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Contents Mercury, page 2 Venus, page 3 Earth
Contents Mercury, page 2 Venus, page 3 Earth

... Mercury is one of four terrestrial planets in the Solar System, and is a rocky body like the Earth. It is the smallest planet in the Solar System, with an equatorial radius of 2,439.7 km. Mercury is even smaller—albeit more massive—than the largest natural satellites in the Solar System, Ganymede an ...
The Origin of the Solar System and Other Planetary Systems
The Origin of the Solar System and Other Planetary Systems

... Orbits of 60 of the known extrasolar planets; note that some of them are very close to their star. ...
Skinner Chapter 2
Skinner Chapter 2

... presence or absence of a biosphere. Discuss, using the terrestrial planets for comparative purposes. 52. Our Sun is currently in a phase of its stellar evolution in which it is producing helium from hydrogen present in its core. All other, heavier elements can form only in the cores of stars more m ...
Jun - Wadhurst Astronomical Society
Jun - Wadhurst Astronomical Society

... Now you will all remember that the asteroid belt is situated between the orbits of Mars and Jupiter, and Ceres is the largest object in this location of our Solar System. Well, apparently they have just found water on it! Water jets have been spotted by the ESA space observatory, Hershel. This is go ...
Bringing E.T. into Your Classroom The Search for
Bringing E.T. into Your Classroom The Search for

... 4. Small diameter planets or large diameter planets. 5. Small mass planets or large mass planets. 6. Planets close to star or planets far from star. ...
Universe Now - Course Pages of Physics Department
Universe Now - Course Pages of Physics Department

... • The formation theory has to explain currently observed dynamical and physical properties of different objects in the Solar System: – Orbits of the planets are nearly circular and nearly in the equatorial plane of the Sun (but not exactly!). – The planets are orbiting in the same direction (also t ...
Three Media Reports by Carole Gallagher
Three Media Reports by Carole Gallagher

... 10,000 times dimmer than the faintest star in the sky visible to the unaided eye. Since 1930, no new planets have been discovered using telescopes. This is because other planets beyond our solar system are so far away in our galaxy that they are billions of times fainter than Pluto and cannot be see ...
Properties of the Planets & Formation of the Solar
Properties of the Planets & Formation of the Solar

... • The only surface liquid water in the solar system ...
Planets in the sky
Planets in the sky

... • Motion of planets very important in historical context of how we came to figure out the nature of the Solar System ...
2012年雅思阅读考试考前冲刺试题(1)
2012年雅思阅读考试考前冲刺试题(1)

... of the sky,measuring the brightness of about 10,000 stars every 512 seconds. 5."At the present moment we are hoping to find out more about the nature of planets around stars which are potential habitats.We are looking at habitable planets,not inhabited planets.We are not going to find any little gre ...
"Earth" among 7 distant planets
"Earth" among 7 distant planets

... The lead scientists in the study is Michaël Gillon. He is a scientist in Belgium. Gillon and his fellow scientists have been interested in TRAPPIST-1 since late 2015. They found out that there were small dips in the star's brightness at regular times. These dips were caused by planets crossing betwe ...
New Stars, New Planets?
New Stars, New Planets?

... solar system; the new planets under consideration are 500,000 times more distant than Pluto. Astronomers look for small, regular variations in the Doppler shifts of light emitted by stars. Such changes indicate a back and forth "wobbling" of the star's motion, perhaps due to gravity effects from an ...
Planets - uni
Planets - uni

... (b) has sufficient mass for its self­gravity to overcome rigid body forces, so that it assumes a hydrostatic  equilibrium (nearly round) shape (note 2), and (c) has cleared the neighborhood around its orbit. A "dwarf planet" is a celestial body that (a) is in orbit around the Sun, (b) has sufficient ...
Powerpoint
Powerpoint

... Inner parts of Solar Nebula hotter (due to forming Sun): mostly gas. Accretion of gas atoms onto dust grains relatively inefficient. Jovian planets: Outer parts cooler: ices form (but still much gas), also ice "mantles" on dust grains => much more solid material for accretion => larger planetesimals ...
Summary of the Presentation
Summary of the Presentation

... ATCs. Solar systems dynamics indicates that K7, and smaller, stars are unsuitable for this reason. The number of F7 to K6 main sequence stars per billion cubic light years obtained from the Gliese catalog was 385,000. After correcting for close binaries and (assuming a constant production rate) elim ...
PISGAH Dr. Bob Hayward ASTRONOMICAL Astronomer/Educator
PISGAH Dr. Bob Hayward ASTRONOMICAL Astronomer/Educator

... on it and particularly note it on Saturday evening when it is just to the north of the still nearly full moon. Mars follows Jupiter by rising a few minutes before 1 a.m. It is getting brighter as we approach it in our orbit around the sun and its red color will become more apparent. The beautiful ri ...
Name
Name

... D) Jupiter-sized planets are radioactive E) Jupiter-sized planets have hotter surface temperatures 17) The density of a material is 4,100 kg/m3. What is the density in g/cm3? A) B) C) D) E) ...
Solar System`s Age - Empyrean Quest Publishers
Solar System`s Age - Empyrean Quest Publishers

... Formation of Planets • Condensation temperature determines whether a certain substance is a solid or a gas. – Above the condensation temperature, gas state – Below the condensation temperature, solid sate • Hydrogen and Helium: always in gas state, because concentration temperatures close to absolu ...
power_point_slides
power_point_slides

... Theological question: Should we expect that God made life on other planets? “Scripture strongly implies that no intelligent life exists elsewhere…. Earth was created to be home for creatures made in God the Creator's image. It was on Earth that the first human couple rebelled against its creator an ...
Exoplanets - An ESO/OPTICON/IAU summer school on modern
Exoplanets - An ESO/OPTICON/IAU summer school on modern

... (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighbourhood around its orbit." IAU, Resolution B5 "Extrasolar planet is: an object that has a mass between that of Pluto and the deu ...
Impossible planets.
Impossible planets.

... light-years away, both in Virgo -- were equally strange in another way. While they orbited at a slightly more conventional distance from their respective stars, their orbits were highly eccentric -- not the nearly, circular orbits of Jupiter and Saturn but more elongated. One possible explanation wo ...
Lecture9_2014_v2 - UCO/Lick Observatory
Lecture9_2014_v2 - UCO/Lick Observatory

... tens to hundreds of Earth masses of nebular gas, before gas is lost from the disk. Slide credit: Jonathan Fortney ...
Planetary Taxonomy
Planetary Taxonomy

... definition applicable to exoplanets. exoplanets 2) Make the definition more rigorous by adopting an explicit criterion for dynamical dominance (such as a threshold on the directly observable scattering parameter Λ~M2/P). 3) Because all dynamical dominant bodies exceed the size threshold for roundnes ...
Twinkle, twinkle little star, how I wonder what you are. Up
Twinkle, twinkle little star, how I wonder what you are. Up

... #2 We’re as Different as Day and Night CHORUS We’re as different as day and night. We’re as different as black and white. But in this great big galaxy, I need you and you need me. Part 1 (first time only) I’m the sun, the center of the system. I’m number one, so everybody listen. I wait for all my ...
summary - guideposts
summary - guideposts

... All four of the Jovian worlds have ring systems and large families of moons. Jupiter’s Galilean satellites were discovered by Galileo. The terrestrial planets have no visible rings and few moons. Studies of craters on the moon show that the planets suffered a heavy bombardment of meteorite impact wh ...
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Planet



A planet (from Ancient Greek ἀστήρ πλανήτης (astēr planētēs), or πλάνης ἀστήρ (plánēs astēr), meaning ""wandering star"") is an astronomical object orbiting a star, brown dwarf, or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.The term planet is ancient, with ties to history, science, mythology, and religion. Several planets in the Solar System can be seen with the naked eye. These were regarded by many early cultures as divine, or as emissaries of deities. As scientific knowledge advanced, human perception of the planets changed, incorporating a number of disparate objects. In 2006, the International Astronomical Union (IAU) officially adopted a resolution defining planets within the Solar System. This definition is controversial because it excludes many objects of planetary mass based on where or what they orbit. Although eight of the planetary bodies discovered before 1950 remain ""planets"" under the modern definition, some celestial bodies, such as Ceres, Pallas, Juno, Vesta (each an object in the solar asteroid belt), and Pluto (the first trans-Neptunian object discovered), that were once considered planets by the scientific community are no longer viewed as such.The planets were thought by Ptolemy to orbit Earth in deferent and epicycle motions. Although the idea that the planets orbited the Sun had been suggested many times, it was not until the 17th century that this view was supported by evidence from the first telescopic astronomical observations, performed by Galileo Galilei. By careful analysis of the observation data, Johannes Kepler found the planets' orbits were not circular but elliptical. As observational tools improved, astronomers saw that, like Earth, the planets rotated around tilted axes, and some shared such features as ice caps and seasons. Since the dawn of the Space Age, close observation by space probes has found that Earth and the other planets share characteristics such as volcanism, hurricanes, tectonics, and even hydrology.Planets are generally divided into two main types: large low-density giant planets, and smaller rocky terrestrials. Under IAU definitions, there are eight planets in the Solar System. In order of increasing distance from the Sun, they are the four terrestrials, Mercury, Venus, Earth, and Mars, then the four giant planets, Jupiter, Saturn, Uranus, and Neptune. Six of the planets are orbited by one or more natural satellites.More than a thousand planets around other stars (""extrasolar planets"" or ""exoplanets"") have been discovered in the Milky Way: as of 1 October 2015, 1968 known extrasolar planets in 1248 planetary systems (including 490 multiple planetary systems), ranging in size from just above the size of the Moon to gas giants about twice as large as Jupiter. On December 20, 2011, the Kepler Space Telescope team reported the discovery of the first Earth-sized extrasolar planets, Kepler-20e and Kepler-20f, orbiting a Sun-like star, Kepler-20. A 2012 study, analyzing gravitational microlensing data, estimates an average of at least 1.6 bound planets for every star in the Milky Way.Around one in five Sun-like stars is thought to have an Earth-sized planet in its habitable zone.
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