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For Chapter 16 on November 26, 2012
For Chapter 16 on November 26, 2012

... • (2) It must have sufficient mass for self-gravity to form a nearly round shape. • (3) It must be the dominant body within its orbit. The last statement disqualifies Pluto The IAU established two new categories for objects that orbit the Sun. Dwarf planets is one of the categories Pluto, Ceres, Eri ...
Objects In Space -- research questions
Objects In Space -- research questions

... 5. Can we see them from Earth? If so, what do they look like? ...
Powerpoint file
Powerpoint file

... explosion 2. Second Generation Planets: Planets that formed in the debris disk left behind after the supernova explosion (more likely) Debris disk found around another pulsar fits this picture! ...
The planets in the solar system
The planets in the solar system

... are formed during the collapse of a nebula into a thin disk of gas and dust. A proto-star (proto = early) forms at the core, surrounded by a rotating proto-planetary disk. Through a process called accretion (i.e., sticky collision) dust particles in the disk steadily accumulate mass to form ever-lar ...
Studying Planets in the Solar System
Studying Planets in the Solar System

... 7. After their research is complete, have the groups create a presentation to share their planetary information with the class. Presentations may be in the form of a written report with illustrations, a three-dimensional model, or a bulletin board display. ...
Extra-Solar Planets
Extra-Solar Planets

... stars with more than one planet - true planetary systems ...
File - Mrs. Ratzlaff
File - Mrs. Ratzlaff

... The largest, Ceres, is nearly _________ across, it is called a dwarf planet. Scientist believe the rocks are left over from a __________ that never formed. Asteroids ___________ as the ___________ around the Sun, just like the planets. Some asteroids even have _________! We have even landed a space ...
Searching for planets around evolved stars with COROT
Searching for planets around evolved stars with COROT

... of Padova Observatory (ref d), we can determine the corresponding evolution stage (Teff and L/L) of stars having the limit radius above for a given mass (fig 2). The results, for a solar abundance, are present in table 2 and the position of the stars in the Padova's evolution tracks are shown in Fi ...
Bringing Our Solar System to Life Grade 5 Overview Since the Solar
Bringing Our Solar System to Life Grade 5 Overview Since the Solar

... The classroom contains roughly 20 fifth graders. The genders in the classroom are about even. These students have had one prior lesson on the solar system and its planets which was presented in a lecture form, with pictures, by the teacher. The setting of the school is rural. 5.2.1 Recognize that ou ...
HotJup
HotJup

... The central star is a G0V solar-type dwarf star ...
Large and small planets Journey through the Solar System
Large and small planets Journey through the Solar System

... Using the table below, write the information from the second column (the diameter) next to the planets on the board. Explain clearly to the children that the Sun is very large, and that it is not a planet at all, but a star. It is interesting to see how large the sun is compared to the planets. Use ...
Planetary system
Planetary system

... been the most successful with a few exoplanets being detected every week this way. Mostly find large Jupiter like planets. The orbits of large planets cause a star to wobble, causing a Doppler effect shifting from red to blue wavelengths. ...
`earthlike` and second the probability that they have suitable climate
`earthlike` and second the probability that they have suitable climate

... which are ‘earthlike’ and second the probability that they have suitable climate. ...
Planets Beyond the Solar System
Planets Beyond the Solar System

... (International Astronomical Union) a brown dwarf has a mass above that needed for fusion of deuterium (approximately 13 Jupiter masses). An object lower than that mass and orbiting a star (or star remnant) is said to be a planet. ...
Chapter 2: Perihelion of Mercury`s Orbit
Chapter 2: Perihelion of Mercury`s Orbit

... A third prediction from Einstein’s theory of general relativity is the excess precession of the perihelion of the orbit of Mercury of about 0.01° per century. This effect had been known and unexplained for some time, so in some sense its correct explanation represented an immediate success of the th ...
Planets Beyond the Solar System
Planets Beyond the Solar System

... (International Astronomical Union) a brown dwarf has a mass above that needed for fusion of deuterium (approximately 13 Jupiter masses). An object lower than that mass and orbiting a star (or star remnant) is said to be a planet. ...
The new europian project ROPACS (Rocky Planets Around …
The new europian project ROPACS (Rocky Planets Around …

... Feedback to the network. assessments. ...
Document
Document

... The time taken for the planet to complete one full orbit relative to the distant fixed stars (i.e. its ‘true’ orbital period) is called its sidereal period. However, during this time, the Earth has also been moving in its orbit: after one planetary sidereal period, the planet still appears to be in ...
The Solar System Solar System Today (Not to Scale) Inner Planets
The Solar System Solar System Today (Not to Scale) Inner Planets

... Comparisons among the nine planets show distinct similarities and significant differences ...
Extra-Solar Planets
Extra-Solar Planets

... radial velocity monitoring in 1995. The data imply the presence of a planet with - a roughly circular orbit - a distance of 0.052 A.U. - a mass of 0.46 MJup It’s like a very hot Jupiter! ...
Extrasolar Planets = 403
Extrasolar Planets = 403

... Common orbital and rotation direction & plane => nebular disk Jovian / Terrestrial => range of temperatures in disk Common ages => simultaneous formation in disk Problems: Speed of Jupiter’s formation, angular momentum, clearing disk, discrepancies, moon! ...
October 3
October 3

... Which planet will have the most extreme seasons? ...
That star is an M-dwarf, smaller, dimmer and cooler than our sun. So
That star is an M-dwarf, smaller, dimmer and cooler than our sun. So

... (12) Many scientists have thought that life couldn’t develop near M-dwarf stars. This is because they give off more damaging radiation than G-type stars like our sun. Kepler-186f, however, appears to sit far away enough from its star to be out of harm’s way. “That’s Very Exciting” (13) The discovery ...
Answers - Partake AR
Answers - Partake AR

... and 6 minutes. (Answer: Day) Asteroids don’t have an atmosphere and there are ____________ leftover from the formation of the solar system. (Answer: Millions) ...
Space - FIVES R US
Space - FIVES R US

... Neptune is the stormiest planet. The winds there can blow up to 1,240 miles per hour, that is three times as fast as Earth's Hurricanes. Neptune is a sea blue color due to the methane gas in its atmosphere. It once had a great dark spot similar to Jupiter. Neptune only receives 1/900 of the solar e ...
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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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