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... – How does it collapse – What heats it up ...
Characteristic Properties
Characteristic Properties

... NOT evidence that the planets formed in a disk surrounding the Sun is: a)  The planets orbits are inclined only a few degrees to the equator of the Sun (=ecliptic) b)  The planets all orbit in the same direction as the Sun rotates c)  We see protoplanetary disks around other stars in star formation ...
Universal Gravitation
Universal Gravitation

... distance from the Earth the less it will weigh.  No matter how great the distance Earth’s gravity does not drop to zero.  The gravitational influence of every object is exerted through all space. ...
The formation of the Solar system
The formation of the Solar system

... a protoplanet due to the large gravitational field of Jupiter constantly disturbing their motion. These are in the asteroid belt and also include the Trojan asteroids. • Planetesimals further out were “kicked” into outer orbits and form the Oort cloud. • Most planetesimals formed beyond Neptune are ...
Kepler 186f - Forum Skylive
Kepler 186f - Forum Skylive

... Since 2012, the SETI Institute’s Allen Telescope Array in northern California, near Mt. Lassen, has been observing all reported Kepler candidate exoplanets in search of signals from extraterrestrial technological civilizations. This search is looking for patterns in frequency and time that could ind ...
2- Origin of the Universe
2- Origin of the Universe

... • Contain thousands of icy and rocky objects • Kuiper Belt – Neptune to about 30 to 55 AU • Oort Cloud – from 5000 AU to 100000 AU  Pluto and Eris are the best known dwarf planets found in Kuiper belt Pluto was reclassified as a dwarf planet in ...
Classroom activity
Classroom activity

... diameter to tiny piece of dust. However, unlike Saturn, Uranus’s rings are dark and very difficult to see. Neptune has the fastest winds of any planet in the solar system. The winds of this gas giant can reach 1,200 mi/hr. Pluto is the smallest, coldest planet in the solar system. It is the only one ...
Visiting Pluto
Visiting Pluto

physics140-f07-lecture21 - Open.Michigan
physics140-f07-lecture21 - Open.Michigan

... evaluation, advice, diagnosis or treatment by a healthcare professional. You should speak to your physician or make an appointment to be seen if you have questions or concerns about this information or your medical condition. Viewer discretion is advised: Material may contain medical images that may ...
Universal Gravitation Principle of Superposition Gravity and the Earth
Universal Gravitation Principle of Superposition Gravity and the Earth

... all other mass. This is the rst time the concept of gravity was extended beyond the earth to include planets, moons, and stars. Through careful measurements, he was able to show that the force causing the curved path of the moon was the same as the force causing objects to fall to the earth. Newton ...
Benchmark One Study Guide: Science Benchmark Wed
Benchmark One Study Guide: Science Benchmark Wed

... 2. What two factors affect the gravitational force between two objects? Mass and Distance 3. Why do the planets revolve around the Sun? Because the Sun is the largest object in our solar system, it has the most mass, so it has the strongest gravitational force. 4. Why does the moon revolve or orbit ...
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Hubble observations of Ceres and Pluto:

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Science 1 (MillinerSci1)

... 13. In a family of rabbits, half the rabbits are brown and half are white. Which statement BEST explains why the rabbits have two different colors? A. The white rabbits were in the Sun more than the brown rabbits. B. The brown rabbits inherited different coat colors than the white rabbits. C. The br ...
pals_20160211_howpla.. - Department of Physics and Astronomy
pals_20160211_howpla.. - Department of Physics and Astronomy

... “Drag” from proto-planetary nebula gas? Gravitational interactions with each other? We think that Uranus & Neptune formed closer to Sun, were flung to their present orbits by interactions with Jupiter, maybe Saturn ...
Women`s Club Hockey team > places second at NEWCHA finals
Women`s Club Hockey team > places second at NEWCHA finals

... thing seen orbiting the sun to call Sedna a new planet," since the discovery of Pluto in Brown said. "But at the same 1930, and the questions it time, we think it's not reasonraises have astronomers both able to call Pluto a planet, eibaffled and excited. "Very ther." What is exciting for scilittle ...
general information on uranus
general information on uranus

...  The density of Venus is 5,240 kg/m3, _________________________________________ and the third densest planet in our Solar System LENGTH OF A DAY AND YEAR ON VENUS  Each day on Venus __________________________________. It takes 224.7 Earth days for Venus to __________________________________. The s ...
- IIT Kanpur
- IIT Kanpur

... But comets emerging out of the ‘Ourt Cloud’ have disordered orbit. Comets are mainly of two types. Those of the first type take more than 200 years for revolution around the sun and others takes less than 20 years. 'Ourt Cloud’ hypothesis gives a correct explanation about the orbit's inclination and ...
Our Space Journey
Our Space Journey

... How come earth spins but the sun doesn't? It takes the sun 25 days to go all the way round and it takes 24 hours to rotate. The earth is the third planet from the sun. As the earth orbits the sun the moon orbits the sun as well. Moon orbit takes 27 1/2 days but ... Because earth keeps on moving it ...
Neptune Nachman
Neptune Nachman

PPT - El Camino College
PPT - El Camino College

PH507 - University of Kent
PH507 - University of Kent

... 4. The temperature of an opaque cloud is measured to be 20K. Find the wavelength of the peak blackbody emission. In which part of the electromagnetic spectrum does the peak lie? ...
6 Scale Model of the Solar System
6 Scale Model of the Solar System

... in New Mexico is 455 miles. Using this distance to represent the Sun to Pluto distance (40 AU), and assuming that the Sun is located at the start of I-25 here in Las Cruces and Pluto is located along the Colorado-New Mexico border, you will determine: • the scaled locations of each of the planets in ...
Mountain-Skies-2016-0718
Mountain-Skies-2016-0718

... moves  away  from  it  but  still  outshines  any  of  the  stars  in  the  sky.    The  observer  with  a  good  telescope   can  still  make  out  some  of  the  markings  on  the  surface.    (With  the  exception  of  Mercury,  Mars  is  the  only   planet  whose  surface  marking  can  be  obse ...
6 Scale Model of the Solar System
6 Scale Model of the Solar System

... in New Mexico is 455 miles. Using this distance to represent the Sun to Pluto distance (40 AU), and assuming that the Sun is located at the start of I-25 here in Las Cruces and Pluto is located along the Colorado-New Mexico border, you will determine: • the scaled locations of each of the planets in ...
Gravitation Problems
Gravitation Problems

... 1992M3. A spacecraft of mass 1,000 kilograms is in an elliptical orbit about the Earth, as shown above. At point A the spacecraft is at a distance rA = 1.2 x 107 meters from the center of the Earth and its velocity, of magnitude VA = 7.1 x 103 meters per second, is perpendicular to the line connect ...
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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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