Solar System Data Sheet
... Superior Planets (having an orbit farther from the Sun than Earth) – Mars, Jupiter, Saturn, Uranus, Neptune Giant Planets (larger than Earth) - Jupiter, Saturn, Uranus, Neptune Small Planets (smaller than Earth) – Mercury, Venus, Mars ...
... Superior Planets (having an orbit farther from the Sun than Earth) – Mars, Jupiter, Saturn, Uranus, Neptune Giant Planets (larger than Earth) - Jupiter, Saturn, Uranus, Neptune Small Planets (smaller than Earth) – Mercury, Venus, Mars ...
The Planet Walk Brochure - Take it on the walk for fun on the go
... To begin, visit the Sun station on the corner of 5th Avenue and “G” Street. The map will guide you. Then proceed down 5th Avenue, following the signs to each of the four inner planet stations: Mercury, Venus, Earth, and Mars. If you’re up for more, you can continue the Planet Walk along the Tony Kno ...
... To begin, visit the Sun station on the corner of 5th Avenue and “G” Street. The map will guide you. Then proceed down 5th Avenue, following the signs to each of the four inner planet stations: Mercury, Venus, Earth, and Mars. If you’re up for more, you can continue the Planet Walk along the Tony Kno ...
solarsystem_intermed..
... object we have found in our Solar System. For fun, we have calculated how far away it would be on our scale: between 45-450m (it has a very elliptical orbit). Alpha Centauri is the closest star to us at ~4 light years away. On the same scale, Alpha Centauri would be ~125 km away! What hope do we hav ...
... object we have found in our Solar System. For fun, we have calculated how far away it would be on our scale: between 45-450m (it has a very elliptical orbit). Alpha Centauri is the closest star to us at ~4 light years away. On the same scale, Alpha Centauri would be ~125 km away! What hope do we hav ...
The Solar System
... planets were left as collections of metal and rock. • The inner planets are Mercury, Venus, Earth and Mars. ...
... planets were left as collections of metal and rock. • The inner planets are Mercury, Venus, Earth and Mars. ...
Who Wants To Be A Millionaire?
... Terrestrial planets Far away from the sun Gas giants Very small ...
... Terrestrial planets Far away from the sun Gas giants Very small ...
Worksheet 1
... R. Microscopic solid dust particles in interstellar space S. An object that orbits the Sun and is massive enough that its gravity compresses it into an approximately spherical shape. However, it has not swept its orbital region clear of other objects of comparable mass T. A small, generally rocky, s ...
... R. Microscopic solid dust particles in interstellar space S. An object that orbits the Sun and is massive enough that its gravity compresses it into an approximately spherical shape. However, it has not swept its orbital region clear of other objects of comparable mass T. A small, generally rocky, s ...
High-velocity collisions from the lunar cataclysm recorded in
... the orbits of the surviving test asteroids were reasonably similar to those of the present main belt. Note that the population of Earth/Moon-crossing asteroids generated as a result of the giant planet migration has been shown to fit the LHB-era lunar cratering record16 , the crater size-frequency d ...
... the orbits of the surviving test asteroids were reasonably similar to those of the present main belt. Note that the population of Earth/Moon-crossing asteroids generated as a result of the giant planet migration has been shown to fit the LHB-era lunar cratering record16 , the crater size-frequency d ...
ori pro 02 semifin [sfn] - SwRI Boulder
... The latter possibility has particularly interesting ramifications. The paper reporting our investigations of this hypothesis (Levison et al. 2001; Appendix D) considers the effects of a plausible, late formation of Uranus and Neptune on neighboring icy planetesimals. Their transport would have cause ...
... The latter possibility has particularly interesting ramifications. The paper reporting our investigations of this hypothesis (Levison et al. 2001; Appendix D) considers the effects of a plausible, late formation of Uranus and Neptune on neighboring icy planetesimals. Their transport would have cause ...
Comets, asteroids, and meteors oh my!
... • Too small and too numerous to be planets • Common in the in the inner solar system • Chunks of rock and metal, no tail like a comet • There is an asteroid belt – This belt is located between Mars and Jupiter ...
... • Too small and too numerous to be planets • Common in the in the inner solar system • Chunks of rock and metal, no tail like a comet • There is an asteroid belt – This belt is located between Mars and Jupiter ...
Review for Test #2 March 9
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
Pocket Solar System - Faculty Web Sites at the University of Virginia
... Solar System moves relative to one planet www.gunn.co.nz/astrotour/?data=tours/retrograde.xml ...
... Solar System moves relative to one planet www.gunn.co.nz/astrotour/?data=tours/retrograde.xml ...
mid term exam crossword
... 116. explained the forces involved with an orbiting object 117. path of a revolving object, Pluto's _____ ...
... 116. explained the forces involved with an orbiting object 117. path of a revolving object, Pluto's _____ ...
Meteorites
... • About 20 meteorites (out of >20,000) have been identified as Moon rocks from their chemistry and isotopes. • Most are breccias from the highlands. • A few are mare basalt (volcanic) samples. • These rocks are free (but random) samples of different places on the Moon than those sampled by Apollo mi ...
... • About 20 meteorites (out of >20,000) have been identified as Moon rocks from their chemistry and isotopes. • Most are breccias from the highlands. • A few are mare basalt (volcanic) samples. • These rocks are free (but random) samples of different places on the Moon than those sampled by Apollo mi ...
The Inner Planets - sciencewithskinner
... • _____________ planet in the solar system with over twice the mass of ______________________ combined. • ________________________: a giant storm about twice the size of Earth. ...
... • _____________ planet in the solar system with over twice the mass of ______________________ combined. • ________________________: a giant storm about twice the size of Earth. ...
The Solar System - Kennesaw State University
... shapes in the sky. They were given their names many hundreds of years ago to help us remember which stars are which. We use constellations to divide up the sky; finding one can help us find another because constellations move so slowly that, in our lifetime, they will always be found in about the sa ...
... shapes in the sky. They were given their names many hundreds of years ago to help us remember which stars are which. We use constellations to divide up the sky; finding one can help us find another because constellations move so slowly that, in our lifetime, they will always be found in about the sa ...
The Center of It All
... surfaces and is primarily composed of silicate racks and/or metals. There are 4 known terrestrial planets in our solar system – Mercury, Venus, Earth and Mars, which are all inner planets and one terrestrial dwarf planet, Ceres, located in the asteroid belt. ...
... surfaces and is primarily composed of silicate racks and/or metals. There are 4 known terrestrial planets in our solar system – Mercury, Venus, Earth and Mars, which are all inner planets and one terrestrial dwarf planet, Ceres, located in the asteroid belt. ...
Planets - Cloudfront.net
... Occasionally, the ninth planet Pluto crosses Neptune's orbit and becomes the "eighth planet". Its bluish color comes from its atmosphere of methane gas. The planet has 13 moons and a very ...
... Occasionally, the ninth planet Pluto crosses Neptune's orbit and becomes the "eighth planet". Its bluish color comes from its atmosphere of methane gas. The planet has 13 moons and a very ...
Solar System Reading Packet
... times larger than it does on Earth. When the Sun is overhead on Mercury, the temperature rises to about 430°C ...
... times larger than it does on Earth. When the Sun is overhead on Mercury, the temperature rises to about 430°C ...
BIO 10 Lecture 2
... “contaminated” with the heavier elements produced by the supernova of another star • ~ 4.5 billion years ago, The Earth formed from the same spinning disk that formed the Sun. • Metals and other heavy elements remained closer to the sun; gaseous planets like Jupiter and Saturn formed farther out ...
... “contaminated” with the heavier elements produced by the supernova of another star • ~ 4.5 billion years ago, The Earth formed from the same spinning disk that formed the Sun. • Metals and other heavy elements remained closer to the sun; gaseous planets like Jupiter and Saturn formed farther out ...
Slide 1
... Where can you find them? • In the Asteroid Belt between Mars and Jupiter. • There are thousands of known and lots more discovered every year. • Ceres is the largest with a diameter of 974 km • All the asteroids put together would not even be half of the moons mass. http://upload.wikimedia.org/wikip ...
... Where can you find them? • In the Asteroid Belt between Mars and Jupiter. • There are thousands of known and lots more discovered every year. • Ceres is the largest with a diameter of 974 km • All the asteroids put together would not even be half of the moons mass. http://upload.wikimedia.org/wikip ...
Powerpoint for today
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
... Rocky fragments ranging from 940 km across (Ceres) to < 0.1 km. 100,000 known. Most in Asteroid Belt, at about 2-3 AU, between Mars and Jupiter. The Trojan asteroids orbit 60 o ahead of and behind Jupiter. Some asteroids cross Earth's orbit. Their orbits were probably disrupted by Jupiter's gravity. ...
Relative sizes of astronomical objects
... This image represents the relative sizes of our Sun and Sirius (Alpha Canis Majoris), Pollux (Beta Geminorum) and Arcturus (Alpha Bootes). ‘Giant’ Jupiter is just 1 pixel in this perspective. Earth is invisible on this scale. ...
... This image represents the relative sizes of our Sun and Sirius (Alpha Canis Majoris), Pollux (Beta Geminorum) and Arcturus (Alpha Bootes). ‘Giant’ Jupiter is just 1 pixel in this perspective. Earth is invisible on this scale. ...
Late Heavy Bombardment
The Late Heavy Bombardment (abbreviated LHB and also known as the lunar cataclysm) is a hypothetical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, corresponding to the Neohadean and Eoarchean eras on Earth. During this interval, a disproportionately large number of asteroids apparently collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars. The LHB happened after the Earth and other rocky planets had formed and accreted most of their mass, but still quite early in Earth's history.Evidence for the LHB derives from lunar samples brought back by the Apollo astronauts. Isotopic dating of Moon rocks implies that most impact melts occurred in a rather narrow interval of time. Several hypotheses are now offered to explain the apparent spike in the flux of impactors (i.e. asteroids and comets) in the inner Solar System, but no consensus yet exists. The Nice model is popular among planetary scientists; it postulates that the gas giant planets underwent orbital migration and scattered objects in the asteroid and/or Kuiper belts into eccentric orbits, and thereby into the path of the terrestrial planets. Other researchers argue that the lunar sample data do not require a cataclysmic cratering event near 3.9 Ga, and that the apparent clustering of impact melt ages near this time is an artifact of sampling materials retrieved from a single large impact basin. They also note that the rate of impact cratering could be significantly different between the outer and inner zones of the Solar System.