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THE HR DIAGRAM
THE HR DIAGRAM

Chapter1&2Review
Chapter1&2Review

... 1. From what you know about astronomical units and light-years, how would you define a light-minute? 2. From what you know about astronomical units and light-years, how would you define a light-minute? 3. Describe the path that a star on the celestial equator follows from the time it rises until it ...
Chapter 21
Chapter 21

... The sun is a medium-sized star. Stars that are much larger than the sun are called ______________ or __________________.  Composition – The chemical composition of most stars is about 73 % ______________ and 25 % ____________________. How can astronomers infer which elements are found in stars? ___ ...
HR Diagram - Geneva 304
HR Diagram - Geneva 304

Stars: the Hertzsprung
Stars: the Hertzsprung

... star with a given mass and chemical composition – if we start with a just formed protostar of a given mass and chemical composition, we can calculate how that star will evolve over its entire life. • This is extremely useful because it greatly simplifies the study of stars and is the basic reason wh ...
Table Number: _____
Table Number: _____

CONSTELLATIONS
CONSTELLATIONS

... These are numbered East (i.e. to the left) to West (Sun rises in East and sets in West). ...
changing constellations
changing constellations

The Danger of Deadly Cosmic Explosions
The Danger of Deadly Cosmic Explosions

... radiation • Penetrates underground and underseas. • Equivalent to 1 kiloton TNT / km2 over earth surface • Kills everything exposed. • Destroys atmosphere, brings on nuclear winter. ...
I : Internal structure of main sequence stars
I : Internal structure of main sequence stars

... A star leaves the main sequence once it exhausts its supply of hydrogen in the core ...
PowerPoint Presentation - ASTR498E High energy
PowerPoint Presentation - ASTR498E High energy

... A star leaves the main sequence once it exhausts its supply of hydrogen in the core ...
9ol.ASTRONOMY 1         ... Identify Terms -  Matching (20 @ 1 point each =...
9ol.ASTRONOMY 1 ... Identify Terms - Matching (20 @ 1 point each =...

... 28. .Radioactive dating techniques have revealed that our Earth and Moon are approximately how old? 29. According to our theory of solar system formation, what three major changes occurred in the solar nebula as it shrank in size? 30. According to our present theory of solar system formation, why w ...
May 2013 - Joliet Junior College
May 2013 - Joliet Junior College

15.4 Star Systems and Galaxies
15.4 Star Systems and Galaxies

... I. Star Systems and Planets A. Star system-groups of two or more stars 1. Binary stars - two stars or double stars a. Eclipsing binary-a system in which one star blocks the light from another II. Planets Around Other Stars A. Astronomers study gravitational effects on stars to see if there is a pla ...
Space Science Unit
Space Science Unit

... • The stars are plotted on the diagram according to their surface temperature and absolute magnitude. • Once the stars are placed on the diagram, astronomers have noticed clustering of the plotted stars. • These clusters are grouped together into the various stages of a stars life cycle. • Let’s loo ...
Earth - Capital High School
Earth - Capital High School

... The Hubble Ultra Deep Field, or HUDF, is an image of a small region of space in the constellation Fornax, composited from Hubble Space Telescope data accumulated over a period from September 3, 2003 through January 16, 2004. It is the deepest image of the universe ever taken in visible light, lookin ...
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... is based on the Doppler shift in the star's light as the star moves towards or away from us. ...
Chapter 1 Vocabulary – The Puzzled of Matter
Chapter 1 Vocabulary – The Puzzled of Matter

THE BIRTH AND DEATH OF A LOW/MEDIUM MASS STAR
THE BIRTH AND DEATH OF A LOW/MEDIUM MASS STAR

... • THE STAGE WHEN A STAR IS IN IT’S “BEST” LIFE CYCLE • OUR SUN IS A MAIN SEQUENCE STAR • MAIN SEQUENCE STARS HAVE MOSTLY HYDROGEN. • THE HYDROGEN EXPLODES, GIVING OFF LIGHT AND HEAT • AS IT EXPLODES, THE HYDROGEN TURNS TO HELIUM. • HELIUM IS LIGHTER THAN HYDROGEN. • OUR SUN IS 4.6 BILLION YEARS OLD. ...


... 1. A beam of light shining through a dense molecular cloud is diminished in intensity by a factor of: 2 for every: 5 pc it travels. By how many magnitudes is the light from a background star dimmed if the total thickness of the cloud is: 60 pc? ...
Homework #2
Homework #2

11.1 Stars - St John Brebeuf
11.1 Stars - St John Brebeuf

... Large high mass stars often explode as supernovas, spreading elements throughout the universe. ...
coSmoS in youR PockET
coSmoS in youR PockET

Friday, November 7 - Otterbein University
Friday, November 7 - Otterbein University

... • Some have names that go back to ancient times (e.g. Castor and Pollux, Greek mythology) • Some were named by Arab astronomers (e.g. Aldebaran, Algol, etc.) • Since the 17th century we use a scheme that lists stars by constellation – in order of their apparent brightness – labeled alphabetically in ...
Section 25.2 Stellar Evolution
Section 25.2 Stellar Evolution

...  Stars with masses similar to the sun evolve in essentially the same way as lowmass stars.  During their collapse from red giants to white dwarfs, medium-mass stars are thought to cast off their bloated outer layer, creating an expanding round cloud of gas called planetary nebula. ...
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Ursa Minor



Ursa Minor (Latin: ""Smaller She-Bear"", contrasting with Ursa Major), also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the name Little Dipper. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor has traditionally been important for navigation, particularly by mariners, due to Polaris being the North Star.Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging from apparent magnitude 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and magnitude 3 Gamma Ursae Minoris have been called the ""guardians of the pole star"". Planets have been detected orbiting four of the stars, including Kochab. The constellation also contains an isolated neutron star—Calvera—and H1504+65, the hottest white dwarf yet discovered with a surface temperature of 200,000 K.
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