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finding masses of extrasolar planets
finding masses of extrasolar planets

... Each of the various techniques for finding extrasolar planets also provides extra information about the planets and their stars. For example, the Doppler technique gives us information about the star’s velocity toward or away from us, and from this we can find it’s mass. It is possible to calculate ...
Geochemistry & Lab
Geochemistry & Lab

...  The characteristics of the solar system 1. The sun occupies 99.8% of the total mass, but only 2% of the angular momentum 2. Seen from the sky far above the north pole, all the planets revolve around the Sun anticlockwise on the same plane. 3. They turn on their axis in the same direction with the ...
Claire
Claire

... First planet from the sun. There are no moon on Mercury. There are no rings on Mercury. There are 88 days in a year. 59 Earth days in a day. ...
ExamView - Untitled.tst - Newark Catholic High School
ExamView - Untitled.tst - Newark Catholic High School

... ____ 27. What is the main reason why Venus’ surface is so hot? a. the large number of volcanoes on Venus b. the very efficient greenhouse effect on Venus c. the extremely fast rotation of Venus d. the great amount of water on Venus ____ 28. Which of the following is one of the characteristics an obj ...
Chapter Overview
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... The four outer planets are very different from the small, rocky inner planets. Jupiter and Saturn, the two largest planets in the solar system, are considered gas giants, while Uranus and Neptune are called ice giants. The outer planets are very different from the terrestrials with regards to size, ...
Name ______ Per ______ Date ____________ SOLAR SYSTEM
Name ______ Per ______ Date ____________ SOLAR SYSTEM

... Read the information about Neptune you will find that Neptune is the last of a certain type of planet. What is the name given to planets like Jupiter, Saturn, Uranus, and Neptune? _____________________________________________________________ How many moons does Neptune have? ________________________ ...
Parallels: Proto-Planetary Disks and rings
Parallels: Proto-Planetary Disks and rings

... snow line or ice line) rocky objects become asteroids • Far from the Sun (outside frost-line) icy objects form the comets and Kuiper Belt Objects ...
Our Cosmic Neighborhood From our small world we have gazed
Our Cosmic Neighborhood From our small world we have gazed

... an atmosphere. Earth's atmosphere is primarily nitrogen and oxygen. Venus has a thick atmosphere of carbon dioxide, with traces of poisonous gases such as sulphur dioxide. Mars's carbon dioxide atmosphere is extremely thin. Jupiter, Saturn, Uranus, and Neptune are primarily hydrogen and helium. When ...
Components of the Solar System Learning Targets
Components of the Solar System Learning Targets

... straight line (inertia) Because the sun makes up 99% of the solar system’s mass, it has a very large gravitational pull that holds the planets and other objects in orbit. Target 5: The Galilean moons are the four largest moons of Jupiter (Io, Europa, Ganymede, and Callisto) and were first discovered ...
Orbital Motion
Orbital Motion

... A weather satellite completes a circular orbit every 3.5 hours. How far above the Earth’s surface is it? 2) A double star consists of two identical stars, each with a mass of 3.0 x 1030 kg. They are separated by 2.0 x 1011 m between their centres. How long do they take to complete one orbit? (p. 301 ...
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... University of Bonn and the Max-Planck-Institute for Radioastronomy (MPIfR) and the MPIfR's Dr. Wilhelm Altenhoff has now resolved this problem by using measurements of the amount of heat UB313 radiates to determine its size, which when combined with the optical observations also allows them to deter ...
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New "planet" is larger than Pluto

The Solar system
The Solar system

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On the Revolutions of Heavenly Spheres

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The Solar System
The Solar System

... August 25, 1989. Voyager 2 took many pictures of the planet, and much of what we know today about Neptune came from this single visit. These pictures show a brilliant blue planet with a few thin white clouds laced around its surface.  In Neptune's atmosphere, there is a large white cloud that moves ...
Life - Physics
Life - Physics

... galaxy you expect life within about 10 kpc of the center. • This would increase with time. • Develop inner boundary as metals get high. ...
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Objectives

... Many scientists have declassified Pluto from planetary status. They do not believe it qualifies as a major planet. ...
1 The Synodic and Orbit Periods of the Planets
1 The Synodic and Orbit Periods of the Planets

... Look up each planet's mean orbit radius (semimajor axis length) in millions of kilometers. Calculate the speed of each planet in km/hour from this radius and the time period P, assuming that its orbit is a circle in shape. Plot speed vs. planet number. Comment on the shape of the plot and why Copern ...
Study Guide - James E. Neff
Study Guide - James E. Neff

... Why does a rotating, collapsing cloud form a disk? Why do all the planets orbit the Sun in more or less the same direction the same plane? What is accretion, and why did collisions of planetesimals tend to accrete into larger planets rather than blasting each other into smaller fragments? The inner ...
The Synodic and Orbit Periods of the Planets
The Synodic and Orbit Periods of the Planets

... Look up each planet's mean orbit radius (semimajor axis length) in millions of kilometers. Calculate the speed of each planet in km/hour from this radius and the time period P, assuming that its orbit is a circle in shape. Plot speed vs. planet number. Comment on the shape of the plot and why Copern ...
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... the discovery of Eris, which is larger than Pluto, a formal definition of “planet” was developed that reclassified Pluto as a dwarf planet. The IAU definition: A “planet” is a celestial body that: (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body for ...
A105 –Stars and Galaxies
A105 –Stars and Galaxies

... in terms of AU (1 AU = 1 astronomical unit, the average distance between the Earth and the Sun, about 150,000,000 kilometers). Again we will use the laws of orbital motion from Chapter 5. The formula is ...
Grade 3: Solar System
Grade 3: Solar System

... markers to create their orbits. Upon completion of all strings being put into place, each student group will choose one member to stand on their orbit strings in a straight line away from the sun. Students who are not participating will stand outside the solar system and observe the planets’ rotatio ...
Document
Document

... (Jupiter, Saturn, Uranus and Neptune) are the Jovian planets. An asteroid belt lies between the inner and outer planets. The outermost icy planet, Pluto, is in a class called Trans-Neptunian Objects (TNO). It’s a dwarf planet. ...
Planetary Sciences
Planetary Sciences

... 5. find Icarus online (or in the library) 6. choose 3 planetary topic(s) you are most interested in --- start project EARLY 7. do homework --- Solar System Explorers, quizzes, etc. ...
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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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