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The Planets
The Planets

... •Jupiter core is slightly bigger than earth but weighs about 20 times more. •Jupiter is the biggest planet in our solar system. •Over 1300 Earths could fit inside Jupiter. ...
The Outer Planets - Duplin County Schools
The Outer Planets - Duplin County Schools

... into space by the Cassini orbiter, will descend to Titan’s surface for further studies In this section, we’ll take a clue from Cassini and explore the outer planets—Jupiter, Saturn, Neptune, Uranus, and Pluto ...
Slide 1
Slide 1

... -Jupiter, Saturn, Uranus, Neptune ________________________________________________ -larger and further from Sun ________________________________________________ -mostly liquid and gas (hydrogen and helium) ________________________________________________ - are less dense and have no solid surface __ ...
Properties of Earth (6.E.1.2)
Properties of Earth (6.E.1.2)

... Earth. The planet revolves around the star Gliese 581, one of the closest stars outside our solar system. Data collected over a number of years shows that Gliese 581 wobbled. This wobble indicates that a planet is orbiting the star. The orbit appears to last about 13 Earth days. The planet is in a r ...
The Solar System Solar System Today (Not to Scale) Inner Planets
The Solar System Solar System Today (Not to Scale) Inner Planets

... Planets, Sizes to Scale •  Top Row: Jupiter & Saturn •  Middle Row: Uranus & Neptune •  Bottom Row: Earth, Venus, Mars, Mercury, & the Moon ...
Objects in Space
Objects in Space

... – (2) has sufficient mass for its gravity to assume a nearly round shape – (3) has “cleared the neighborhood” around its orbit. • it has enough gravity that it does not share its orbit space with any other similarly sized body other than its own moons. (Pluto shares its orbit so it’s now a dwarf pla ...
Brock physics - Brock University
Brock physics - Brock University

... 6. Aristarchus argued that the Sun must be the centre of the solar system because (a) he reasoned that the Sun is much larger than the Earth, and so it made sense that the larger object should be at the centre. (b) careful observations showed that the Sun does not move, but the Earth does move. (c) ...
Mars
Mars

c. Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune 3. c
c. Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune 3. c

... a. Each other b. A star or sun ...
What is the universe???
What is the universe???

... in a row, 1 cm apart, on your balloon  Label one “Earth” and the others A-D (these represent other galaxies) • Partially inflate the balloon (1-2 big breaths) and hold it…do not tie it! Use a piece of yarn to measure the distances at time 1, convert to centimeters using your ruler, and record • Rep ...
Here - Al Ghaf
Here - Al Ghaf

... • Saturn is immensely heavy, but not very dense. If you could find an ocean of water large enough to put Saturn in, the planet would float! • Saturn’s spectacular rings are made up of thousands of millions of chunks of ice. And the wide rings are made up thousands of ringlets. • By the time the ...
d Transparent Deception In yet Another Alleged Extra
d Transparent Deception In yet Another Alleged Extra

... That Model is, in short, the greatest of all deceptions throughout human history that has ever been designed to confuse and lead mankind away from God’s Truth.... (I Cor.14:33) ...
History of Astronomy Notes
History of Astronomy Notes

... Explains apparent changes in brightness for some planets. Explains some of the observed non-uniform motions of the Sun, Moon, and Planets. Can fine-tune the model by adding epicycles. Failures of Ptolemy’s System: It was really, REALLY complicated. ...
Why is it so difficult to detect planets around other stars? Planet
Why is it so difficult to detect planets around other stars? Planet

... •  A young planet’s motion can create waves in a young star’s disk •  Models show that matter in these waves can tug on a planet, causing its orbit to migrate inward ...
Earth has formed in our solar system
Earth has formed in our solar system

... • Competing forces induce flattening ...
Extra-Solar Planets
Extra-Solar Planets

... 1) Old enough to allow time for evolution (rules out high-mass stars - 1%) 2) Need to have stable orbits (might rule out binary/multiple star systems - 50%) 3) Size of “habitable zone”: region in which a planet of the right size could have liquid water on its surface. Even so… billions of stars in t ...
Final Exam from 2008
Final Exam from 2008

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Day_14

... A. Planets move fastest when they are moving toward the Sun. B. Planets move equal distances throughout their orbit of the Sun. C. Planets move slowest when they are moving away from the Sun. D. Planets travel farther in a given time when they are closer to the Sun. E. Planets move the same speed at ...
Gravitation and Orbital Motion
Gravitation and Orbital Motion

Tycho Brahe & Johannes Kepler
Tycho Brahe & Johannes Kepler

The Solar System
The Solar System

... Sun at a distance of 30.1 AU, approximately 30 times the Earth-Sun distance. ...
7-15-08 Cropcircle 10th planet Nibiru
7-15-08 Cropcircle 10th planet Nibiru

... Image Peter Sorensen Copyright 2008 The new formation is obviously a diagrammatic representation of the Sun and planets (with no care for proper astronomical proportions). But the smaller inner ones (Mercury, Venus, Earth and Mars) are clearly delineated from the giant outer ones (Jupiter, Saturn ...
Word doc - UC-HiPACC - University of California, Santa Cruz
Word doc - UC-HiPACC - University of California, Santa Cruz

... So far, Kepler hasn’t yet found an identical twin to Earth: a rocky body of similar mass, sweet with liquid water, in the “Goldilocks zone” for temperatures just right for life as we know it to evolve. In fact, Kepler hasn’t yet found even an exoplanetary system resembling our Solar System, with roc ...
solar system - New Concept
solar system - New Concept

... Epimetheus and Janus, just inside the orbit of Mimas, are continually exchanging orbits with one another in a "waltz" -- they are called the coorbital satellites. ...
Planetary Configurations
Planetary Configurations

... out and spiralled in via interactions with protoplanetary disk. • Some have large eccentricities, which is similar to binary stars and may indicated Brown Dwarf companions (recall that Doppler gives only lower limits to companion mass). • Planets are “Jupiter-ish” and not likely habitable; however, ...
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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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