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Chapter 28 Notes
Chapter 28 Notes

... Formation of the Solar System • Nebular Theory: a) Interstellar cloud contracts and spins b) Dense center begins nuclear fusion (sun) c) Remaining material forms planetesimals and then planets ...
Formation of the solar system
Formation of the solar system

... Ceres (760 km diameter). These are thought to be the source of metoerites 4) The outer planets - Jupiter, Saturn, Uranus, Neptune, Pluto are much further from the sun and much less ...
Gravity in the Solar System Quiz
Gravity in the Solar System Quiz

... 9) If you are on the top of a mountain and drop an apple, it will fall to the ground, even though the apple is gravitationally attracted to you. Why? a) Earth is larger and has a much stronger gravitational pull. b) Apples always fall down. c) Centrifugal forces pull the apple to the Earth and that ...
Planets
Planets

... Mercury - Mercury is the planet closest to the Sun. Venus - Venus is the second planet from the Sun. It is the hottest planet. Earth - Earth is the third planet from the Sun and the planet we live on. Mars - Mars is a red planet and the fourth planet from the Sun. Jupiter - Jupiter is the fifth plan ...
Earth has formed in our solar system
Earth has formed in our solar system

... • Competing forces induce flattening ...
Planets
Planets

... Why would this ...
Chapter27
Chapter27

... Earth with the treatment of life elsewhere. This material was part of the chapter on Earth. My reason for having such a limited discussion of life in the Universe was that I thought the subject was still very speculative. For example, at that time, only a little more than 10 years ago, we didn’t yet ...
Jovian Planets and Interiors
Jovian Planets and Interiors

... So why is Venus so different from Earth given the similar size and distance from the Sun? The answer lies in the minor difference in distance to the Sun. When a planet warms more water evaporates. Since water is a greenhouse gas, having more in the atmosphere warms the planet further. This positive ...
AST101 Lecture 16 Extra Solar Planets
AST101 Lecture 16 Extra Solar Planets

... Doppler Wobble: Gliese 876 ...
Something Big Out There - binaryresearchinstitute.com
Something Big Out There - binaryresearchinstitute.com

... Two Spanish astronomers, Carlos and Raul de la Fuente Marcos, at the Complutense University of Madrid in Spain, have examined these distant dwarfs and noticed some unusual patterns. They have concluded that because Biden and Sedna are not large enough to exert much influence on each other, they must ...
without video - Scott Marley
without video - Scott Marley

... and Dale Frail announced the discovery of two planets orbiting the pulsar PSR 1257+12. This discovery is generally considered to be the first definitive detection of exoplanets. These pulsar planets are believed to have formed from the unusual remnants of the supernova that produced the pulsar, in a ...
AST101 Lecture 16 Extra Solar Planets
AST101 Lecture 16 Extra Solar Planets

... Doppler Wobble: Gliese 876 ...
Gravity in the Solar System Quiz - cK-12
Gravity in the Solar System Quiz - cK-12

... 9) If you are on the top of a mountain and drop an apple, it will fall to the ground, even though the apple is gravitationally attracted to you. Why? a) Earth is larger and has a much stronger gravitational pull. b) Apples always fall down. c) Centrifugal forces pull the apple to the Earth and that ...
Planets & Motions
Planets & Motions

... Jovian planets (a.k.a. Outer/Gaseous planets) – Huge – gas giants = thick atmosphere, – much less dense (Saturn floats!), – rings, – beyond asteroid belt – Jupiter, Saturn, Uranus, Neptune ...
02-Voyage to the Planets
02-Voyage to the Planets

... The force of gravity caused these clumps to form the Jovian planets (Jupiter, Saturn, Uranus and Neptune) ...
24exoplanets8s
24exoplanets8s

... planets in the habitable zone Many systems have detected multiple planets ...
Class Notes for Monday, Feb 20th
Class Notes for Monday, Feb 20th

... – Our star (Sun) and everything that orbits around it (planets, asteroids, comets, etc.) • Galaxy – Huge collection of stars bound together by gravity (the Sun is 1 star among 100400 billion stars in the Milky Way galaxy) • Universe – Everything (~100 billion galaxies) ...
Quiz 5
Quiz 5

... 23. (1  pt.)  The  planet  with  the  largest  volcano  in  the  solar  system  is   a. Earth.   b. Mars.   c. Venus.   d. Mercury.   ...
Overview of the Solar System AST 105
Overview of the Solar System AST 105

... • Is neither a star nor a satellite of a planet Consequences: • Pluto/Charon is a (double) planet • So are Ceres, Sedna, and Eris • And an estimated 40+ Kuiper belt objects! ...
Farthest Known Planet Opens the Door for Finding New Earths
Farthest Known Planet Opens the Door for Finding New Earths

... • Radial Velocity Measurements (119) looking for the Doppler shifts due to “Stellar Wobble” as planet pulls on star, • Transit Measurements (3) looking for periodic dimming as planet eclipses ...
21. Solar System Formation
21. Solar System Formation

... 1. Within the frost line, bits of rock and metal clumped together to make planetesimals. 2. As the planetesimals grew, they became large enough to attract each other. 3. Finally, only a few planets were left. ...
Are we Alone? The Search for Life Beyond the
Are we Alone? The Search for Life Beyond the

... Are we Alone? - The Search for Life beyond the Earth. ...
answers_exam_review_space
answers_exam_review_space

... as hydrogen and helium Orbit – the path an object takes as it moves around another object i.e. planets orbit around the sun Fill in the blanks for each of the following questions: 1. universe 20. winter 2. astronomy 21. towards 3. constellations 22. away from 4. Orion 23. Sun 5. Solar system 24. sat ...
Lecture - Faculty
Lecture - Faculty

... Gas collects into “disk”, and cools leading to formation of condensates Growth of planetesimals by collisions a) Build up minor bodies and small rocky worlds b) Build up Jovian cores that sweep up outer gases ...
Unit 3: The Solar System Historical Models of the Solar System
Unit 3: The Solar System Historical Models of the Solar System

... - He was ridiculed and his model was not accepted ...
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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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