here
... By far the smallest planet. Not a gas giant like other outer planets. Has an icy composition like a comet. Has a very elliptical, inclined orbit. Pluto has more in common with comets than with the eight major planets ...
... By far the smallest planet. Not a gas giant like other outer planets. Has an icy composition like a comet. Has a very elliptical, inclined orbit. Pluto has more in common with comets than with the eight major planets ...
Integrative Studies 410 Our Place in the Universe
... when and for how long in the Hertzsprung-Russell ...
... when and for how long in the Hertzsprung-Russell ...
Exploring the Outer Solar System Jane Luu When I was
... than 200 yrs to go around the Sun) originated in the Oort cloud, a large, spherical cloud located at roughly 50,000 AU (Oort 1950). Based on the long-period comets’ large, randomly oriented orbits, Oort inferred that they comets must come from a spherical cloud of comets about 105 AU away. At this k ...
... than 200 yrs to go around the Sun) originated in the Oort cloud, a large, spherical cloud located at roughly 50,000 AU (Oort 1950). Based on the long-period comets’ large, randomly oriented orbits, Oort inferred that they comets must come from a spherical cloud of comets about 105 AU away. At this k ...
printer-friendly sample test questions
... 1st Item Specification: Recognize the difference between moons, asteroids, and comets. Depth of Knowledge Level 1 1. Each of the following are objects found in our solar system EXCEPT A. quasars. B. comets. C. asteroids. D. planets. 2. Planets known to have rings include each of the following EXCEPT ...
... 1st Item Specification: Recognize the difference between moons, asteroids, and comets. Depth of Knowledge Level 1 1. Each of the following are objects found in our solar system EXCEPT A. quasars. B. comets. C. asteroids. D. planets. 2. Planets known to have rings include each of the following EXCEPT ...
Ch 12 slides - UNLV Physics
... •! These large, icy objects have orbits similar to the smaller objects in the Kuiper Belt that become short period comets •! So are they very large comets or very small planets? ...
... •! These large, icy objects have orbits similar to the smaller objects in the Kuiper Belt that become short period comets •! So are they very large comets or very small planets? ...
Document
... QuickTime™ and a TIFF (Uncomp resse d) de co mpres sor a re ne eded to see this picture . ...
... QuickTime™ and a TIFF (Uncomp resse d) de co mpres sor a re ne eded to see this picture . ...
Arguments for the presence of a distant large undiscovered Solar
... The mass of the hypothetical object would presumably be large compared with those of the known planets, in order to produce a detectable family of comets. However, the mass cannot be too large or it would be subject to energy-releasing nuclear reactions (Saumon et al. 1995) that would make the objec ...
... The mass of the hypothetical object would presumably be large compared with those of the known planets, in order to produce a detectable family of comets. However, the mass cannot be too large or it would be subject to energy-releasing nuclear reactions (Saumon et al. 1995) that would make the objec ...
Arguments for the presence of a distant large
... The mass of the hypothetical object would presumably be large compared with those of the known planets, in order to produce a detectable family of comets. However, the mass cannot be too large or it would be subject to energy-releasing nuclear reactions (Saumon et al. 1995) that would make the objec ...
... The mass of the hypothetical object would presumably be large compared with those of the known planets, in order to produce a detectable family of comets. However, the mass cannot be too large or it would be subject to energy-releasing nuclear reactions (Saumon et al. 1995) that would make the objec ...
Arguments for the presence of a distant large undiscovered Solar
... The mass of the hypothetical object would presumably be large compared with those of the known planets, in order to produce a detectable family of comets. However, the mass cannot be too large or it would be subject to energy-releasing nuclear reactions (Saumon et al. 1995) that would make the objec ...
... The mass of the hypothetical object would presumably be large compared with those of the known planets, in order to produce a detectable family of comets. However, the mass cannot be too large or it would be subject to energy-releasing nuclear reactions (Saumon et al. 1995) that would make the objec ...
Minor bodies - Polarisation.eu
... - Strongly affected by solar wind. - Exact outwards direction. * Dust tail (silicate and carbon dust grains): - Weakly affected by radiative pressure. - Slightly inclined to the outward direction. ...
... - Strongly affected by solar wind. - Exact outwards direction. * Dust tail (silicate and carbon dust grains): - Weakly affected by radiative pressure. - Slightly inclined to the outward direction. ...
12_LectureOutlines
... • Extinction level events ~ millions of years. • Major damage ~ tens to hundreds of years. ...
... • Extinction level events ~ millions of years. • Major damage ~ tens to hundreds of years. ...
Lesson #1: Introduction to the Solar System
... planets, are primarily composed of rock and metal. The four outer planets, Jupiter, Saturn, Uranus and Neptune, also called the gas giants, are composed largely of hydrogen and helium and are far more massive than the terrestrials. The Solar System is also home to two main belts of small bodies. The ...
... planets, are primarily composed of rock and metal. The four outer planets, Jupiter, Saturn, Uranus and Neptune, also called the gas giants, are composed largely of hydrogen and helium and are far more massive than the terrestrials. The Solar System is also home to two main belts of small bodies. The ...
Lecture Notes-PPT
... collect together by gravity. During the exchange of energy between the stars, some stars reach escape velocity from the protocluster and become runaway stars. The rest become gravitationally bound, meaning they will exist as collection orbiting each other forever. ...
... collect together by gravity. During the exchange of energy between the stars, some stars reach escape velocity from the protocluster and become runaway stars. The rest become gravitationally bound, meaning they will exist as collection orbiting each other forever. ...
Biblical Astrophysics - The Call of the Bride
... parable beginning to emerging. It occurred to me that some of the asteroids have been saved by the king (Jupiter). Some follow behind the red dragon (unknown destroyer object). But, many still orbit in the valley of decision? I am still unsure if I am seeing this clearly, but if there was a planet b ...
... parable beginning to emerging. It occurred to me that some of the asteroids have been saved by the king (Jupiter). Some follow behind the red dragon (unknown destroyer object). But, many still orbit in the valley of decision? I am still unsure if I am seeing this clearly, but if there was a planet b ...
E8B2_CRT_CR_MSTIPS_Final
... Response addresses all parts of the question clearly and correctly. A. Asteroids and comets are similar in that both revolve around the Sun in measurable orbits. Differences are that asteroids orbit within the plane of the ecliptic and generally in the same direction of revolution, while the orbits ...
... Response addresses all parts of the question clearly and correctly. A. Asteroids and comets are similar in that both revolve around the Sun in measurable orbits. Differences are that asteroids orbit within the plane of the ecliptic and generally in the same direction of revolution, while the orbits ...
Comet Catalina 2016 - Fraser Heights Chess Club
... Comets formed at the same time our solar system did, 4.6 billion years ago, perhaps even in among the planets. By examining them up close with satellites and landers, scientists hope to learn more about what our Solar System looked like in its earliest days. ...
... Comets formed at the same time our solar system did, 4.6 billion years ago, perhaps even in among the planets. By examining them up close with satellites and landers, scientists hope to learn more about what our Solar System looked like in its earliest days. ...
The cometary zoo
... • The big variability of D/H in comets points to the fact that they were formed over a large region, that the comet families (Oort cloud, Kuiper belt, etc.) were not formed separately, but just have a dynamically different history • The Earth did not get the bulk of its water from comets ...
... • The big variability of D/H in comets points to the fact that they were formed over a large region, that the comet families (Oort cloud, Kuiper belt, etc.) were not formed separately, but just have a dynamically different history • The Earth did not get the bulk of its water from comets ...
Lecture14
... • Stars are born from this gas and dust, collectively known as the interstellar medium. • During their lifetime, stars may return some material to the ISM through surface winds or explosive events ...
... • Stars are born from this gas and dust, collectively known as the interstellar medium. • During their lifetime, stars may return some material to the ISM through surface winds or explosive events ...
Comets, Meteors, and Asteroids Oh My!! Terms
... • A comets tail ALWAYS points away from the sun ...
... • A comets tail ALWAYS points away from the sun ...
Chapter 8 (in pdf)
... Which of these facts is NOT explained by the nebular theory? a) There are two main types of planets: terrestrial and jovian. b) Planets orbit in same direction and plane. c) Existence of asteroids and comets. d) Number of planets of each type (4 terrestrial and 4 jovian). ...
... Which of these facts is NOT explained by the nebular theory? a) There are two main types of planets: terrestrial and jovian. b) Planets orbit in same direction and plane. c) Existence of asteroids and comets. d) Number of planets of each type (4 terrestrial and 4 jovian). ...
The Kuiper Belt - UCLA - Earth, Planetary, and Space Sciences
... August 30, 1992, we were taking the third of a four-exposure sequence while blinking the first two images on a computer. We noticed that the position of one faint “star” appeared to move slightly between the successive frames. We both fell silent. The motion was quite subtle, but it seemed definite. ...
... August 30, 1992, we were taking the third of a four-exposure sequence while blinking the first two images on a computer. We noticed that the position of one faint “star” appeared to move slightly between the successive frames. We both fell silent. The motion was quite subtle, but it seemed definite. ...
Animated Planets PowerPoint Presentation
... Because you asked…….. The next visible comet is Comet Faye. Comet Faye's last perihelion was on November 15, 2006. It reached an apparent magnitude of 9.5 during that orbit. The orbital period of Comet Faye is 7.55 years Its next perihelion will occur on May 29, 2014. During this next appearance, i ...
... Because you asked…….. The next visible comet is Comet Faye. Comet Faye's last perihelion was on November 15, 2006. It reached an apparent magnitude of 9.5 during that orbit. The orbital period of Comet Faye is 7.55 years Its next perihelion will occur on May 29, 2014. During this next appearance, i ...
Comets vs. Asteroids
... or less to make one orbit around the Sun. These are called short-period comets. Comets also come from their other hangout, the Oort Cloud. The Oort Cloud is a far-fardistance cloud of possibly a trillion comets that surrounds the Solar System. One trip around the Sun could take one of these comets 3 ...
... or less to make one orbit around the Sun. These are called short-period comets. Comets also come from their other hangout, the Oort Cloud. The Oort Cloud is a far-fardistance cloud of possibly a trillion comets that surrounds the Solar System. One trip around the Sun could take one of these comets 3 ...
Introduction to Basic Stargazing Part II - Naples Free-Net
... It is a peculiarity of comets that no matter where the comet is headed, the tail always points away from the Sun. Comets can also have two tails, one is of mostly dust, the other gas. Meteors: Remember all that dust and dirt the comets give off? It does not disappear, but continues to orbit the Sun ...
... It is a peculiarity of comets that no matter where the comet is headed, the tail always points away from the Sun. Comets can also have two tails, one is of mostly dust, the other gas. Meteors: Remember all that dust and dirt the comets give off? It does not disappear, but continues to orbit the Sun ...
Chapter 2 - The Solar System
... Most comets have highly eccentric orbits which take them far beyond the orbit of Pluto; these are seen once and then disappear for millennia. Only the short- and intermediate-period comets (like Comet Halley), stay within the orbit of Pluto for a significant fraction of their orbits. ...
... Most comets have highly eccentric orbits which take them far beyond the orbit of Pluto; these are seen once and then disappear for millennia. Only the short- and intermediate-period comets (like Comet Halley), stay within the orbit of Pluto for a significant fraction of their orbits. ...
Oort cloud
The Oort cloud (/ˈɔrt/ or /ˈʊərt/) or Öpik–Oort cloud, named after Dutch astronomer Jan Oort and Estonian astronomer Ernst Öpik, is a theoretical spherical cloud of predominantly icy planetesimals believed to surround the Sun at a distance of up to around 100,000 AU (2 ly). This places it at almost half of the distance to Proxima Centauri, the nearest star to the Sun, and in interstellar space. The Kuiper belt and the scattered disc, the other two reservoirs of trans-Neptunian objects, are less than one thousandth as far from the Sun as the Oort cloud. The outer limit of the Oort cloud defines the cosmographical boundary of the Solar System and the region of the Sun's gravitational dominance.The Oort cloud is thought to comprise two regions: a spherical outer Oort cloud and a disc-shaped inner Oort cloud, or Hills cloud. Objects in the Oort cloud are largely composed of ices, such as water, ammonia, and methane.Astronomers conjecture that the matter composing the Oort cloud formed closer to the Sun and was scattered far into space by the gravitational effects of the giant planets early in the Solar System's evolution. Although no confirmed direct observations of the Oort cloud have been made, it may be the source of all long-period and Halley-type comets entering the inner Solar System, and many of the centaurs and Jupiter-family comets as well. The outer Oort cloud is only loosely bound to the Solar System, and thus is easily affected by the gravitational pull both of passing stars and of the Milky Way itself. These forces occasionally dislodge comets from their orbits within the cloud and send them towards the inner Solar System. Based on their orbits, most of the short-period comets may come from the scattered disc, but some may still have originated from the Oort cloud.