they are investigating. In this activity, you will measure the speed of astronomical phenomena using the scaling clues and the time intervals between photographs of three phenomena: A supernova explosion, a coronal mass ejection, and a solar flare shock wave. [Grade level: 6-8 | Topics: Finding the scale of an image; metric measurement; distance = speed x time; scientific notation] [Click here]

Problem 52 Measuring the size of a Star Cluster - Astronomers often use a photograph to determine the size of astronomical objects. The Pleiades is a famous cluster of hundreds of bright stars. In this activity, students will determine the photographic scale, and use this to estimate the projected (2-D) distances between the stars in this cluster. They will also use internet and library resources to learn more about this cluster. [Grade level: 4-6 | Topics: Online research; Finding the scale of an image; metric measurement; decimal math] [Click here]

Problem 47 Discovering the Milky Way by Counting Stars. - It is common to say that there are about 8,000 stars visible to the naked eye in both hemispheres of the sky, although from a typical urban setting, fewer than 500 stars are actually visible. Students will use data from a deep-integration image of a region of the sky in Hercules, observed by the 2MASS sky survey project to estimate the number of stars in the sky. This number is a lower-limit to the roughly 250 to 500 billion stars that may actually exist in the Milky Way. [Grade level: 4-6 | Topics: Tallying data; decimal math] [Click here]

Problem 44 Interstellar Distances with the Pythagorean Theorem - If you select any two stars in the sky and calculate how far apart they are, you may discover that even stars that appear to be far apart are actually close neighbors in space. This activity lets students use the Pythagorean distance formula in 3-dimensions to explore stellar distances for a collection of bright stars, first as seen from Earth and then as seen from a planet orbiting the star Polaris. Requires a calculator and some familiarity with algebra and square-roots. [Grade level: 9-11 | Topics: Decimal math; Pythagorean Theorem; square root] [Click here]