Solar System Litho! IS~~SOIII\3 for Earth and Space Science
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Educational Product EaTeachers Grades K-12 NASA-EP-33 8 Solar System Litho! IS~~SOIII\3 for Earth and Space Science This set contains the following materials: Our Star-The Sun Mercury Venus Earth Moon Mars Jupiter Saturn Uranus Neptune Pluto Asteroids: Ida with Moon and Gaspra (Inset) NASA Resources for Educators Electronic Resources for Educators National Aeronautics and Our Star - The Sun @ Space Administration Our Star The Sun 7 National Aeronautics and - Space Administration v The Sun is a huge, bright sphere of mostly ionized gas the Sun. Temperature steadily increases with altitude degrees K. The process that heats the corona is.very about 5billionyears old. The closest star to Earth, it is 16 up to 50,000 K, while density drops to 100,000 times mysterious and poorly understood, since the laws of million km distant (this distance is called an Astronomi- less than in the photosphere. Above thechromosphere thermodynamics state that heat energy flows from a cal Unit). The next closest star is 300,000 times further lies the corora ("crown"), extending outward from the hotter to a cooler place. Mysterious phenomena, such away. There are probably millions of similar stars in the Sun in the form of the "solar wind" to the edge of the as this, are studied by researchers in NASA's Space Milky Way galaxy (and even more galaxies in the Uni- solar system. The corora is extremely hot -millions of Physics Division. vem), but the Sun is the most important to us because it supports life on Earth. It powers photosynthesis in green plants and is ultimately the source of all food and fossil fuel. The Sun's power causes the seasons, the climate, the Fast Facts SignmCant Dates cumnts in the ocean, the circulation of the air, and the weather in the atmosphere. Spectral Type of Star G2 V 585 BC First solar eclipse successfully predicted The Sun is some 333,400 times more massive than 1610 Galileoobservessunspdswithhistelescope 4.5 Billion Years Earth (mass= 1.99 x 1030 kg), and contains99.86% of the Age 1650-1715 Maunder Sunspot Minimum discovered mass of the entire solar system. It is held together by Mean Distance to Earth 150 Million Kilometers 1854 Fust connectionmade between solar activity gravitational attraction, producing immense pressure Rotation Period (at equator) 26.8 days andgeomagneticactivity and temperature at its core (more than a billion times Radius 695poO Kilometers Helium lines first observed in solar spectrum that of the atmosphere on Earth, and a density about First measurenent of of magnetic fields 160 times that of water). Mass 1.99 x 1030 Kilograms taken At the core the temperature is 16 million degrees K, Composition Hydrogen 7196, Helium 26.596, First radio emission from Sun observed which is sufficient to sustain thermonuclear fusion Other 2.5% First observation of solar ultraviolet using a reactions. The released energy prevents the collapse Temperature sounding- of the Sun and keeps it in gaseous form. The total Effective Surface l,OMI,OMIKtemperatureofmrona discovered energy radiated is 383 billion trillion kilowatts/sec- Energy Output (Luminosity) viacodspectralines ond, which is equivalent to that generated by 100 Solar Constant First observation of solar x-rays using a billion tons of TNT exploding each second. Inclination of Solar Equator to Ecliptic 7.2S0 sounding- In addition to the energy-producing solar core, the Galactic dcrays found to change interior has two distinct regions: a radiative and a in intensity with the 11-year sunspot cycle convective zone. From the edge of the core outward, ~argestohewed solar &re occukd - first through the radiative and then through the con- About the Image- First direct observations of solar wind made vective zone, the temperature decreases from 8 million byMariner2 to 7,000 K, and density decreases from 20 gm/cm3to 4 This image of the Sun, taken January24,1992,is ztiezoed First observations of solar gamma rays made x lo-' gm/m3. It takes about 10 million years for from space at x-ray wavelengths. The image, as seen by the by Orbiting Solar Observatory 1(OS01) photons to escape from the dense core and reach the soft X-ray Telescopeon theJapan/US/UKYohkoh Mission First mammmmt of solar neutrino flux surface. (orbiting solar obserpultory), reveals the hot, three-dimen- taken Because the Sun is gaseous, it rotates faster at the sionalgeomettyof the corona across thefill disk of the Sun. Skylab obsened Sun, discovered coronal equator (26.8 days) than at the poles (as long as 35 The large bright areas are regions where the Sun's magnetic holes as days). The Sun's "surface," known the photosphere, field is so strong that it can trap hot gases even though the 1982 First observations of neutrons from a solar is just the visible 500 km-thick layer from which most ~bySolarMaxim~~(~ temperature ofthe regions arecnrer 1 million degrees K. The of the Sun's radiation and light finally escapes, and is 1-5 UlyssesfJiesoverpolarq@onsofSun dark amare ammnl holes, which are the origin ofstrermrs the place where sunspots are found. Above the photo- Rduemca sphere lies the chromosphere ("sphere of color") that of particb, called the high speed solar wind, that flozo past 1.1&!km,"BduationrlBrisltEB-l06,NASA~W~DC may be seen briefly during total solar eclipees as a Eflrtha#dthroughthesolsr~atabout700~ reddish rim, caused by hot hydrogen atoms, around ptr=f"'d* A National Aeronautics and J Space Administration Mercury 9 - National Aeronautics and Space Administration Mercury 9 Mercury is the planet closest to the Sun. Of all the planets, the planet. Mercury also has experienced a unique Caloris basin was formed by collision of a gigantic asteroid it has the most elliptical orbit, except for Pluto. Because of geological history which has resulted in a global system of with Mercury. The strong shock wave produced by the its elliptical orbit, Mercury's closest distance to the Sun is fractures caused by shrinkage of the planet. impact traveled through the planet to instantaneously form the only 46 million km while its greatest distance is 70 million hilly, lineated terrain on the opposite side of the planet. krn. Another unique aspect of Mercury is its rotational and Soon after the planet formed it nearly melted from decay of Afterward, eruption of lava within and surrounding the orbital period. Mercury rotates on its axis once every 58.9 radioactive elements and the inward migration of iron that Caloris, and other large basins formed the smooth plains. days and circles the Sun once every 87.9 days. As a result formed its enormous core. This led to the expansion of the Over the next half billion years the core and mantle began to Mercury rotates exactly three times around its axis for planet and extensive fracturing of the surface which cool, Mercury's radius decreased by about 2 to 4 km, and the every two orbits around the Sun. If you wanted to stay up provided an exit for lava to reach the surface and form the crust was subjected to compressive stresses that resulted in a for a solar day on Mercury (sunrise to sunrise), you would smooth plains within and between the craters. At about the unique global system of fractures. As this occurred, volcan- be awake for two Mercurian years (a total of 176 Earth same time and like the other planets, Mercury was subjected ism ceased when compressive stresses in the lithosphere days.) Because Mercury is so close to the Sun, its surface to heavy bombarded by asteroidal and cometary debris left became strong enough to close off magma sources. Since that temperature has the greatest temperature range of any over from accretion of the solar system. During this early time, only occasional impacts of comets and asteroids have planet or satellite in the solar system. The surface tempera- ~eriodof heavv bombardment. the 1300 krn diameter occurred. ture reaches a maximum of 427" Celsius on the side closest to the Sun, and - 183°C on the night side. Mercury's Significant Dates Fast Facts atmosphere is tenuous and like a vacuum. The atmosphere is composed of sodium and potassium, which is probably 1610 - Italian astronomer Galileo Galilei made first Namesake Messenger of the Roman Gods derived from the surface. While Mercury does have an telescopic obersewation of Mercury. Diameter 4878 km atmosphere, it does not have satellites. 1631 - French astronomer Pierre Gassendi made first Mean Distance from Sun 57.8 million km telescopic obervations of the transit of Mercury Mass 61100 the mass of Earth Physically, Mercury is smaller than any other planet except across the face of the Sun. Density 5.44 glcc Pluto, measuring about one-third the size of Earth. 1639 - Italian astronomer Giovanni Zupus discovered Surface Temperature However, Mercury's density (5.4 g/cm3) is about the same Mercury has phases, which is evidence that the Maximum Day Side 740" Kelvin (467" C) as Earth's; therefore, scientists assume that the planet has planet circle the Sun. Maximum Night Side 90" Kelvin (-1 83" C) an enormous iron core that composes some 75 percent of 1841 - German astronomer, Johann Franz Encke made the Rotational Period 58.6 days Mercury's diameter (42 percent of the volume). The core is first mass determination using gravity effect on the Eccentricity of Orbit 0.206 surrounded by a rocky mantle and crust only about 600 km comet Encke. Rotational Period thick. Aside from Earth, Mercury is the only terrestial 1889 - Italian astronomer, Giovanni Schiaparelli produced (1 Mercury Day) 58.6 Earth days planet with a magnetic field. Although the magnetic field the first map of Mercury's surface features.