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Mystic nebula
Mystic nebula

... • Other stars form here • Planets can form inside nebulae ...
Astronomy Final Exam Review
Astronomy Final Exam Review

... • Star- celestial object composed of gas, held together by its own gravity, and supported by nuclear fusion in its core • Galaxy- very large collection of gas, dust, and stars orbiting a common center of mass • Nebula- star nursery • Planetary nebula-remnants of a supernova explosion • Supernova- ...
pdf format
pdf format

... – Center of G.C.s is 26,000 LY = 8000 parsecs from Earth – Center in direction of Sagittarius – (see Links section of class webpage for more on Shapley’s debate with Curtis about the size of the Galaxy, our location in it, and the nature of the “nebulae”.) ...
How is Light Made?
How is Light Made?

... • Two stars with same T, different luminosities – the more luminous star must be larger to emit more light ...
CELT Review: 1,2 May 2002 Session 1
CELT Review: 1,2 May 2002 Session 1

... – Lesson from Keck is that it is difficult to anticipate the most exciting science areas a decade in advance. Major advances in capability have always resulted in unexpected new discoveries. ...
Origins of the Universe
Origins of the Universe

... • When we look into the sky all the stars we can see are red shifted. • The farther a star is from us the more it is red shifted • The only explanation for that is if everything is moving away from us. • This means the universe is expanding ...
4.1 – 4.3 - s3.amazonaws.com
4.1 – 4.3 - s3.amazonaws.com

... • Celestial Clouds • nebulae –large clouds of gas and dust floating in space –They are most common in spiral and irregular galaxies –horse head nebula is one of the most widely known nebulae ...
Lecture 4 - Empyrean Quest Publishers
Lecture 4 - Empyrean Quest Publishers

... Once you find the North Star, Turn around 180 degrees— The Ecliptic and the planets will be in the sky toward the South. ...
Ch. 11 and 12 Study Guide (ANSWERS)
Ch. 11 and 12 Study Guide (ANSWERS)

... 12) Look at the black H-R diagram on pg. 515. Which stars are the brightest according to this diagram? a) White dwarves b) Sun c) Red Giants d) Supergiants 13) Which stars have the hottest temperatures? a) White dwarves b) Sun c) Red Giants ...
Our galaxy is one galaxy among billions of galaxies. Our solar
Our galaxy is one galaxy among billions of galaxies. Our solar

... Our galaxy is one galaxy among billions of galaxies. Our solar system is one star in our galaxy. Keywords Solar System: the sun and the celestial bodies moving around it. Astronomical Unit (AU): the distance between the Earth and the Sun (a measure of distance within the solar system) 1AU = 150,000, ...
Space
Space

... are pushed forwards surround the rocket spread inwards ...
Einstein Postulates for Special Relativity
Einstein Postulates for Special Relativity

... perpendicular to the line extending through D. Classical theory predicts no such effect. ...
Introduction to Astronomy
Introduction to Astronomy

... of the sun’s radius. The central density is 150 times that of water; the central temperature is 15 million kelvin. ...
Light Years Away
Light Years Away

... 5. The Oort cloud is located A. Between the orbit of Mars and Jupiter B. On the outer rim of our solar system C. Within the atmosphere of Neptune D. Within the Andromeda Galaxy ...
Geology Chapter 24 – Studying the Sun
Geology Chapter 24 – Studying the Sun

Em Waves
Em Waves

Astronomy Topics http://www.compadre.org/astronomy/search
Astronomy Topics http://www.compadre.org/astronomy/search

Astronomy Scavenger Hunt Distances 1. What is the
Astronomy Scavenger Hunt Distances 1. What is the

... How many miles is the equivalent of a light year? What is the speed of light? How many light years is the equivalent of a Parsec? What is the distance between the Sun and the next nearest star? What is the distance between the Sun and the star in Orion named Betelgeuse? 9. What is the distance acros ...
glossary - Discovery Education
glossary - Discovery Education

... cosmology — a branch of astronomy concerned with the study of the origin and evolution of the universe. dark matter — matter that cannot be detected with current technology. It is too cold and dark to see or measure; scientists believe it makes up about 90 percent of the universe. fusion — a nuclear ...
The Big Bang
The Big Bang

... 1 solar mass = 2x10 kg ...
View as Printable PDF
View as Printable PDF

... distance from the center of the Sun to the center of the Earth (approximately 149,599,000 kms). A light year is equal to the distance light travels in 1 year (approximately 9.5 trillion kms). It is used for longer distances – to stars and galaxies. The distance to our nearest star, Proxima Centauri ...
No Slide Title
No Slide Title

... Once thought to foretell doom and destruction its next visit doesn’t happen until 2061 and sadly, Edmund won’t be around to see it ...
Sample Exam for Final (with correct answers)
Sample Exam for Final (with correct answers)

... (a) Clusters of galaxies are all moving away from each other. ∗ (b) Clusters of galaxies are all moving closer together. (c) New matter is always coming into existence between clusters of galaxies. (d) The laws of physics were much different in the remote past. (e) The primary properties of the univ ...
Main Sequence Stars
Main Sequence Stars

... They plotted the locations of stars on a graph with the horizontal coordinate being spectral type (equivalent to temperature) and the vertical coordinate being absolute magnitude (equivalent to luminosity). The result, called the Hertzsprung-Russell diagram, or H-R diagram, is widely used in modern ...
Photon
Photon

... observations of solar-type stars in open clusters allow us to establish a stellar chronometer, and create an age-ranking system for an ensemble of nearby, well-studied clusters. With the aid of new observations of Blanco 1, an high-Galactic latitude, Pleiades-age cluster, I will show how deriving st ...
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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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