![evidence for a distant giant planet in the solar system](http://s1.studyres.com/store/data/006706333_1-3c0b888e62fa9dfa86d7ff9a543599e0-300x300.png)
evidence for a distant giant planet in the solar system
... We estimate the statistical significance of the observed clustering by assuming that the detection biases for our clustered objects are similar to the detection biases for the collection of all objects with q>30 AU and a>50 AU. We then randomly select six objects from the sample 100,000 times and ...
... We estimate the statistical significance of the observed clustering by assuming that the detection biases for our clustered objects are similar to the detection biases for the collection of all objects with q>30 AU and a>50 AU. We then randomly select six objects from the sample 100,000 times and ...
Solar Nebula
... – i the inclinaEon, which establishes the Elt of the orbital plane, relaEve to the eclipEc plane – Ω the longitude of the ascending node (ascending crossover point of the orbit, measured with respect ...
... – i the inclinaEon, which establishes the Elt of the orbital plane, relaEve to the eclipEc plane – Ω the longitude of the ascending node (ascending crossover point of the orbit, measured with respect ...
100 Apple Solar System
... What is the biggest body in our solar system? . Sun What is the largest planet? Second largest? . Jupiter . Saturn What are the next two, which are relatively close in size? . Uranus . Neptune How do the objects in our solar system compare with each other? ...
... What is the biggest body in our solar system? . Sun What is the largest planet? Second largest? . Jupiter . Saturn What are the next two, which are relatively close in size? . Uranus . Neptune How do the objects in our solar system compare with each other? ...
Lesson 1 Key Questions for PPT
... Its mission is to promote and safeguard the science of astronomy in all its aspects through international cooperation. ...
... Its mission is to promote and safeguard the science of astronomy in all its aspects through international cooperation. ...
Our Solar System - World Book Online
... 11. _________ Comets are made up mainly of fire. 12. _________ Comets in our solar system come from the Oort cloud or the Kuiper belt. 13. _________ The asteroid belt is located between the orbits of Jupiter and Saturn. 14. _________ The smallest asteroid in the asteroid belt is called Ceres. © ...
... 11. _________ Comets are made up mainly of fire. 12. _________ Comets in our solar system come from the Oort cloud or the Kuiper belt. 13. _________ The asteroid belt is located between the orbits of Jupiter and Saturn. 14. _________ The smallest asteroid in the asteroid belt is called Ceres. © ...
Orbits…the celestial paths of planets
... figures….agrees with observed fact that orbits lie in a plane ...
... figures….agrees with observed fact that orbits lie in a plane ...
Magnetic fields
... of moons, most of which are airless and composed of ice/rock mix. One interesting moon, though, is Uranus’ moon Miranda. While small, this moon is interesting. The moon is covered with a mass of ...
... of moons, most of which are airless and composed of ice/rock mix. One interesting moon, though, is Uranus’ moon Miranda. While small, this moon is interesting. The moon is covered with a mass of ...
Small Solar System Bodies
... to as a large orbital inclination). They also typically have orbits that are far from being perfectly circular (technically referred to as having a large orbital eccentricity). All of these distinguishing characteristics are scientifically interesting in that they suggest a different origin from the ...
... to as a large orbital inclination). They also typically have orbits that are far from being perfectly circular (technically referred to as having a large orbital eccentricity). All of these distinguishing characteristics are scientifically interesting in that they suggest a different origin from the ...
The Outer Planets - Mr. Cramer
... • Pluto is so far away from the sun that it revolves around the sun only once every 248 Earth years • Orbit is elliptical and comes closer to the sun than Neptune on part of its orbit • Many icy objects larger and farther out than Pluto have astronomers creating a new class of objects called “dwarf ...
... • Pluto is so far away from the sun that it revolves around the sun only once every 248 Earth years • Orbit is elliptical and comes closer to the sun than Neptune on part of its orbit • Many icy objects larger and farther out than Pluto have astronomers creating a new class of objects called “dwarf ...
Document
... Consequently, it exerts a tremendous gravitational pull on planets, dwarf planets, satellites, asteroids, comets, and meteoroids. How the solar system was formed. Astronomers believe the solar system formed about 4.7 billion years ago. However, they differ in their beliefs about how it formed. Most ...
... Consequently, it exerts a tremendous gravitational pull on planets, dwarf planets, satellites, asteroids, comets, and meteoroids. How the solar system was formed. Astronomers believe the solar system formed about 4.7 billion years ago. However, they differ in their beliefs about how it formed. Most ...
Pluto and Comets
... Neptune, why doesn’t it ever collide with Neptune? A. They do collide every few thousand years. B. Neptune is primarily made of gases, so Pluto would pass right through it. C. Pluto’s orbit is steeply tilted with respect to Neptune’s, so they never actually cross. D. The synchronized timing of their ...
... Neptune, why doesn’t it ever collide with Neptune? A. They do collide every few thousand years. B. Neptune is primarily made of gases, so Pluto would pass right through it. C. Pluto’s orbit is steeply tilted with respect to Neptune’s, so they never actually cross. D. The synchronized timing of their ...
Ch. 17: The Solar System
... Upper atmosphere is methane Has Great Dark Spot similar to Jupiter’s Great Red Spot Winds blow east to west @1500 km/h ...
... Upper atmosphere is methane Has Great Dark Spot similar to Jupiter’s Great Red Spot Winds blow east to west @1500 km/h ...
ASTR100 Class 01
... Which explanation for the asteroid belt seems the most plausible? A. The belt is where all the asteroids happened to form. B. The belt is the remnant of a large terrestrial planet that used to be between Mars and Jupiter. C. The belt is where all the asteroids happened to survive. But WHY didn’t the ...
... Which explanation for the asteroid belt seems the most plausible? A. The belt is where all the asteroids happened to form. B. The belt is the remnant of a large terrestrial planet that used to be between Mars and Jupiter. C. The belt is where all the asteroids happened to survive. But WHY didn’t the ...
The scattered disk population as a source of Oort cloud comets
... ∼ 6 × 108 SDOs could supply all the observed JF comets, though this result might be model-dependent and actually represent a lower limit. This is because they start with a sample of test particles already in Neptune-encountering orbits, while a large fraction of the SDOs have perihelia well above Ne ...
... ∼ 6 × 108 SDOs could supply all the observed JF comets, though this result might be model-dependent and actually represent a lower limit. This is because they start with a sample of test particles already in Neptune-encountering orbits, while a large fraction of the SDOs have perihelia well above Ne ...
Lesson 2
... Today, we know that the orbits of the planets are only slightly elliptical, but the orbits of objects such as Pluto and comets are highly elliptical. Kepler found that a planet moves slower at aphelion, sweeping out a narrow sector on the ellipse. Conversely, a planet moves faster at perihelion, swe ...
... Today, we know that the orbits of the planets are only slightly elliptical, but the orbits of objects such as Pluto and comets are highly elliptical. Kepler found that a planet moves slower at aphelion, sweeping out a narrow sector on the ellipse. Conversely, a planet moves faster at perihelion, swe ...
exploring the kuiper belt with the magellan telescopes
... carried out by Kern (2005b). In another KBO program, we are measuring object colors as a function of orbital-pole alignment, with respect to the pole of the mean orbital plane of the Kuiper belt as determined by the DES (Elliot et al. 2005). Using photometric data from MagIC, Gulbis, Elliot & Kane ( ...
... carried out by Kern (2005b). In another KBO program, we are measuring object colors as a function of orbital-pole alignment, with respect to the pole of the mean orbital plane of the Kuiper belt as determined by the DES (Elliot et al. 2005). Using photometric data from MagIC, Gulbis, Elliot & Kane ( ...
What Is a Planet? Pluto and Its Place in the Solar System
... other objects (KBOs) are similar to Pluto • Since 2005, we have learned that Pluto isn’t even the biggest KBO (Eris) • Pluto is one of the biggest and most interesting KBOs • Continue to study it, learn about how the solar system works ...
... other objects (KBOs) are similar to Pluto • Since 2005, we have learned that Pluto isn’t even the biggest KBO (Eris) • Pluto is one of the biggest and most interesting KBOs • Continue to study it, learn about how the solar system works ...
Guided Notes - Duplin County Schools
... Some asteroids have very eccentric orbits and travel very near the sun, and a few larger ones regularly pass close to Earth and the moon Many of the most recent impact craters on the moon and Earth were probably caused by _____________________________ with asteroids Inevitably, future Earth-asteroid ...
... Some asteroids have very eccentric orbits and travel very near the sun, and a few larger ones regularly pass close to Earth and the moon Many of the most recent impact craters on the moon and Earth were probably caused by _____________________________ with asteroids Inevitably, future Earth-asteroid ...
What are the Jovian Planets? Characteristics of Jovian Planets
... Orbital periods obey Kepler’s 3rd Law: P2=a3 ...
... Orbital periods obey Kepler’s 3rd Law: P2=a3 ...
Chapter 15 The Formation of Planetary Systems
... • Orbits mostly between Mars and Jupiter • Jupiter’s gravity kept them from condensing into a planet, or accreting onto an existing one • Fragments left over from the initial formation of the solar system ...
... • Orbits mostly between Mars and Jupiter • Jupiter’s gravity kept them from condensing into a planet, or accreting onto an existing one • Fragments left over from the initial formation of the solar system ...
Final exam
... 1910 : doctors sold "comet pills" to ward off ill effects of Earth passing through tail of Comet Halley Actually tails very diffuse but small particles are kicked off surface of comet and left ...
... 1910 : doctors sold "comet pills" to ward off ill effects of Earth passing through tail of Comet Halley Actually tails very diffuse but small particles are kicked off surface of comet and left ...
File
... Explanation: How many planets are in the Solar System? This popular question now has a new formal answer according the International Astronomical Union (IAU): eight. Last week, the IAU voted on a new definition for planet and Pluto did not make the cut. Rather, Pluto was re-classified as a dwarf pl ...
... Explanation: How many planets are in the Solar System? This popular question now has a new formal answer according the International Astronomical Union (IAU): eight. Last week, the IAU voted on a new definition for planet and Pluto did not make the cut. Rather, Pluto was re-classified as a dwarf pl ...
Chapter 24 Vocabulary link - Flushing Community Schools
... the orbit of Neptune, 30-50 AU from the Sun. It is like the asteroid belt, but it is about 200 times as massive. Like the asteroid belt, it consists of remnants from the Solar System's formation. ...
... the orbit of Neptune, 30-50 AU from the Sun. It is like the asteroid belt, but it is about 200 times as massive. Like the asteroid belt, it consists of remnants from the Solar System's formation. ...
Jovian Planet Systems (Chapter 11) Jupiter and Saturn are mostly
... Jupiter and Saturn are mostly hydrogen, with layers of gas, liquid, and metallic hydrogen above a small rock/ice (water, methane, ammonia) core. Uranus and Neptune have a thinner outer layer of hydrogen gas, a thick ice mantle, and a core. All four planets contain about 10 Earth masses of ice, rock, ...
... Jupiter and Saturn are mostly hydrogen, with layers of gas, liquid, and metallic hydrogen above a small rock/ice (water, methane, ammonia) core. Uranus and Neptune have a thinner outer layer of hydrogen gas, a thick ice mantle, and a core. All four planets contain about 10 Earth masses of ice, rock, ...
Scattered disc
![](https://commons.wikimedia.org/wiki/Special:FilePath/Eris_and_dysnomia2.jpg?width=300)
The scattered disc (or scattered disk) is a distant region of the Solar System that is sparsely populated by icy minor planets, a subset of the broader family of trans-Neptunian objects. The scattered-disc objects (SDOs) have orbital eccentricities ranging as high as 0.8, inclinations as high as 40°, and perihelia greater than 30 astronomical units (4.5×109 km; 2.8×109 mi). These extreme orbits are thought to be the result of gravitational ""scattering"" by the gas giants, and the objects continue to be subject to perturbation by the planet Neptune.Although the closest scattered-disc objects approach the Sun at about 30–35 AU, their orbits can extend well beyond 100 AU. This makes scattered objects among the most distant and coldest objects in the Solar System. The innermost portion of the scattered disc overlaps with a torus-shaped region of orbiting objects traditionally called the Kuiper belt, but its outer limits reach much farther away from the Sun and farther above and below the ecliptic than the Kuiper belt proper.Because of its unstable nature, astronomers now consider the scattered disc to be the place of origin for most periodic comets in the Solar System, with the centaurs, a population of icy bodies between Jupiter and Neptune, being the intermediate stage in an object's migration from the disc to the inner Solar System. Eventually, perturbations from the giant planets send such objects towards the Sun, transforming them into periodic comets. Many Oort cloud objects are also thought to have originated in the scattered disc. Detached objects are not sharply distinct from scattered disc objects, and some such as Sedna have sometimes been considered to be included in this group.