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Section 3: Evolution of Stars pages 114-119
Section 3: Evolution of Stars pages 114-119

The power plant of the Sun and stars
The power plant of the Sun and stars

... MS stars fuse hydrogen into helium, releasing prodigious amounts of energy in the process. Their fuel source is the matter of which they are made ...
A small mass difference between Hydrogen and Helium The
A small mass difference between Hydrogen and Helium The

... Sun, but what is going on on the rest of the Main Sequence? ...
Open clusters
Open clusters

The Hidden Lives of Galaxies NSTA 2001
The Hidden Lives of Galaxies NSTA 2001

... • Under collapse, protons and electrons combine to form neutrons. • 10 Km across Black Hole (If mass of core > 5 x Solar) • Not even compacted neutrons can support weight of very massive stars. ...
Challenging our Understanding of Stellar Structure and Evolution
Challenging our Understanding of Stellar Structure and Evolution

... • Pre-Main Sequence Stars. With the exception of solar mass objects, evolution of stars from birth to the zero-age main sequence is poorly calibrated (Schaefer et al. 2008 and references therein). Binaries in star formation regions provide an opportunity to determine precise dynamical masses in low- ...
Chapter 28 – Stars and Galaxies
Chapter 28 – Stars and Galaxies

...  If a Cepheid is located in another galaxy, astronomers can find the distance to these galaxies by comparing absolute and apparent ...
1. Introduction
1. Introduction

... Stars whose luminosity varies periodically have been known for centuries. However, only within the last hundred years has it been definitely established that in many cases these variations are due to intrinsic pulsations of the stars themselves. For obvious reasons studies of pulsating stars initial ...
Star Types
Star Types

... Most stars appear on the Main Sequence, where stars appear to obey a Mass-Luminosity relation: L  M3.5 For example, if the mass of a star is doubled, its luminosity increases by a factor 23.5 ~ 11. Thus, stars like Sirius that are about twice as massive as the Sun are about 11 times as luminous. Th ...
Chapter 25 - Notes Super Size
Chapter 25 - Notes Super Size

... Stars & Galaxies Stars Constellations • _________________ of stars representing mythological characters, animals, or familiar objects. • Most constellations come from the _________________. • The stars in a constellation may appear close, however each star can be _________________ of light-years awa ...
Earth Science Unit Test Review
Earth Science Unit Test Review

answers - Salem State University
answers - Salem State University

August Evening Skies
August Evening Skies

... The planet Jupiter is plotted at map time, mid-August 2008. Seven objects of first magnitude or brighter are visible. In order of brightness they are: Jupiter, Arcturus, Vega, Altair, Antares, Spica, and Deneb. In addition to stars, other objects that should be visible to the unaided eye are labeled ...
The science potential of atmospheric Cherenkov arrays used as intensity interferometers
The science potential of atmospheric Cherenkov arrays used as intensity interferometers

... At least 50 young stars for which CTA-I.I. could provide images ...
Stellar Evolution
Stellar Evolution

... • When energy is used, it shrinks to make a white dwarf ...
Section 19.2
Section 19.2

Midterm 3 Review Sessions Two choices:
Midterm 3 Review Sessions Two choices:

... Computing the structure of the sun We can write equations expressing the following ideas: • The Sun is a gas. • The Sun is neither contracting nor expanding. • Each point inside the Sun stays at a fixed temperature. • How energy generation rate depends on density, temperature, composition. • How en ...
Constellation Information
Constellation Information

... The night skies of winter are famously bright with stars. People often think this is because the air is especially clear at this time of year. Its true dry winter air is more transparent than the humid hazes of summer, but theres a more important reason why we see brighter stars now. They really a ...
Supernovae, Neutron Stars, Black Holes
Supernovae, Neutron Stars, Black Holes

... Triggering the Formation of the Solar System --- New data from meteorites indicates that formation of the Solar System was triggered by a supernova. Written by G. Jeffrey Taylor Hawai'i Institute of Geophysics and Planetology One of the most amazing discoveries in space science is the unambiguous ev ...
Ch. 5 The Universe and Solar System
Ch. 5 The Universe and Solar System

... Our Sun: An Average Star • The Sun is a stable, average size yellow star in the main sequence. • Has a surface temperature of 5500°C. • Largest object in our solar system—a million Earths could fit inside it. • Light takes 8 minutes and 20 seconds to reach the Earth. • Much of what we know about th ...
Simulating Gravitational Attraction Activity
Simulating Gravitational Attraction Activity

The Celestial Sphere - Department of Physics and Astronomy
The Celestial Sphere - Department of Physics and Astronomy

... change relative to each other. Instead, all the motions that we see are due to the rotation of the Earth and the orbit of the Earth around the Sun. ...
For each statement or question, select the word or expression that
For each statement or question, select the word or expression that

... ____ 9. The constellation that contains the "pointer stars" used to locate Polaris is A. Canis Major B. Cassiopeia C. Orion D. Ursa Major ____ 10. An example of a winter constellation is A. Lyra B. Orion C. Cygnus D. Cassiopeia ____ 11. A light-year measures A. time B. distance C. speed D. energy _ ...
Chapter 13
Chapter 13

AST 301 Introduction to Astronomy - University of Texas Astronomy
AST 301 Introduction to Astronomy - University of Texas Astronomy

... The more distant star (Spica) appears fainter. Since it is twice as distant as Canopus, it appears 4 times fainter, or ¼ as bright. We could use the magnitude system to describe how much fainter Spica is than Canopus, but I prefer to talk about fluxes instead of magnitudes. ...
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Hipparcos



Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993. It was the first space experiment devoted to precision astrometry, the accurate measurement of the positions of celestial objects on the sky. This permitted the accurate determination of proper motions and parallaxes of stars, allowing a determination of their distance and tangential velocity. When combined with radial-velocity measurements from spectroscopy, this pinpointed all six quantities needed to determine the motion of stars. The resulting Hipparcos Catalogue, a high-precision catalogue of more than 118,200 stars, was published in 1997. The lower-precision Tycho Catalogue of more than a million stars was published at the same time, while the enhanced Tycho-2 Catalogue of 2.5 million stars was published in 2000. Hipparcos‍ '​ follow-up mission, Gaia, was launched in 2013.The word ""Hipparcos"" is an acronym for High precision parallax collecting satellite and also a reference to the ancient Greek astronomer Hipparchus of Nicaea, who is noted for applications of trigonometry to astronomy and his discovery of the precession of the equinoxes.
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