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Unit 3 - Section 9.1 2011 Distances in Space0
Unit 3 - Section 9.1 2011 Distances in Space0

... It makes intuitive sense that the farther a star is from Earth, the longer it takes light from the star to reach Earth. The star Polaris is 400 ly from Earth. In other words, it takes light from Polaris 400 years to reach Earth. The light that we see when we look at Polaris is 400 years old. We are ...
Universe ppt - Killeen ISD
Universe ppt - Killeen ISD

... An artist's rendering shows a neutron star—located 50,000 light-years from Earth—that flared up so brightly in December 2004 that it temporarily blinded all the x-ray satellites in space and lit up the Earth's upper atmosphere. The flare-up occurred when the star's massive, twisting magnetic field r ...
NASC 1100
NASC 1100

... the star’s radius, making its surface hotter. In the H-R diagram, the star goes down and to the left. All low-mass stars fuse helium into carbon at nearly the same rate  they have almost the same luminosity, but differ in temperature. ...
Neutron Stars - Otterbein University
Neutron Stars - Otterbein University

... through the star and blows off the outer layers, including the heavy elements – a supernova • A million times brighter than a nova!! • The actual explosion takes less than a second ...
Spectrum Analysis Activity File
Spectrum Analysis Activity File

... Name: ______________________________________ Date: _________________ Period: ________ Table #_________ ...
A Star is Born worksheet and key
A Star is Born worksheet and key

... size. Sun-like stars have a mass up to 1.5 times the size of the Sun. Huge stars have a mass from 1.5-3 times of the Sun. Giant stars have a mass over 3 times of the Sun. 3. List the lifecycle of a Giant star. Giant: Red Supergiant  Supernova  Black Hole 4. If a star is blue, what does that reveal ...
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...  Each element has its own unique pattern of spectral lines. ...
HEIC0410: FOR RELEASE 15:00 (CEST)/9:00 AM EDT 15 June
HEIC0410: FOR RELEASE 15:00 (CEST)/9:00 AM EDT 15 June

... Both components of the binary system belong to the L spectral class that includes the lowest mass stars and the highest mass brown dwarfs in our solar neighbourhood. This spectral class was discovered in 1997 and was added to the spectral classification that had remained unchanged for half a century ...
mass_spetral
mass_spetral

... When the stars are farther apart (a is increased) they move more slowly in their orbit. Measuring the time it takes for the spectral lines to return to their starting wavelength gives us the orbital ...
Three types of binary stars.
Three types of binary stars.

... When the stars are farther apart (a is increased) they move more slowly in their orbit. Measuring the time it takes for the spectral lines to return to their starting wavelength gives us the orbital period ...
15 - Edmodo
15 - Edmodo

... Using pages 300-301 in your Investigating Science 9 textbook, draw a labeled Hertzsprung diagram below: (7 Marks) ...
~Crowfoot
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... 4)2 The stars in this “Jewel Box” of the southern hemisphere are a) young stars still in their nursery “open cluster.” b) not physically associated, but aligned along our line of sight. c) in the nearest globular cluster to Earth. 5)2 This world is Io a) 10 AU from the sun b) Io, one of the Galilean ...
Small Planets of our Solar System (Pluto is a Dwarf Planet)
Small Planets of our Solar System (Pluto is a Dwarf Planet)

... ...
Stars, Stellar classification, H
Stars, Stellar classification, H

... These two stars have about the same luminosity -which one appears brighter? A. Alpha Centauri B. The Sun ...
Astronomy Study Guide
Astronomy Study Guide

...  Only one with large amounts of liquid water & oxygen: Earth  Tilted on its side so one side gets constant day & the other constant night: Uranus  Density is so low it would float in water: Saturn  Has a huge hurricane large enough to fit Earth inside: Jupiter • Comets tails always point away fr ...
Stars - HMXEarthScience
Stars - HMXEarthScience

... 1. Large clouds of dust and gas are pulled together by gravity (these clouds are called nebulae) 2. Gases in the nebula contract due to gravity, resulting in the formation of a protostar. 3. Pressure and temperature increase until the gases “ignite” and nuclear fusion begins 4. Once the star has ful ...
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... A. Become white dwarf B. Explode as a supernova C. Become a protostar ...
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... full size, but some observations suggest it could have a diameter 3000 times larger than that of the Sun. ...
For instance, two hydrogen atoms may fuse together to form one
For instance, two hydrogen atoms may fuse together to form one

... Astronomers classify stars based on their age, color, and brightness. These characteris tics help them identify and understand the different kinds of stars. A star’s surface temperature determines the amount of visible light given off (its brightness) and the color we perceive the star to be. For ex ...
Superwind - The University of Sydney
Superwind - The University of Sydney

... Astronomers at The University of Manchester believe they have found the answer to the mystery of a powerful ‘superwind’ which causes the death of stars. Writing in Nature, the team of researchers, lead by Barnaby Norris from the University of Sydney in Australia, used new techniques which allowed th ...
AstroProjectDay4b
AstroProjectDay4b

... STAR, AND MUCH SMALLER THAN MANY OTHER STARS ...
What is the difference between geocentric and heliocentric theories?
What is the difference between geocentric and heliocentric theories?

... • Contain very little gas or dust. • Because of little gas, no new stars are forming. • The largest and smallest galaxies are elliptical galaxies. ...
Chapter-08
Chapter-08

... Suppose that a certain star has no planets or other “debris” orbiting it. Does the star create a gravitational field around it? 1. Yes 2. No 3. Yes, but it’s a field of dreams. ...
The Family of Stars
The Family of Stars

... parallax, nearby stars also show continuous motions across the sky. ...
8 clusters stellar evo
8 clusters stellar evo

... horizontal axis ...
< 1 ... 351 352 353 354 355 356 357 358 359 ... 433 >

Corvus (constellation)



Corvus is a small constellation in the Southern Celestial Hemisphere. Its name comes from the Latin word ""raven"" or ""crow"". It includes only 11 stars with brighter than 4.02 magnitudes. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi from a distinctive quadrilateral in the night sky. The young star Eta Corvi has been found to have two debris disks.
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