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a description of planets and stars you may see
a description of planets and stars you may see

... ring system and at least 63 moons, including the four large moons called the Galilean moons that were first discovered by Galileo in 1610. Uranus is the seventh planet from the Sun. It has the third-largest planetary radius and fourth-largest planetary mass in the Solar System. Herschel discovered U ...
Outer Planets Review Sheet with answers: 1.) Give the order of the
Outer Planets Review Sheet with answers: 1.) Give the order of the

... b.) The object must have enough mass for its gravity to have pulled it into a sphere shape. c.) The Planet must have cleared its orbit. (The objects orbiting the planet must not combine to make up more than half of the actual planet’s size.) 40.) Which of these rules did Pluto fail? (1 Mark) Pluto f ...
The Planets
The Planets

...  Most meteoroids originate from any one of the following three sources: (1) interplanetary debris that was not gravitationally swept up by the planets during the formation of the solar system, (2) material from the asteroid belt, or (3) the solid remains of comets that once traveled near Earth’s or ...
IMPORTANT HISTORICAL DATES AND EVENTS
IMPORTANT HISTORICAL DATES AND EVENTS

... at just the right distance to hold on to watery oceans and host the chemical of life. The planets can be divided up into two groups of four. Closest to the sun are the four inner planets, Mercury, Venus, Earth and Mars. The inner planets are compact and rocky with just three moons between them. They ...
SES4U ~ The Formation of Our Solar Systemstudentcopy
SES4U ~ The Formation of Our Solar Systemstudentcopy

... • These grains will settle to the disk midplane since they are heavier than the H and He gas. What happens next is uncertain. – One possibility is that the thin disk of dust is gravitationally unstable, leading to the formation of roughly 1 kilometer size objects known as planetesimals. – Another po ...
Moons of the Solar System Curriculum
Moons of the Solar System Curriculum

... (energy) through nuclear fusion and rotates on its axis, but it remains in an essentially constant position. A planet rotates on its axis and orbits a star. A moon rotates on its axis and orbits a planet while the planet orbits its star. Note: The above is a very simple and broad definition for plan ...
Saturn
Saturn

... 9. Ring material may come from ripped up moons. The point where the gravitational pull of Saturn equals the structural integrity of the moon itself is the _______________ _________________. This is also called the tidal stability limit. Page 310 10. The largest gap in the rings is called the _______ ...
Study Guide 2 - Otterbein University
Study Guide 2 - Otterbein University

Powerpoint 2003
Powerpoint 2003

... telescope to make detailed observations of the sky Though he did not invent the telescope, he made many working prototypes and trained them on a variety of celestial bodies ...
Pluto and the Kuiper Belt
Pluto and the Kuiper Belt

... 100 km diameter. Pluto is distinguished from other Plutinos only because it is bigger: it is 2374 km in diameter. Even Charon, is 1212 km in diameter. Quaoar (discovered 2002) is 1200 km in diameter. Ixion is 1065 km in diameter. Why is the 3:2 resonance so full? We believe that, via angular momentu ...
History of astronomy
History of astronomy

... Why were there no telescopes prior to 1600? Consider the following passage, from the Opus Majus of Roger Bacon (1267): “Greater things than these may be performed by refracted vision. For it is is easy to understand by the canons above mentioned that the greatest things may appear exceeding small, ...
Gravitation
Gravitation

... measurements reveal variations in the density of underground rock. This information can be used to indicate whether resources like oil are possibly present. Suppose a certain type of gravimeter has a test mass of 0.500 kg inside it. How large is the gravitational force between this mass and a mounta ...
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Document

... very large magnetic fields. – Jupiter’s is 20,000 times as strong as Earth’s, and if it were visible, would appear larger than the full Moon in our sky. – Saturn’s field is 500 times as strong as Earth’. ...
Page 1 of 5
Page 1 of 5

... Europa, and we know that Europa has an outer layer of water 100 to 200 km thick. If the temperature rises to about 250 K at the bottom of this layer, there might be an ocean. (As mentioned in lecture, Ganymede's magnetic field also suggests the possibility of a liquid "water sandwich" below Ganymede ...
AGU Fall 2011 SH34B-08
AGU Fall 2011 SH34B-08

... length of the cycle was close to the orbital period of Jupiter. He even constructed a formula involving the periods of Jupiter, Saturn, Venus, and Earth that reproduced the sunspot numbers 1834-1858. Unfortunately the formula failed for both earlier and subsequent cycles and Wolf concluded at the en ...
solar system form
solar system form

... • The only surface liquid water in the solar system ...
GalileoPresentation by Jeremy - Math-Around-the
GalileoPresentation by Jeremy - Math-Around-the

... The Catholic Church persecuted Galileo for his support of Copernicus’ Heliocentric theory, wherein the Earth orbited the Sun instead of the Sun orbiting the Earth as the Church taught. Seen as a heretic, he tried to appeal to the oppressive church by stating that “Mathematics is the language in whic ...
Taylor - St. Brigid
Taylor - St. Brigid

... ‡ One year equals 12 Earth years long ‡ One day equals 9.8 hours long ...
Welcome to Our Universe!
Welcome to Our Universe!

... • Closest planet to the size of Earth • Has a thick mantle and iron core • Much drier than Earth and atmosphere is 90% more dense • Hottest planet  Over 400⁰C • No moons • Terrestrial Planet • 7,521 miles in diameter ...
Solar System
Solar System

... called Triton which is the largest of them all. The color of Neptune is blue its is because they are full of methane gas. Neptune tilted around 28.3 degrees and is tilting from right to left. The name of Neptune is from the god of the sea in the Roman Mythology, and their moons are called after Mino ...
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 ...
By: Kaylea Stone, Kalena Karp, Megan
By: Kaylea Stone, Kalena Karp, Megan

... high to support life on Mercury. To date, there is no evidence that there is life on Mercury. ...
13 - Joe Griffin Media Ministries
13 - Joe Griffin Media Ministries

... since the planet seems to be moving in a direction opposite to that which is typical for planets. Finally as Earth swings past the planet in its orbit, it appears to resume its normal west-to-east drift on successive nights.1 With at least a cursory understanding of retrogradation of planets viewed ...
Untitled - IES Bachiller Sabuco
Untitled - IES Bachiller Sabuco

... largest of the nine planets. The temperature on Mercury ranges from 90 K to 700 K. Mercury is a small, rocky planet which looks like our Moon. It is covered with craters and it has nearly changed since it was created by a very large crash early in the history of the solar system. One of Mercury's la ...
Chapter 16 - The Solar System
Chapter 16 - The Solar System

... Jupiter also has a ring system ...
< 1 ... 6 7 8 9 10 11 12 13 14 ... 22 >

Galilean moons



The Galilean moons are the four largest moons of Jupiter—Io, Europa, Ganymede, and Callisto. They were discovered by Galileo Galilei around January 1610 and were the first group of objects found to orbit another planet. Their names derive from the lovers of Zeus. They are among the most massive objects in the Solar System with the exception of the Sun and the eight planets, with radii larger than any of the dwarf planets. Ganymede is the largest moon in the Solar System, and is even bigger than the planet Mercury. The three inner moons—Io, Europa, and Ganymede—are in a 4:2:1 orbital resonance with each other.The Galilean moons were discovered in either 1609 or 1610 when Galileo made improvements to his telescope, which enabled him to observe celestial bodies more distinctly than ever. Galileo's discovery showed the importance of the telescope as a tool for astronomers by proving that there were objects in space that cannot be seen by the naked eye. More importantly, the incontrovertible discovery of celestial bodies orbiting something other than Earth dealt a serious blow to the then-accepted Ptolemaic world system, or the geocentric theory in which everything orbits around Earth.Galileo initially named his discovery the Cosmica Sidera (""Cosimo's stars""), but the names that eventually prevailed were chosen by Simon Marius. Marius discovered the moons independently at the same time as Galileo, and gave them their present names, which were suggested by Johannes Kepler, in his Mundus Jovialis, published in 1614.
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