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Program Information Packet
Program Information Packet

... AIR PRESSURE: The force exerted on an object by the atmosphere. ATMOSHERE: A layer of gas held around a planet by its gravity. COMET: A small, frozen object made of ice, dust, ammonia and organic matter that orbits the Sun. CHEMICAL CHANGE: A change by which one or more new substances are formed. Th ...
Chapter 08
Chapter 08

... force. Strong force is strongest of the 4 known forces: electromagnetic, weak, strong, gravitational. ...
So What All Is Out There, Anyway?
So What All Is Out There, Anyway?

Constellations
Constellations

... How stars would appear if they were all the same distance from earth. All stars place 32.6 LY from the sun Our sun abs. Mag = 4.8 Negative is brighter ...
Stars - Robert M. Hazen
Stars - Robert M. Hazen

... The Nebular Hypothesis ...
Ch11_Lecture
Ch11_Lecture

... back to when they first condensed from the solar nebula • Some chondrules contain ancient dust grains that have survived from before the Solar System’s birth! ...
Friday, Sep. 5
Friday, Sep. 5

... Syllabus, class notes, and homeworks are at: www.as.utexas.edu  courses  AST 301, Lacy Reading for this week: chapter 3 (4 by next Wednesday) The homework handed out today is due in two weeks. It requires observations of the Moon and planets. We will take this week’s homework next Monday if you ha ...
The Stars - Department of Physics and Astronomy
The Stars - Department of Physics and Astronomy

... Corona ...
Lecture 3
Lecture 3

... Jupiter's face at different rates. For example, the outermost moon Callisto orbits the slowest of the three satellites. Callisto's shadow moves across the planet once for every 20 shadow crossings of Io. Add the crossing rate of Ganymede's shadow and the possibility of a triple eclipse becomes even ...
Tips Packet part 2 - Doral Academy Preparatory School
Tips Packet part 2 - Doral Academy Preparatory School

... just a few hours to reach the outer planets. • Over the course of a year, light travels 5.87849981 x 1012 miles. Written out, that’s 5,878,499,810,000 miles= 1 year ...
Properties of Stars
Properties of Stars

...  Death of Medium-Mass Stars • Stars with masses similar to the sun evolve in essentially the same way as low-mass stars. • During their collapse from red giants to white dwarfs, mediummass stars are thought to cast off their bloated outer layer, creating an expanding round cloud of gas called plane ...
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... •  The Earth is a sphere but it is not perfectly round. It is slightly flattened at the poles. ...
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Sun and Other Stars Notes

... (low mass stars die gently while high mass stars die catastrophically) -When all H is gone a star gets brighter and over 100 million years grows to a red giant and moves to the cooler position on the HR Diagram -The Sun grows to 8 times the mass of the Sun- (considered a high mass star) -What happen ...
Astronomical co-ordinates
Astronomical co-ordinates

... 1B11 Precession and Nutation • Precession occurs due to the gravitational pull of the Sun and the Moon (mostly the Moon). • Over 26,000 years, the positions of the celestial poles and the equinoxes change with respect to the stars. • Thus it is always necessary to specify a date for equatorial co-o ...
Stars and The Universe
Stars and The Universe

Astronomy Through the Ages: 2 Middle ages through Renaissance
Astronomy Through the Ages: 2 Middle ages through Renaissance

... Mars than any other planet. – But the Mars positions Tycho had recorded did not fit well with any of the models, Ptolemy’s, Copernicus’ or Tycho’s. – The best match of Mars data to a Copernican orbit left him with an discrepancy of 8 arc minutes. • It was larger than the accuracy of Tycho’s data (wh ...
The Planets
The Planets

... be roughly spherical in shape but not massive enough to undergo thermonuclear fusion in their cores like a star. ...
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1. Heraclides of Pontus

... observation supported the heliocentric model, because the moons were in orbit around Jupiter, and did not orbit earth. In the geocentric model, everything orbits earth. The church did not like these findings, since they strongly supported the geocentric model, and thought earth had to be in the cent ...
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... Meridian. A circle of longitude passing from the South point of the horizon, through the zenith to the North point of the horizon. It coincides with geographical longitude - a great circle crossing the equator and passing through the poles. Every point on the Earth's surface has its own meridian or ...
Galileo`s Motion, Newton`s Gravity
Galileo`s Motion, Newton`s Gravity

Lecture03
Lecture03

... In the movie below, you will see the Sun, Mercury, Venus, Earth, Mars, Jupiter, and Saturn looking down on the plane of the solar system from the Earth’s perspective ...
MT 2 Answers Version A
MT 2 Answers Version A

... It is converted into light energy, giving o↵ a flash of light upon impact. ...
MT 2 Answers Version D
MT 2 Answers Version D

... 22. Examine the figure below. What method of looking for extrasolar planets requires the planet to pass in front of the star? ...
Jupiter Reading Comprehension Worksheet
Jupiter Reading Comprehension Worksheet

... the largest planet in our solar system and the fifth planet from the Sun. It is so large that all of the other planets in the solar system could fit inside of it. Jupiter has the most natural satellites or moons of any planet. The count is currently at 63, although not all of them have been named. I ...
MT 2 Answers Version C
MT 2 Answers Version C

... 11. Which sequence correctly lists the spectral classes of stars in order of decreasing temperature (from hottest to coolest)? (a) ...
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Formation and evolution of the Solar System



The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.
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