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1 - Quia
1 - Quia

... B. Carbon C. Hydrogen D. Nitrogen 16. What is the first stage in the life cycle of a star? (2 points) ...
Astronomy Part 2 - Malvern Troop 7
Astronomy Part 2 - Malvern Troop 7

... a) List the names of the five most visible planets. Explain which ones can appear in phases similar to lunar phases and which ones cannot, and explain why. b) Find out when each of the five most visible planets that you identified in requirement 5a will be observable in the evening sky during the ne ...
Binary Stars - Mid-Pacific Institute
Binary Stars - Mid-Pacific Institute

observingopenclusters-2-2-1
observingopenclusters-2-2-1

... to the Sun Slide your scope or binoculars parallel to the dog’s back and then move west of that line. You will pick up a large rich field of stars – Open Cluster M41 Procyon (Canis Minor) Locate next large and (also close) Procyon This points the way to 2 very different open clusters in Monocerous, ...
EX - Uplift North Hills Prep
EX - Uplift North Hills Prep

... (ii) Modern techniques enable the measurement from Earth’s surface of stellar parallax angles as small as 5.0 × 10–3 arcsecond. Calculate the maximum distance that can be measured using the method of stellar parallax. ...
ppt - UCL
ppt - UCL

Directed Reading A
Directed Reading A

White Dwarfs - Indiana University
White Dwarfs - Indiana University

Stars
Stars

Name _________ Date _____________ Period ______ Skills
Name _________ Date _____________ Period ______ Skills

... COMPOSITION OF STARS _____ 5. The band of colors produced when white light passes through a prism is a(n) a. color wheel. b. emission line. c. ultraviolet light. d. spectrum. _____ 6. A hot, solid object gives off a(n) a. continuous spectrum. b. absorption spectrum. c. emission line. d. partial spec ...
Star Maps and Constellations (pdf 3.7 Megs)
Star Maps and Constellations (pdf 3.7 Megs)

Stars…Giants, Supergiants, Dwarfs….
Stars…Giants, Supergiants, Dwarfs….

Date_________________ TWINKLE, TWINKLE
Date_________________ TWINKLE, TWINKLE

Solutions3
Solutions3

Masers and high mass star formation Claire Chandler
Masers and high mass star formation Claire Chandler

... If you know flux density, dust temperature, distance to source, and opacity characteristics of dust, you can get Md. Assume dust to gas ratio and you get total mass of object. ...
Astro 10 Practice Test 2
Astro 10 Practice Test 2

... d. Mostly iron, similar to the hot iron core of the Earth, with a little bit of helium and some heavier elements. 17. On a clear autumn night, you spend some time examining the glowing HII regions in the galaxy M33, using a large reflecting telescope. If you were IN the galaxy M33, looking at these ...
What is a Scientist? - Cockeysville Middle School
What is a Scientist? - Cockeysville Middle School

... Stars are giant spheres of glowing gases. A star is powered by nuclear fusion. This is a process whereby hydrogen atoms are fused together to create helium atoms. In the process a tremendous amount of energy is given off in the form of electromagnetic waves and heat. There are billions of stars in a ...
Ages of Star Clusters - Indiana University Astronomy
Ages of Star Clusters - Indiana University Astronomy

... sequence sooner. In a cluster in which all the stars formed at the same time, the stars “peel off” the main sequence from the top, leaving only progressively less and less massive stars remaining on the main sequence as time goes by. The main sequence turnoff is the point on the main sequence for wh ...
ppt document
ppt document

Document
Document

A-36_SF
A-36_SF

... • We learn about star formation by studying groups of stars – Color indicates age: hot, massive, blue stars die quickly – …but not before they blow away the cloud they were born from – Galactic rotation disperses clustered stars ...
Star Basics
Star Basics

... helium. At these temperatures most of the hydrogen is ionized, so the hydrogen lines are weak. Both HeI and HeII (singly ionized helium) are seen in the higher temperature examples. The radiation from O5 stars is so intense that it can ionize hydrogen over a volume of space 1000 light years across. ...
The magnitude scale
The magnitude scale

... times fainter again, i.e. 10,000 times fainter than one at the naked eye limit, and so on. ...
The Birth of Stars Guiding Questions • Because stars shine by
The Birth of Stars Guiding Questions • Because stars shine by

... 1. Why do astronomers think that stars evolve (bad use of term – this is about the birth, life and death of stars and that is NOT evolution)? 2. What kind of matter exists in the spaces between the stars? 3. In what kind of nebulae do new stars form? 4. What steps are involved in forming a star like ...
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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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