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luminosities
luminosities

... your study of the billions of stars that dot the sky. In a sense, the star is the basic building block of the universe. If you hope to understand what the universe is and how it works, you must understand the stars. ...
DO NOW - PBworks
DO NOW - PBworks

Week 10
Week 10

Nov 2017 - What`s Out Tonight?
Nov 2017 - What`s Out Tonight?

Types of Galaxies - Spring Branch ISD
Types of Galaxies - Spring Branch ISD

... b. The star’s distance from Earth 38. The Hertzsprung-Russell diagram shows the relationship between surface temperature and brightness 39. Look at the Hertzsprung-Russell diagram in Figure 11 on page 289. Write what is measured on each of the two axes of the diagram. a. x-axis (horizontal axis): Su ...
Astronomy Study Guide
Astronomy Study Guide

... b. The star’s distance from Earth 38. The Hertzsprung-Russell diagram shows the relationship between surface temperature and brightness 39. Look at the Hertzsprung-Russell diagram in Figure 11 on page 289. Write what is measured on each of the two axes of the diagram. a. x-axis (horizontal axis): Su ...
Rogava_Course_-_First_lecture
Rogava_Course_-_First_lecture

... • Mizar A was the very first spectroscopic binary: in 1889 Edward PIckering found that it is a binary star.This binary is 35 times brigter than the Sun. • Orbital period ~20 days. • There exist double-lined (SB2) and single-lined (SB1) spectroscopic binaries. • Famous SB1 - Cygnus X-1 System. ...
Lecture notes -- pdf file - University of Iowa Astrophysics
Lecture notes -- pdf file - University of Iowa Astrophysics

... • If the distance between the Earth and Sun were shrunk to 1 cm (0.4 inches), Alpha Centauri would be 2.75 km (1.7 miles) away ...
Lecture17
Lecture17

08 September: How far away are the closest stars?
08 September: How far away are the closest stars?

Last time: Star Clusters (sec. 19.6)
Last time: Star Clusters (sec. 19.6)

... accumulates in core (can’t burn the He as fuel—would require higher temperatures), H-burning only occurs in outer core. Contraction of He core. He nuclei can’t fuse, so there is a pressure deficit compared to gravity, so core contracts, heating up (just like for a protostar). But the overlying layer ...
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Stars

Lecture 9: Stellar Spectra
Lecture 9: Stellar Spectra

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Chapter11

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July - astra

Introduction to the HR Diagram
Introduction to the HR Diagram

... Important features of the HR diagram:  The Y-axis is the total energy output of the star, called the Luminosity. The luminosity of stars is measured in units of the luminosity of the Sun or one solar luminosity. Thus a star that has a luminosity of 10 solar luminosities outputs 10 times more energ ...
Unit 4: Astronomy
Unit 4: Astronomy

... 4) Describe the evolution of a “low-mass” star (a star that has the same mass as our sun or smaller) once it leaves the main-sequence. {your answer should include descriptions of giants and white dwarfs} 5) Describe the evolution of a “massive” star once it leaves the main-sequence. {your answer sho ...
Slide 1 - Personal.psu.edu
Slide 1 - Personal.psu.edu

planetary nebulae
planetary nebulae

... • 3+ solar masses and there is no force greater than the star’s gravity. • The star collapse never stops, it disappears leaving only it’s mass to create a gravity field. • Nothing goes fast enough to escape, not even light. This is a black hole. ...
Phys 100 – Astronomy (Dr. Ilias Fernini) Review Questions for
Phys 100 – Astronomy (Dr. Ilias Fernini) Review Questions for

... 10. The binary star, Mizar A, is shown with the motion of the members around one another. The mass of a visual binary pair of stars can be obtained from a. the time in years for them to orbit one another. b. the size of their orbit. c. their location in space. * d. both a and b 11. We know the white ...
What are the Spectral Lines? - University of Texas Astronomy Home
What are the Spectral Lines? - University of Texas Astronomy Home

... • Bessel: 61 Cygni - 1/3 arcsec 10.3 Lightyears • almost simultaneously: - Wilhelm Struve: Vega - Thomas Henderson: Alpha Centauri ...
Major Stars of the Orion Constellation
Major Stars of the Orion Constellation

... We start our comparison of major Orion stars by describing Alpha Orionis, Betelgeuse, which forms Orion’s right shoulder. It’s actually fainter than Beta Orionis (Rigel) due to a misclassification error as Betelgeuse was found to be a variable star. [Wiscweb] “Astronomers now know that these regula ...
Document
Document

Neutron Star - Perry Local Schools
Neutron Star - Perry Local Schools

... of 1.4 to 3 solar masses, the remnant can become a neutron star. – If the leftover core has a mass that is greater than three solar masses, it will collapse to form a black ...
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Corona Borealis

Corona Borealis /kɵˈroʊnə bɒriˈælɨs/ is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means ""northern crown"". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from our Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.
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