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Contact: Sharon Worthy
Contact: Sharon Worthy

... that two Earths would fit in it. The spot is thought to be a high-pressure weather system. Befitting such a behemoth, astronomers so far have discovered 61 celestial bodies orbiting Jupiter, including four large moons, three of which are larger than Earth’s moon. The Galileo spacecraft was launched ...
Sun`s energy and interior
Sun`s energy and interior

... (http://nobelprize.org/nobel_prizes/physics/articles/bahcall/) ...
EUV and Soft X-ray Optics, Thin Films and Outer Space.
EUV and Soft X-ray Optics, Thin Films and Outer Space.

... history of water on the surface of Mars, where has all of this water gone? Several speculations state that the water exists frozen beneath the permafrost of the planets surface. Another speculation is that water on Mars evaporated into its atmosphere where it was then literally blown away by the sol ...
Solar-cycle variation of low density solar wind during
Solar-cycle variation of low density solar wind during

... from density-depleted prominence cavities. The plasma inside ejecta at 1 AU is not always low density however. Intrinsically higher density plasma, for example including prominence material, may be encountered, and plasma compression may also occur, for example at the leading edge where the ejecta i ...
Strong
Strong

... shadows on each other. Most parts of the rings are only about 10 meters thick, due to the energy lost during collisions between ring particles. However, observations of the rings planned by SwRI Cassini scientists and colleagues during this year’s “equinox” have shown that some parts of the rings ar ...
Origin of the Solar System
Origin of the Solar System

... The Great Nebula in Orion is one of the most interesting of all astronomical nebulae known. Here 15 pictures from the Hubble Space Telescope have been merged to show the great expanse and diverse nature of the nebula. In addition to housing a bright open cluster of stars known as the Trapezium, the ...
Astronomy Jeopardy
Astronomy Jeopardy

... What is Uranus? ...
Lesson 28 - Purdue Math
Lesson 28 - Purdue Math

... Finally Kepler (1571-1630) is credited with discovering that the planets revolve in elliptical orbits about the sun. He wrote 3 laws of planetary motion. The first law states: The orbit of each planet in the solar system is an ellipse with the sun as one focus. (The sun is not at the center or an or ...
a-cr-ccp-803/pf-001 15-5-1 royal canadian air cadets
a-cr-ccp-803/pf-001 15-5-1 royal canadian air cadets

... The twin spacecraft Voyager-1 and Voyager-2 were launched by NASA in the summer of 1977 from Cape Canaveral, Florida. The Voyagers were to conduct close-up studies of Jupiter, Saturn, Saturn’s rings and the larger moons of the two planets. To accomplish their two-planet mission, the spacecraft were ...
Big Idea 5
Big Idea 5

... H-R Diagram ...
Formation of the Solar System
Formation of the Solar System

... contain grains of compounds that are expected to have formed in a cooling cloud of cosmic abundance at temperatures of a few hundred degrees. ...
HIGHLIGHTS: this week in A&A Volume 462-3 (February II 2007)
HIGHLIGHTS: this week in A&A Volume 462-3 (February II 2007)

... “The widest ultracool binary”, by J.A. Caballero A&A 462, p. L61 The leading scenario for the formation of brown dwarfs and very low-mass stars is that they are ejected from their formation region before they have a chance to accrete more mass, and it predicts that pairs of very low mass stars must ...
The Sun - Sheldon ISD
The Sun - Sheldon ISD

... Solar flares take place in the corona. They are enormous discharges of magnetic energy. Huge streams of protons and electrons are sent into space. They can interrupt communications networks on earth. Did you know that there are solar winds? They result from the expansion of gas in the corona. The io ...
May - RASC Hamilton
May - RASC Hamilton

... traveled 950 kilometres from Toronto to Ottawa, Illinois to find clear skies, and produced the image on the front cover of Orbit this month. It is one of the most beautiful pictures of a lunar eclipse I’ve seen, and it captures perfectly the sort of view I’d expect through a wide field eyepiece or a ...
File
File

... made up of two protons and one neutron 3. Two nuclei made up of two protons and one neutron collide and fuse—as this fusion happens two protons are released, the remaining fuse together and form a helium nucleus How much less mass does a helium nucleus have compared to a hydrogen nucleus? 0.7% ...
The Asteroid Belt as the Consequence of Resonance Density
The Asteroid Belt as the Consequence of Resonance Density

... organization of the transformation of virtual particles to real particles or influence the types of elements with their specific numbers of protons and electrons could be examined. There might be a potential mechanism to explain why carbon-endowed asteroids dominate the proximal asteroids, while sil ...
Cosmic Collisions
Cosmic Collisions

... scattered in random directions, but gravity acts so gradually that planetary orbits are not disturbed. A collision takes about a billion years; during the last billion years, life on Earth evolved from single-celled organisms to amazingly primative apes who still think digital watches are pretty nea ...
No Slide Title
No Slide Title

... – Saturn is 95 times the mass of the Earth and takes over 29 y to orbit the sun. It rotates in 10.7 h. – Saturn’s rings are narrow bands of tiny particles of dust, rock, and ice. – Saturn has more than 40 satellites. • Saturn may still be forming. – Saturn radiates three times more energy than it re ...
Chapter 6 The Solar System
Chapter 6 The Solar System

... Conservation of angular momentum says that product of radius and rotation rate must be constant ...
Chapter 6 The Solar System
Chapter 6 The Solar System

... Conservation of angular momentum says that product of radius and rotation rate must be constant ...
answers
answers

... C) in random directions A) The movement of the particles is mostly random but there will be a net spin sin some direction. This will become more evident as the mass pulls in, in the same way that a figure skater spins faster when the arms are pulled in. Demonstrate this with the rotating platform. b ...
Catherine and Puti 7F
Catherine and Puti 7F

... yellow star which scientists have named Sol, after the ancient Roman name. This is why our system of planets is called the Solar System. There are trillions of other stars in the universe just like it. Many of these stars have their own systems of planets, moons, asteroids, and comets. ...
3D SOLAR SYSTEM MOBILE
3D SOLAR SYSTEM MOBILE

... The planets move around the Sun in paths called orbits. The orbits are roughly circular (in reality they are ellipses). The further a planet is from the Sun, the longer its orbit, and the longer its year (the time it takes to complete one orbit). The force of gravity attracts all objects to all othe ...
Formation of solar system HW
Formation of solar system HW

... Meanwhile, the outer parts of the disk were cooling off. Matter condensed from the cloud and small pieces of dust started clumping together. These clumps collided and combined with other clumps. Larger clumps, called planetesimals, attracted smaller clumps with their gravity. Gravity at the center o ...
Book 2, Chapter 1 - Magnetism – Quizzes Quiz 1 and 2 – label the
Book 2, Chapter 1 - Magnetism – Quizzes Quiz 1 and 2 – label the

... 4. If you follow a compass pointing north, will you reach the geographic north pole? Explain your answer. 5. A(n) ________________________ is a device that has a magnetized needle that can spin freely. 6. ________________________________ is the angle between geographic north and the north to which a ...
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Heliosphere



The heliosphere is the bubble-like region of space dominated by the Sun, which extends far beyond the orbit of Pluto. Plasma ""blown"" out from the Sun, known as the solar wind, creates and maintains this bubble against the outside pressure of the interstellar medium, the hydrogen and helium gas that permeates the Milky Way Galaxy. The solar wind flows outward from the Sun until encountering the termination shock, where motion slows abruptly. The Voyager spacecraft have actively explored the outer reaches of the heliosphere, passing through the shock and entering the heliosheath, a transitional region which is in turn bounded by the outermost edge of the heliosphere, called the heliopause. The overall shape of the heliosphere is controlled by the interstellar medium, through which it is traveling, as well as the Sun, and does not appear to be perfectly spherical. The limited data available and unexplored nature of these structures have resulted in many theories.On September 12, 2013, NASA announced that Voyager 1 had exited the heliosphere on August 25, 2012, when it measured a sudden increase in plasma density of about forty times. Because the heliopause marks one boundary between the Sun's solar wind and the rest of the galaxy, a spacecraft such as Voyager 1 which has departed the heliosphere can be said to have reached interstellar space.
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