Rotation and Revolution - Environmental Science Institute
... 7. Discuss with the students what is he drawing and why is he drawing it. What planet follows this orbit? Why does a planet follow an orbit? 8. Make an orbit for each planet for the students to follow. 9. Finally, ask the students with the planets to move in their orbits. Remind them that a planet n ...
... 7. Discuss with the students what is he drawing and why is he drawing it. What planet follows this orbit? Why does a planet follow an orbit? 8. Make an orbit for each planet for the students to follow. 9. Finally, ask the students with the planets to move in their orbits. Remind them that a planet n ...
solar system websearch
... system and _______________ is the largest planetary moon. F. Saturn is known for its __________. Saturn's largest moon is called _____________________. ...
... system and _______________ is the largest planetary moon. F. Saturn is known for its __________. Saturn's largest moon is called _____________________. ...
The Solar System Information Pack
... sun (and the new planet that has been found!). The relative sizes of the planets and their distance from the sun. The sun is a star at the centre of our solar system. The sun, earth and moon are approximately spherical bodies. That some of the planets have moons and the number of moons for e ...
... sun (and the new planet that has been found!). The relative sizes of the planets and their distance from the sun. The sun is a star at the centre of our solar system. The sun, earth and moon are approximately spherical bodies. That some of the planets have moons and the number of moons for e ...
File
... around, forming an accretion disk. ►Sun formed in the middle from all the heat in the middle of the disk 3.Cooling of the disk caused small shapes to form 4. These cool forms combined to make the 4 SOLID inner planets ...
... around, forming an accretion disk. ►Sun formed in the middle from all the heat in the middle of the disk 3.Cooling of the disk caused small shapes to form 4. These cool forms combined to make the 4 SOLID inner planets ...
Where Are We Going?
... Sun. What do you notice about the sizes of the orbits? Compare the orbits near the Sun with those farther away from the Sun. If you were the commander of a spacebus that traveled among the planets, would you rather travel between the Inner Planets (Mercury, Venus, Earth, Mars) or the Outer Planets ( ...
... Sun. What do you notice about the sizes of the orbits? Compare the orbits near the Sun with those farther away from the Sun. If you were the commander of a spacebus that traveled among the planets, would you rather travel between the Inner Planets (Mercury, Venus, Earth, Mars) or the Outer Planets ( ...
planets of our solar system
... Solar System. It is one of the gas giants--big planets made of gas. It is best known for its rings, which can be seen only through a telescope. Saturn’s rings were first seen by Galileo Galilei in ...
... Solar System. It is one of the gas giants--big planets made of gas. It is best known for its rings, which can be seen only through a telescope. Saturn’s rings were first seen by Galileo Galilei in ...
Comets…
... Small objects in the Solar System Meteors, Comets, : we see them without a telescope Asteroids: small rocky objects mostly between Mars and Jupiter – too faint to see without a telescope Kuiper belt objects: even fainter objects beyond Pluto, debris left over from solar system formation Image of co ...
... Small objects in the Solar System Meteors, Comets, : we see them without a telescope Asteroids: small rocky objects mostly between Mars and Jupiter – too faint to see without a telescope Kuiper belt objects: even fainter objects beyond Pluto, debris left over from solar system formation Image of co ...
Formation of the Solar System Reading Questions
... 6. Watch the animation of the formation of a star cluster. The process is also similar to how a solar system forms. There are two outcomes for new stars that come near a region of high density in a cloud of condensing gas and dust. What are they? ...
... 6. Watch the animation of the formation of a star cluster. The process is also similar to how a solar system forms. There are two outcomes for new stars that come near a region of high density in a cloud of condensing gas and dust. What are they? ...
Solar System - Bishop Seabury Academy
... Spectroscopy reveals the chemical composition of the planets • The spectrum of a planet or satellite with an atmosphere reveals the atmosphere’s composition • If there is no atmosphere, the spectrum indicates the composition of the surface. • The substances that make up the planets can be classi ...
... Spectroscopy reveals the chemical composition of the planets • The spectrum of a planet or satellite with an atmosphere reveals the atmosphere’s composition • If there is no atmosphere, the spectrum indicates the composition of the surface. • The substances that make up the planets can be classi ...
Terrestrial or Inner Planets
... • If there is no atmosphere, the spectrum indicates the composition of the surface. • The substances that make up the planets can be classified as gases, ices, or rock, depending on the temperatures at which they solidify • The terrestrial planets are composed primarily of rocky materials, whereas t ...
... • If there is no atmosphere, the spectrum indicates the composition of the surface. • The substances that make up the planets can be classified as gases, ices, or rock, depending on the temperatures at which they solidify • The terrestrial planets are composed primarily of rocky materials, whereas t ...
What do you think about the origin of most of Jupiter`s moons?
... • Neptune moved rapidly outward. Its elliptical orbit settled down to circular by exchanging angular momentum with the Kuiper objects. ...
... • Neptune moved rapidly outward. Its elliptical orbit settled down to circular by exchanging angular momentum with the Kuiper objects. ...
The Search for Planet X
... Earth’s moon. Its meager gravity could not possibly explain anomalies in the orbits of Neptune and Uranus—which turned out to be just as well because those anomalies faded away on further inspection. In that sense, Pluto was a false alarm. In the big picture, however, its discovery was extraordinar ...
... Earth’s moon. Its meager gravity could not possibly explain anomalies in the orbits of Neptune and Uranus—which turned out to be just as well because those anomalies faded away on further inspection. In that sense, Pluto was a false alarm. In the big picture, however, its discovery was extraordinar ...
Midterm Exam: Chs. 1-3, 7-11
... ____ 24. Which of the following is a necessary condition for lunar or solar eclipses? a. The Earth must be on the celestial equator. b. The Sun must be on the celestial equator. c. The Sun must be close to or crossing the ecliptic plane. d. The Moon must be close to or crossing the ecliptic plane. ...
... ____ 24. Which of the following is a necessary condition for lunar or solar eclipses? a. The Earth must be on the celestial equator. b. The Sun must be on the celestial equator. c. The Sun must be close to or crossing the ecliptic plane. d. The Moon must be close to or crossing the ecliptic plane. ...
Asteroids
... meteor, starfield, and even a moonbow all vying for attention. It is interesting to first note, though, what can't be seen -- a rising moon on the other side of the camera. The bright moon not only illuminated this beautiful landscape in Queensland, Australia last June, but also created the beautifu ...
... meteor, starfield, and even a moonbow all vying for attention. It is interesting to first note, though, what can't be seen -- a rising moon on the other side of the camera. The bright moon not only illuminated this beautiful landscape in Queensland, Australia last June, but also created the beautifu ...
The Solar System
... square of the period of revolution of a planet (in years) is proportional to the cube of the average distance of the planet from the sun (in astronomical units, AU, the average sun-earth distance) ...
... square of the period of revolution of a planet (in years) is proportional to the cube of the average distance of the planet from the sun (in astronomical units, AU, the average sun-earth distance) ...
The Stars
... The patterns of stars in the sky stay the same, although they appear to move across the sky nightly, and different stars can be seen in different seasons. Telescopes magnify the appearance of some distant objects in the sky, including the moon and the planets. The number of stars that can be see ...
... The patterns of stars in the sky stay the same, although they appear to move across the sky nightly, and different stars can be seen in different seasons. Telescopes magnify the appearance of some distant objects in the sky, including the moon and the planets. The number of stars that can be see ...
What are the Jovian Planets? Characteristics of Jovian Planets
... Storms on Saturn • Large storms are rarer • Connected with seasons • ~ every 30 years outbreak of spots are seen in the equatorial ...
... Storms on Saturn • Large storms are rarer • Connected with seasons • ~ every 30 years outbreak of spots are seen in the equatorial ...
Planets
... conceptualize them c. Geometry correctly inferred by Huygens in 1659 d. Complex Composed of small particles (moonlets) that orbit it 1) Most rings fall into two categories based on particle density a) Main rings contain particles from a few centimeters to several meters in diameter Page 5 of 6 ...
... conceptualize them c. Geometry correctly inferred by Huygens in 1659 d. Complex Composed of small particles (moonlets) that orbit it 1) Most rings fall into two categories based on particle density a) Main rings contain particles from a few centimeters to several meters in diameter Page 5 of 6 ...
Nebular Hypothesis
... material that’s currently in the planets, and then add enough volatile materials (mainly H & He) to “reconstitute” a gas disk with the same composition as the Sun. ...
... material that’s currently in the planets, and then add enough volatile materials (mainly H & He) to “reconstitute” a gas disk with the same composition as the Sun. ...
g9u4c12part3
... consume their fuel faster than smaller stars Become red giants. (supergiants) last for only 7 billion years. they collapse in on themselves causing a massive explosion called a supernova. the remaining core of the supernova will eventually collapse to form a neutron star. A sphere only 10 km ...
... consume their fuel faster than smaller stars Become red giants. (supergiants) last for only 7 billion years. they collapse in on themselves causing a massive explosion called a supernova. the remaining core of the supernova will eventually collapse to form a neutron star. A sphere only 10 km ...
EARTH-CENTERED MODELS OF THE SOLAR SYSTEM
... The planets in order from biggest to smallest are: Jupiter, Saturn, Uranus, Neptune, Earth, Venus, Mars, Mercury. ...
... The planets in order from biggest to smallest are: Jupiter, Saturn, Uranus, Neptune, Earth, Venus, Mars, Mercury. ...
Definition of planet
The definition of planet, since the word was coined by the ancient Greeks, has included within its scope a wide range of celestial bodies. Greek astronomers employed the term asteres planetai (ἀστέρες πλανῆται), ""wandering stars"", for star-like objects which apparently moved over the sky. Over the millennia, the term has included a variety of different objects, from the Sun and the Moon to satellites and asteroids.By the end of the 19th century the word planet, though it had yet to be defined, had become a working term applied only to a small set of objects in the Solar System. After 1992, however, astronomers began to discover many additional objects beyond the orbit of Neptune, as well as hundreds of objects orbiting other stars. These discoveries not only increased the number of potential planets, but also expanded their variety and peculiarity. Some were nearly large enough to be stars, while others were smaller than Earth's moon. These discoveries challenged long-perceived notions of what a planet could be.The issue of a clear definition for planet came to a head in 2005 with the discovery of the trans-Neptunian object Eris, a body more massive than the smallest then-accepted planet, Pluto. In its 2006 response, the International Astronomical Union (IAU), recognised by astronomers as the world body responsible for resolving issues of nomenclature, released its decision on the matter. This definition, which applies only to the Solar System, states that a planet is a body that orbits the Sun, is massive enough for its own gravity to make it round, and has ""cleared its neighbourhood"" of smaller objects around its orbit. Under this new definition, Pluto and the other trans-Neptunian objects do not qualify as planets. The IAU's decision has not resolved all controversies, and while many scientists have accepted the definition, some in the astronomical community have rejected it outright.