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Interplanetary Vagabonds
Interplanetary Vagabonds

... Apollo Asteroids Some asteroids have very eccentric orbits so that they cross Earth’s orbit They are called Apollo asteroids and raise the concern of a possible collision with the Earth 4400 such asteroids have been discovered so far, of which about 800 have been designated as potentially hazardous ...
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Evidence for Design: Earth & Solar System
Evidence for Design: Earth & Solar System

... “Constancy of the tilt angle is a factor that provides long-term stability of the Earth’s temperature. If the polar tilt axis had undergone wide deviations from its present value, Earth’s climate would have been much less hospitable….. Rare Earth, p 224. These results show that the situation of the ...
Astronomy 111 Overview of the Solar system
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... show that any specific star will cross directly overhead (on the meridian) about four minutes earlier every day. In other words, the day according to the stars (the sidereal day) is about four minutes shorter than the day according to the sun (the solar day). If we measure a day from noon to noon - ...


... study the impact of a strong flare from the M dwarf, AD Leo, on the atmospheric chemistry of a hypothetical Earth-like planet located in the habitable zone. The simulations were performed using a 1-D photochemical model. We simulated six atmospheres with high concentrations of CO2 and CH4 . The resp ...
here.
here.

... B) Two times slower than the earth's orbital period C) Twice as fast as the earth's orbital period D) Four times slower than the earth's orbital period 5) If our year were twice as long (that is, if Earth took twice as many days to complete each orbit around the Sun), but Earth's rotation period and ...
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Small Bodies in the Outer Solar System
Small Bodies in the Outer Solar System

... How was the extended scattered disk and Sedna formed? Sedna’s current large perihelion distance (∼76 AU) along with its large eccentricity (∼0.84) are hard to explain with what we currently know about the Solar System. If Sedna formed in its current location it must have initially been on a circular ...
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Final Exam - Practice questions for Unit V

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... modern values of planet/earth orbit ratios. System worked very well. • Contrary to popular myths, Ptolemy's system was not overly cumbersome, and it accounted for subtleties like the uneven motion of the Sun • It is not Ptolemy's fault he did such a good job that it took 1500 years to improve on him ...
Student Text, pp. 139-144
Student Text, pp. 139-144

... of the universe. Astronomers studied the motion of Uranus over many years and discovered that its path was not quite as smooth as expected. Some distant hidden object appeared to be “tugging” on Uranus causing a slightly uneven orbit. Using detailed mathematical analysis, they predicted where this h ...
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Gingin Observatory July 2015 Newsletter
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... Is in the eastern dawn sky, is only visible early this month as it descends towards the Sun and superior conjunction (Earth and Mercury on opposite sides of the Sun) on the 24 th. Subsequently this speedy little planet moves into the evening dusk sky joining the brightest planets Venus and Jupiter i ...
AS 300 Chpt 3 Ls 3 The Outer Planets
AS 300 Chpt 3 Ls 3 The Outer Planets

... Callisto. They are about the same size as Earth’s Moon. Their orbits are nearly perfect circles. The smallest of the “big four” that Galileo discovered, Europa, is more massive than the largest of the non-Galilean moons by a factor of 7,000. The Galilean moons present some amazing features. Io is co ...
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... in the journal Science. “The massive planets could not have formed so close to their host stars so they must have migrated [or been scattered] into smaller orbits. When this happens, it is likely that they would destroy any terrestrial planets in the circumstellar habitable zone.” Consequently, Line ...
Giant Planets at Small Orbital Distances
Giant Planets at Small Orbital Distances

... As the search for planets and brown dwarfs around nearby stars accelerates, we should expect to be surprised. In no instance is this better illustrated than in the recent discovery by Mayor & Queloz (1995) of a planet orbiting a G2.5 star, 51 Pegasi, 14 parsecs away. With a 4.23{day period, a semi-m ...
The Development Of Astronomy
The Development Of Astronomy

... Platonic Solid Model – Kepler believed God must have had some geometric design for placing the six planets (Uranus and Neptune were yet to be discovered) at particular distances from the Sun. A sudden revelation led Kepler to consider that the reason there is only six planets was because there were ...
Script
Script

... is subtracted from its intensity before or after, only the signal caused by the planet remains. It is then possible to measure the planet's temperature and even to detect possible signs of cloud formations on it. This method has two major disadvantages. First of all, planetary transits are only obse ...
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IAU definition of planet



The definition of planet set in Prague in 2006 by the International Astronomical Union (IAU) states that, in the Solar System, a planet is a celestial body which: is in orbit around the Sun, has sufficient mass to assume hydrostatic equilibrium (a nearly round shape), and has ""cleared the neighborhood"" around its orbit.A non-satellite body fulfilling only the first two of these criteria is classified as a ""dwarf planet"". According to the IAU, ""planets and dwarf planets are two distinct classes of objects"". A non-satellite body fulfilling only the first criterion is termed a ""small Solar System body"" (SSSB). Initial drafts planned to include dwarf planets as a subcategory of planets, but because this could potentially have led to the addition of several dozens of planets into the Solar System, this draft was eventually dropped. The definition was a controversial one and has drawn both support and criticism from different astronomers, but has remained in use.According to this definition, there are eight planets in the Solar System. The definition distinguishes planets from smaller bodies and is not useful outside the Solar System, where smaller bodies cannot be found yet. Extrasolar planets, or exoplanets, are covered separately under a complementary 2003 draft guideline for the definition of planets, which distinguishes them from dwarf stars, which are larger.
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