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AST 207 7 Homew
AST 207 7 Homew

... magnitude or the stars distance from f us. c. (3 pts.) If you turneed the setting on the hot plaate from “higgh” to “mediuum,” how wouuld its i the HR diagram change?? place in It wou uld move to th he right and down. Doing this would firrst, decrease tthe temperatuure, thus reeddening the star s an ...
Larger, high-res file, best for printing
Larger, high-res file, best for printing

... Percival Lowell. Lowell and others believed that there were discrepancies between prediction and observation of the motions of Uranus and Neptune, which might be explained by the gravitational effects of a ninth planet. In the Publications of the Astronomical Society of the Pacific for December 1930 ...
Astronomy for Kids - Uranus
Astronomy for Kids - Uranus

... Uranus, along with Neptune and Pluto, is in the most distant region of our solar system. The giant planet, which is another of the gas giants of our solar system, is more than twice as far away from the Sun as Saturn. If you get a chance to look at Uranus through a telescope, all you will see is a f ...
Answer key for Space study guide
Answer key for Space study guide

... After 4 years the .26 of a day or (6 hrs) each year causes there to be an extra day in a year. The extra day is added to the month of February, you will have 29 days that year (Leap ...
Stellar Evolution Chapter 12
Stellar Evolution Chapter 12

... b. Objects below this mass can only form in HI clouds. c. Objects below this mass are not hot enough to fuse normal hydrogen. d. They form too slowly and hot stars nearby clear the gas and dust quickly. e. Our telescopes do not have enough light gathering power to detect dim objects. ...
Stars - Mike Brotherton
Stars - Mike Brotherton

... If an accreting white dwarf exceeds the Chandrasekhar mass limit, it collapses, triggering a type Ia supernova. ...
What makes stars tick?
What makes stars tick?

... beautiful images in the sky. A planetary nebula is the remnant outer layers from a Sun-like star. ...
Habitability: Good, Bad and the Ugly
Habitability: Good, Bad and the Ugly

... – Volcanic activity but no re-cycling of CO2 (small size preclude plate tectonics) – Higher/thicker atmosphere = Earth early in evolution – Evidence of liquid H20 is great (lab last week) • Dry channels and valley etched by liquid H2O; sedimentary ...
Lecture 3
Lecture 3

... atmosphere. Temperature is just a measure of the average velocity of the atoms and molecules in a gas. For a relatively cool gas there are: (1) Few atomic collisions with enough energy to knock electrons up to the 1st excited state so the majority of the H atoms are in the ground state (2) Few oppor ...
Week8Lecture1
Week8Lecture1

Comets, Meteors, and Asteroids
Comets, Meteors, and Asteroids

... caused by the shadow of the Earth on the Moon Truth: Phases of the Moon are caused by our changing view of the illuminated side of the Moon • ½ of the Moon is always illuminated by the Sun ...
Death Mystery Of Subhash Chandra Bose
Death Mystery Of Subhash Chandra Bose

... However, his body was never recovered, and many theories have been put forward concerning his possible survival. One such claim is that Bose actually died in Siberia, while in Soviet captivity. Several committees have been set up by the Government of India to probe into this matter. Here I have cons ...
Neither Star nor Planet - Max-Planck
Neither Star nor Planet - Max-Planck

Announcements - Lick Observatory
Announcements - Lick Observatory

... • The central `star’ isn’t a star because it has no energy source. This is a white dwarf. • Supported against gravity by e- degeneracy. • Lots of residual heat, no energy source, a white dwarf is like a hot ember. As it radiates energy into space, the white dwarf cools off. • There is an upper limit ...
Explosion of Sun - Scientific Research Publishing
Explosion of Sun - Scientific Research Publishing

... The Sun is about halfway through its main-sequence evolution, during which nuclear fusion reactions in its core fuse hydrogen into helium. Each second, more than 4 million tonnes of matter are converted into energy within the Sun’s core, producing neutrinos and solar radiation; at this rate, the sun ...
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... Many Greek thinkers worried about the movement of stars and planets. The most prominent among them was Eudoxus (410–355 bc, or 408–347 bc). He belonged to Plato’s academy in Athens. Deeply influenced by Plato’s appeal for perfect geometrical forms (sphere, regular solids and so on), Eudoxus proposed ...
Night Sky
Night Sky

... Many people think that lunar phases are caused by Earth's shadow on the Moon They think that the Moon is a thin crescent in the sky rather than a full circle because Earth's shadow is falling on the Moon making most of the circle dark. If Earth's shadow falling on the Moon caused lunar phases, then ...
Draft Science Cases for KPAO
Draft Science Cases for KPAO

... Finally it should be noted that Keck’s highly structured PSF (with a lot of coherence and energy in the wings) will make any high dynamic range imaging very difficult. The need to develop some way to reconstruct the exact (as opposed to statistical) PSF would be crucial for such applications; this i ...
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200 THE COPERNICAN REVOLUTION the opposition to
200 THE COPERNICAN REVOLUTION the opposition to

... as clear as Venus at its greatest brightness; during the next eighteen months the new occupant of the heavens grew gradually dimmer; and finally it vanished altogether early in 1574. From the start the new visitor drew the interest of scientists and nonscientists throughout Europe. It could not be a ...
Review Sheet // Study Guide: ESS Semester II 2002
Review Sheet // Study Guide: ESS Semester II 2002

Assessment Schedule
Assessment Schedule

... • Hydrogen runs out. • When it cannot fuse iron, the core will collapse and then explode. • Star core collapses due to gravity and the outer layers of the star are exploded out. • A very dense neutron star or a black hole remains. • The variability in brightness caused by the gases and plasma explod ...
Level 2 Science (90764) 2011 Assessment Schedule
Level 2 Science (90764) 2011 Assessment Schedule

... • Hydrogen runs out. • When it cannot fuse iron, the core will collapse and then explode. • Star core collapses due to gravity and the outer layers of the star are exploded out. • A very dense neutron star or a black hole remains. • The variability in brightness caused by the gases and plasma explod ...
The birth and life of stars
The birth and life of stars

...  Main-sequence stars with mass between 0.08 and 0.4Msun convert all of their mass into helium and then stop fusing. Their lifetimes last hundreds of billions of years, so none of these stars has yet left the main sequence.  Core hydrogen fusion ceases when hydrogen is exhausted in the core of a ma ...
Student Created Jeopardy
Student Created Jeopardy

... Solar System Jeopardy ...
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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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