The affects of the Jovian planets
... • Uranus is the seventh planet from the sun and the third largest in the solar system • Its atmosphere consists of 83% hydrogen 15% helium and 2% methane. • Uranus has nine rings, but they are very different from those on Saturn and Jupiter. They are made up of boulders of ice and are not reflective ...
... • Uranus is the seventh planet from the sun and the third largest in the solar system • Its atmosphere consists of 83% hydrogen 15% helium and 2% methane. • Uranus has nine rings, but they are very different from those on Saturn and Jupiter. They are made up of boulders of ice and are not reflective ...
Outer Planets: The Ice Giants
... environments beneath their icy crusts. Triton, the largest satellite of Neptune, may be a captured object from the Kuiper Belt − a part of the solar nebula that never coalesced into a planet. Triton has a young surface with active geysers erupting into the thin atmosphere. Giant planets are our link ...
... environments beneath their icy crusts. Triton, the largest satellite of Neptune, may be a captured object from the Kuiper Belt − a part of the solar nebula that never coalesced into a planet. Triton has a young surface with active geysers erupting into the thin atmosphere. Giant planets are our link ...
Flat Earth / Round Earth Activity
... Here are the approximate orbital eccentricities of some solar system objects: Mercury Venus Earth Moon Mars ...
... Here are the approximate orbital eccentricities of some solar system objects: Mercury Venus Earth Moon Mars ...
Beyond Pluto: A new 9th planet? | Science News for Students
... probability of them all crossing the plane at this same point in their orbits by chance is just 0.007 percent, the Caltech team now reports. But, they add, a planet patrolling the borderlands of the solar system could shepherd all of those rocky bodies to cross the plane at the same point in their o ...
... probability of them all crossing the plane at this same point in their orbits by chance is just 0.007 percent, the Caltech team now reports. But, they add, a planet patrolling the borderlands of the solar system could shepherd all of those rocky bodies to cross the plane at the same point in their o ...
Ch 29 Our Solar System
... -In the Early 2000’s, astronmers began to notice large objects in the Kuiper belt. One such object, now named Eris is the same size or larger than Pluto. The Astronomical community then re-evaluated what the definition of planet should be. They decided on a new classification called Pluto and others ...
... -In the Early 2000’s, astronmers began to notice large objects in the Kuiper belt. One such object, now named Eris is the same size or larger than Pluto. The Astronomical community then re-evaluated what the definition of planet should be. They decided on a new classification called Pluto and others ...
Definition - SchoolNotes
... Neptune is the eighth planet in the solar system, located 30.1 AU, or 2.794 billion miles from the Sun. – It is also a gaseous planet composed of hydrogen, helium, and methane – the methane gives Neptune its blue color. – Neptune orbits the Sun in approximately 168 years and makes one complete rotat ...
... Neptune is the eighth planet in the solar system, located 30.1 AU, or 2.794 billion miles from the Sun. – It is also a gaseous planet composed of hydrogen, helium, and methane – the methane gives Neptune its blue color. – Neptune orbits the Sun in approximately 168 years and makes one complete rotat ...
Miscellaneous Questions on Asteroids/Comets/Meteoroids/Exoplane
... One of the more fascinating, still unresolved, mysteries about outer space is that very few of the extra-solar planets we observe seem to have orbits similar to those in our solar system! Either we exist in a very rare environment, or there are difficulties that have so far prevented us from detecti ...
... One of the more fascinating, still unresolved, mysteries about outer space is that very few of the extra-solar planets we observe seem to have orbits similar to those in our solar system! Either we exist in a very rare environment, or there are difficulties that have so far prevented us from detecti ...
Our Solar System
... • A meteoroid that burns up as it passes through the Earth’s atmosphere is known as a meteor. If you’ve ever looked up at the sky at night and seen a streak of light or ‘shooting star’ what you are actually seeing is a meteor. • A meteoroid that survives falling through the Earth’s atmosphere and co ...
... • A meteoroid that burns up as it passes through the Earth’s atmosphere is known as a meteor. If you’ve ever looked up at the sky at night and seen a streak of light or ‘shooting star’ what you are actually seeing is a meteor. • A meteoroid that survives falling through the Earth’s atmosphere and co ...
Asteroids comets meteoroids
... Near-Earth Asteroids “NEA” Asteroids whose orbits bring them close to earth. – More than 1,000 – Possible dangers to earth – Example: Meteor crater, Arizona 50 m asteroid 1 km crater 40,000 years ago • NASA has a congressional mandate to catalog all near-Earth objects. ...
... Near-Earth Asteroids “NEA” Asteroids whose orbits bring them close to earth. – More than 1,000 – Possible dangers to earth – Example: Meteor crater, Arizona 50 m asteroid 1 km crater 40,000 years ago • NASA has a congressional mandate to catalog all near-Earth objects. ...
Chapter 12 Asteroids, Comets, and Dwarf Planets What are
... • Pluto will never hit Neptune, even though their orbits cross, because of 3:2 orbital resonance • Neptune orbits three times during the time Pluto orbits twice ...
... • Pluto will never hit Neptune, even though their orbits cross, because of 3:2 orbital resonance • Neptune orbits three times during the time Pluto orbits twice ...
GEOL3025, Section 030 Lecture #11 31 August 2007
... AKA Jovian Planets (like Jupiter) Gas Giants: Jupiter & Saturn Ice Giants: Uranus & Neptune + Pluto (Rocky-Ice planet?) ...
... AKA Jovian Planets (like Jupiter) Gas Giants: Jupiter & Saturn Ice Giants: Uranus & Neptune + Pluto (Rocky-Ice planet?) ...
The Milky Way
... populated by smaller objects. The asteroid belt, which lies between Mars and Jupiter, is similar to the terrestrial planets as it is composed mainly of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc; linked populations of trans-Neptunian objects composed mostly of ices ...
... populated by smaller objects. The asteroid belt, which lies between Mars and Jupiter, is similar to the terrestrial planets as it is composed mainly of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc; linked populations of trans-Neptunian objects composed mostly of ices ...
The Milky Way
... populated by smaller objects. The asteroid belt, which lies between Mars and Jupiter, is similar to the terrestrial planets as it is composed mainly of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc; linked populations of trans-Neptunian objects composed mostly of ices ...
... populated by smaller objects. The asteroid belt, which lies between Mars and Jupiter, is similar to the terrestrial planets as it is composed mainly of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc; linked populations of trans-Neptunian objects composed mostly of ices ...
Gas Planets
... Gas Planet – a large planet that has a deep, massive atmosphere Planetary Ring – a disk of matter that circles a planet and consists of numerous particles in orbit that range in size from a few millimeters to several hundred meters. ...
... Gas Planet – a large planet that has a deep, massive atmosphere Planetary Ring – a disk of matter that circles a planet and consists of numerous particles in orbit that range in size from a few millimeters to several hundred meters. ...
THE SOLAR SYSTEM
... Jupiter is the largest planet in the solar system. Its diameter is 88,846 miles (142,984 kilometers), more than 11 times that of Earth, and about onetenth that of the sun. It would take more than 1,000 Earths to fill up the volume of the giant planet. It is usually the second brightest planet—after ...
... Jupiter is the largest planet in the solar system. Its diameter is 88,846 miles (142,984 kilometers), more than 11 times that of Earth, and about onetenth that of the sun. It would take more than 1,000 Earths to fill up the volume of the giant planet. It is usually the second brightest planet—after ...
THE SOLAR SYSTEM
... Jupiter is the largest planet in the solar system. Its diameter is 88,846 miles (142,984 kilometers), more than 11 times that of Earth, and about onetenth that of the sun. It would take more than 1,000 Earths to fill up the volume of the giant planet. It is usually the second brightest planet—after ...
... Jupiter is the largest planet in the solar system. Its diameter is 88,846 miles (142,984 kilometers), more than 11 times that of Earth, and about onetenth that of the sun. It would take more than 1,000 Earths to fill up the volume of the giant planet. It is usually the second brightest planet—after ...
The Milky Way - Drage Homepage
... populated by smaller objects. The asteroid belt, which lies between Mars and Jupiter, is similar to the terrestrial planets as it is composed mainly of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc; linked populations of trans-Neptunian objects composed mostly of ices ...
... populated by smaller objects. The asteroid belt, which lies between Mars and Jupiter, is similar to the terrestrial planets as it is composed mainly of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc; linked populations of trans-Neptunian objects composed mostly of ices ...
Document
... Rocky masses that revolve around Sun; usually between Mars and Jupiter Debris left over by a planet that failed to from (about 2.8 AU from Sun) Need a telescope to view them Largest is Ceres (578 mi wide) ...
... Rocky masses that revolve around Sun; usually between Mars and Jupiter Debris left over by a planet that failed to from (about 2.8 AU from Sun) Need a telescope to view them Largest is Ceres (578 mi wide) ...
The Solar System At least 7 billion miles across, home to 8 planets
... At 4.6 billion years old, is the solar system. Its planets, including our own Earth, formed out of what was left over after the birth of the sun. Amazingly, these 8 massive, celestial bodies grew out of tiny specs of dust orbiting the new star. Time and again the young planets collided with floating ...
... At 4.6 billion years old, is the solar system. Its planets, including our own Earth, formed out of what was left over after the birth of the sun. Amazingly, these 8 massive, celestial bodies grew out of tiny specs of dust orbiting the new star. Time and again the young planets collided with floating ...
The tenth planet by Francis Reddy November 2005
... that is, he says, not only the farthest directly observed body in the solar system and the fourth brightest Kuiper Belt object. It is also our solar system’s tenth planet. Since beginning a 5-year, all-sky survey with Palomar Observatory’s 48-inch Samuel Oschin Telescope in 2001, Brown and his colle ...
... that is, he says, not only the farthest directly observed body in the solar system and the fourth brightest Kuiper Belt object. It is also our solar system’s tenth planet. Since beginning a 5-year, all-sky survey with Palomar Observatory’s 48-inch Samuel Oschin Telescope in 2001, Brown and his colle ...
Chapter 8
... inner particles revolve faster than those farther out ring are not rotating as a solid body, rather individual moonlets are revolving around the planet If ring particles are widely spaced, they move independently If the particles are close to each other, there is a gravitationally interaction be ...
... inner particles revolve faster than those farther out ring are not rotating as a solid body, rather individual moonlets are revolving around the planet If ring particles are widely spaced, they move independently If the particles are close to each other, there is a gravitationally interaction be ...
Chapter 12 (in pdf)
... • Kuiper belt comets formed in the Kuiper belt: flat plane, aligned with the plane of planetary orbits, orbiting in the same direction as the planets. • Oort cloud comets were once closer to the Sun, but they were kicked out there by gravitational interactions with jovian planets: spherical distri ...
... • Kuiper belt comets formed in the Kuiper belt: flat plane, aligned with the plane of planetary orbits, orbiting in the same direction as the planets. • Oort cloud comets were once closer to the Sun, but they were kicked out there by gravitational interactions with jovian planets: spherical distri ...
lecture 3
... strong evidence for hyperbolic comets (interstellar comets would have 1/a ~ -1 AU-1) ...
... strong evidence for hyperbolic comets (interstellar comets would have 1/a ~ -1 AU-1) ...
Kuiper belt
The Kuiper belt /ˈkaɪpər/ or /'køypǝr/ (as in Dutch), sometimes called the Edgeworth–Kuiper belt, is a region of the Solar System beyond the planets, extending from the orbit of Neptune (at 30 AU) to approximately 50 AU from the Sun. It is similar to the asteroid belt, but it is far larger—20 times as wide and 20 to 200 times as massive. Like the asteroid belt, it consists mainly of small bodies, or remnants from the Solar System's formation. Although many asteroids are composed primarily of rock and metal, most Kuiper belt objects are composed largely of frozen volatiles (termed ""ices""), such as methane, ammonia and water. The Kuiper belt is home to three officially recognized dwarf planets: Pluto, Haumea, and Makemake. Some of the Solar System's moons, such as Neptune's Triton and Saturn's Phoebe, are also thought to have originated in the region.The Kuiper belt was named after Dutch-American astronomer Gerard Kuiper, though he did not actually predict its existence. In 1992, 1992 QB1 was discovered, the first Kuiper belt object (KBO) since Pluto. Since its discovery, the number of known KBOs has increased to over a thousand, and more than 100,000 KBOs over 100 km (62 mi) in diameter are thought to exist. The Kuiper belt was initially thought to be the main repository for periodic comets, those with orbits lasting less than 200 years. However, studies since the mid-1990s have shown that the belt is dynamically stable, and that comets' true place of origin is the scattered disc, a dynamically active zone created by the outward motion of Neptune 4.5 billion years ago; scattered disc objects such as Eris have extremely eccentric orbits that take them as far as 100 AU from the Sun.The Kuiper belt should not be confused with the hypothesized Oort cloud, which is a thousand times more distant and is not flat. The objects within the Kuiper belt, together with the members of the scattered disc and any potential Hills cloud or Oort cloud objects, are collectively referred to as trans-Neptunian objects (TNOs).Pluto is likely the largest and most-massive member of the Kuiper belt and the largest and the second-most-massive known TNO, surpassed only by Eris in the scattered disc. Originally considered a planet, Pluto's status as part of the Kuiper belt caused it to be reclassified as a dwarf planet in 2006. It is compositionally similar to many other objects of the Kuiper belt, and its orbital period is characteristic of a class of KBOs, known as ""plutinos"", that share the same 2:3 resonance with Neptune.