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The role of Jupiter in driving Earth`s orbital evolution
The role of Jupiter in driving Earth`s orbital evolution

... orbiting nearby stars, and the search for life beyond our Solar system will be able to begin in earnest. However, the observations required to detect evidence of life on Earth-like planets orbiting other stars will be hugely time-consuming and costly – which will in turn mean that we will only be ab ...
Don`t Panic, But the Sun Will (Far) Outlive Earth (Op-Ed)
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... This 10% increase in the sun’s brightness, triggering the evaporation of our oceans, will occur over the next billion years or so. Predictions of exactly how rapidly this process will unfold depend on who you talk to. Most models suggest that as the oceans evaporate, more and more water will be pres ...
The Origin of the Solar System: Progress in Understanding Accretion
The Origin of the Solar System: Progress in Understanding Accretion

... As yet, these new discoveries have not been incorporated into formation models. Where once we thought that Jupiter-like planets would naturally form at the distance from a star where water would condense, and represent a natural bulge in the mass available in the disk, we now have many counter-exam ...
Venus Investigation
Venus Investigation

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... Small Solar System Bodies (SSSB) are objects in the solar system that are neither planets or dwarf planets. Of these, asteroids, comets and meteors are sometimes grouped together because of their similarities, but they are distinct objects. Asteroids are irregularly shaped pieces of rock moving thro ...
SIM-Lite Space Astrometric Observatory
SIM-Lite Space Astrometric Observatory

... • Given “Perfect” instruments, the ultimate limitation to both RV and Astrometric detection of exoplanets is astrophysical noise from the target star. - Star spots on the Sun produce 10~12X higher bias to RV than Astrometry (for planets in a ~1 yr orbit). ...
The Moon - Kaufman ISD
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Asteroids, Comets, and Pluto: The Small Pieces
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Lecture11 - UCSB Physics
Lecture11 - UCSB Physics

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Introduction to Astronomy
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ExamIIRevFa06
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Lecture11 - UCSB Physics
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The Planets
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... The largest was over 40 feet long and had a mirror 48 inches across. It was held up with a framework of wood, and they had to have helpers move it around using ropes and pulleys. It was the largest telescope in the world until over 100 years later. Which planet was formed first and how was it formed ...
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...  Calculate the maximum altitude of the Sun at any location and time of year using te 2-D Local Horizon Map.  Predict where the Sun will be on the Whole Sky Map some number of months after its current position on the ecliptic. Unit 7: The Day  Describe the location of sunrise and sunset along the ...
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... searches are underway to scan the far reaches of space in an organized fashion for evidence of other life. In particular, searches for extraterrestrial intelligence (ETI) and extrasolar planets are each conducted using telescopes that scan locations light years away and outside the solar system. Bot ...
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... allowed extremely accurate predictions of planetary orbits.  Cavendish measured gravitational forces between human-scale objects before 1800. ...
Solar System Debris - Sierra College Astronomy Home Page
Solar System Debris - Sierra College Astronomy Home Page

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... Stéphane Udry1, Jean-Loup Bertaux9 & Jean-Pierre Sivan10 Over the past two years, the search for low-mass extrasolar planets has led to the detection of seven so-called ‘hot Neptunes’ or ‘super-Earths’ around Sun-like stars. These planets have masses 5–20 times larger than the Earth and are mainly ...
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Planets beyond Neptune



Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit. The search began in the mid-19th century and culminated at the start of the 20th with Percival Lowell's quest for Planet X. Lowell proposed the Planet X hypothesis to explain apparent discrepancies in the orbits of the giant planets, particularly Uranus and Neptune, speculating that the gravity of a large unseen ninth planet could have perturbed Uranus enough to account for the irregularities.Clyde Tombaugh's discovery of Pluto in 1930 appeared to validate Lowell's hypothesis, and Pluto was officially named the ninth planet. In 1978, Pluto was conclusively determined to be too small for its gravity to affect the giant planets, resulting in a brief search for a tenth planet. The search was largely abandoned in the early 1990s, when a study of measurements made by the Voyager 2 spacecraft found that the irregularities observed in Uranus's orbit were due to a slight overestimation of Neptune's mass. After 1992, the discovery of numerous small icy objects with similar or even wider orbits than Pluto led to a debate over whether Pluto should remain a planet, or whether it and its neighbours should, like the asteroids, be given their own separate classification. Although a number of the larger members of this group were initially described as planets, in 2006 the International Astronomical Union reclassified Pluto and its largest neighbours as dwarf planets, leaving Neptune the farthest known planet in the Solar System.Today, the astronomical community widely agrees that Planet X, as originally envisioned, does not exist, but the concept of Planet X has been revived by a number of astronomers to explain other anomalies observed in the outer Solar System. In popular culture, and even among some astronomers, Planet X has become a stand-in term for any undiscovered planet in the outer Solar System, regardless of its relationship to Lowell's hypothesis. Other trans-Neptunian planets have also been suggested, based on different evidence. As of March 2014, observations with the WISE telescope have ruled out the possibility of a Saturn-sized object out to 10,000 AU, and a Jupiter-sized or larger object out to 26,000 AU.
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