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Life Cycles of Stars
Life Cycles of Stars

Unit 8 Chapter 30
Unit 8 Chapter 30

Stellar Evolution - Harnett County High Schools Wiki
Stellar Evolution - Harnett County High Schools Wiki

... radiation that from Earth appears to blink on and off as the star spins, like the beam of light from a turning lighthouse. This "pulsing" appearance gives some neutron stars the name pulsars. ...
Packet 3
Packet 3

... 7. Stars that are closer than 32.6 light-years away appear __________________________. Therefore those stars that are further than 32.6 light-years away appear ________________________. 8. How far away a star would be if it’s apparent magnitude and absolute magnitude were equal? _________ Match the ...
constellations
constellations

... Starting from due south, the average time taken for the Sun to appear to travel right around the sky and return to exactly due south is 24 hours. This is the Mean Solar Day. Starting from due south, the time taken for a star to appear to travel right around the sky and return to exactly due south is ...
luminosity1
luminosity1

... • Spectral typing can be used to find the surface temperature of a star. (Along with color and Wien’s Law) • Spectral typing can also be used to find out how much of a given element is in a star. • HD 161817 has much less of all the elements, other than Hydrogen and Helium, than the Sun. • In fact, ...
A little bit more to do. Stefan
A little bit more to do. Stefan

... • Spectral typing can be used to find the surface temperature of a star. (Along with color and Wien’s Law) • Spectral typing can also be used to find out how much of a given element is in a star. • HD 161817 has much less of all the elements, other than Hydrogen and Helium, than the Sun. • In fact, ...
Measuring the distance to Galaxies
Measuring the distance to Galaxies

Document
Document

about Stars
about Stars

... • Astronomers quantify the “color” of a star by using the difference in brightness between the brightness in the B and V spectral regions • The B-V color is related to the slope of the ...
PPT file
PPT file

... Similar to our sun (stays like this for most of their life) These burn H fuel faster than low mass stars and last only about 10 billion years ...
Lecture11
Lecture11

Slide 1
Slide 1

Big Bang and Life Cycle of Stars
Big Bang and Life Cycle of Stars

... Then what? The universe expanded very quickly - After a few thousand years, some cooling occurred, which allowed for the formation of atoms – - first Hydrogen and Helium, but it had to cool still more for the other elements to start to form and be neutral atoms -Anti-matter also formed, composed of ...
5. cosmic distance ladder ii: standard candles
5. cosmic distance ladder ii: standard candles

... easily calculated. However, some special types of variable and exploding stars do have known, standard luminosities. Consequently, if you can identify a star as being one of these special types, you know its luminosity. Then you only have to measure its brightness to be able to compute its distance. ...
Learning Objectives
Learning Objectives

... easily calculated. However, some special types of variable and exploding stars do have known, standard luminosities. Consequently, if you can identify a star as being one of these special types, you know its luminosity. Then you only have to measure its brightness to be able to compute its distance. ...
Exercise 4
Exercise 4

... (b) C > D > E > A > B (Largest m to smallest m, i.e. dimmest to brightest, i.e. least luminous to most luminous since the objects are at the same distance from the Earth) (c) B > A > E > D > C (Using m–M = 5 log d/10, the largest m-M corresponds the farthest star) ...
te acher`s guide te acher`s guide
te acher`s guide te acher`s guide

... Stars asks the following five questions about our Sun and all of its shining counterparts. Space travelers Adi and Woops help viewers clearly answer each question using computer graphics and space footage. What are the signs of the zodiac? The signs of the zodiac are twelve different groups of stars ...
The Temperature of Stars
The Temperature of Stars

... Many stars also have about the same mass as the sun, however some stars may be more or less massive. ...
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 ...
Eyeing the retina nebula
Eyeing the retina nebula

... the outer layers are ejected to form an expanding cloud of dust and gas. Intense radiation from the collapsed star ionizes the surrounding gases, producing the glowing colors. IC4406, nicknamed the Retina Nebula, is one of the closest planetary nebulae to Earth. The Hubble Space Telescope image prov ...
Slide 1
Slide 1

Astronomy 103 – Midterm 2 – October 29, 2014
Astronomy 103 – Midterm 2 – October 29, 2014

... 20. Which of the following lists gives the spectral types of stars in order from the type corresponding to stars with the hottest surfaces to the type corresponding to stars with the coolest surfaces? a) F, B, G, O, M b) A, B, F, G, O c) O, B, F, G, M d) K, M, F, G, B e) B, G, F, M, K ...
Distant Stars Lesson Plan
Distant Stars Lesson Plan

... III ...
Phys133 Sample MidTerm #2 Covers Chs.10
Phys133 Sample MidTerm #2 Covers Chs.10

... 4) What happens when a star exhausts its core hydrogen supply? A) It contracts, becoming hotter and brighter. B) Its core contracts, but its outer layers expand and the star becomes bigger but cooler and therefore remains at the same brightness. C) It expands, becoming bigger but dimmer. D) It contr ...
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Corona Australis



Corona Australis /kɵˈroʊnə ɒˈstreɪlɨs/ or Corona Austrina /kɵˈroʊnə ɒˈstraɪnə/ is a constellation in the Southern Celestial Hemisphere. Its Latin name means ""southern crown"", and it is the southern counterpart of Corona Borealis, the northern crown. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The Ancient Greeks saw Corona Australis as a wreath rather than a crown and associated it with Sagittarius or Centaurus. Other cultures have likened the pattern to a turtle, ostrich nest, a tent, or even a hut belonging to a rock hyrax.Although fainter than its namesake, the oval- or horseshoe-shaped pattern of its brighter stars renders it distinctive. Alpha and Beta Coronae Australis are the two brightest stars with an apparent magnitude of around 4.1. Epsilon Coronae Australis is the brightest example of a W Ursae Majoris variable in the southern sky. Lying alongside the Milky Way, Corona Australis contains one of the closest star-forming regions to our Solar System—a dusty dark nebula known as the Corona Australis Molecular Cloud, lying about 430 light years away. Within it are stars at the earliest stages of their lifespan. The variable stars R and TY Coronae Australis light up parts of the nebula, which varies in brightness accordingly.
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