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Astronomy and the Great Pyramid
Astronomy and the Great Pyramid

Lecture 1 - University of Maryland Astronomy
Lecture 1 - University of Maryland Astronomy

Star Track 2 - The Search for a Supermassive Black... Early radio astronomers detected an immensely
Star Track 2 - The Search for a Supermassive Black... Early radio astronomers detected an immensely

... Early radio astronomers detected an immensely powerful source of radio waves towards the center of the Galaxy in the constellation Sagittarius; this mysterious object was designated SgrA*. More recently, infrared astronomers using adaptive optics have imaged individual stars near this object and tra ...
Project 2. CCD Photometry
Project 2. CCD Photometry

... In 120 B.C. Hipparcus classified the naked‐eye stars according to their brightness into  six categories or magnitudes. The brightest stars were assigned to category one (first  magnitude) and the faintest stars to category six (sixth magnitude), which is the limit  of  human  visual  perception  (wi ...
Standard EPS Shell Presentation
Standard EPS Shell Presentation

... Identify the conditions necessary for fusion to occur inside a star. Describe the information that spectroscopy provides about stars. Relate the color of a star to its temperature. Explain the factors that determine the brightness of a star in the sky. Discuss the importance of the H-R diagram to as ...
Low Mass
Low Mass

The Sky and its Motions
The Sky and its Motions

... Close to where it is now. ...
Study Guide for the Comprehensive Final Exam
Study Guide for the Comprehensive Final Exam

... State the impact of convection in the envelope of very low mass stars on the stars main sequence lifetime. Describe or identify changes in a star during its main sequence lifetime. Describe how shell fusion in a star causes the star to become giants. Identify the “ashes” of H-burning and He-burning ...
12-1 MAIN-SEQUENCE STARS
12-1 MAIN-SEQUENCE STARS

Extra-Solar Planets
Extra-Solar Planets

... 1) Old enough to allow time for evolution (rules out high-mass stars - 1%) 2) Need to have stable orbits (might rule out binary/multiple star systems - 50%) 3) Size of “habitable zone”: region in which a planet of the right size could have liquid water on its surface. Even so… billions of stars in t ...
Stellar Evolution II
Stellar Evolution II

... before collapsing to form stars – very massive stars are rare • Stars with masses above 50 MSUN are unstable – nuclear reactions in their core produce energy at such a fast rate that they blow off their outer layers, losing mass. ...
Astronomy 103 Announcements
Astronomy 103 Announcements

... Now refers to an area of the sky rather than collection of stars Sky is divided into 88 constellations ...
30.2 PowerPoint Stellar Evolution
30.2 PowerPoint Stellar Evolution

... the core of the star  The energy from fusion balances the force of gravity and makes it a very stable stage ...
Physics-Y11-LP3 - All Saints` Catholic High School
Physics-Y11-LP3 - All Saints` Catholic High School

Contents ISP 205 Section 2 Study Guide for Test 3 28 March 2007
Contents ISP 205 Section 2 Study Guide for Test 3 28 March 2007

... 8. Suppose star A and star B are both main sequence stars of the same temperature. Star A is 100 times fainter than star B. Compare the stars’ luminosities and distances. Luminosities are same, since temperature is same. For star A to be fainter, it is 10 times as far as B. Flux=L/D2 9. On a HR diag ...
Magnitudes lesson plan
Magnitudes lesson plan

... that he could see from his latitude into six classes of brightness. His idea of six classes probably came from the Babylonians whose base number was six. The formal introduction of six magnitudes has been credited to Ptolemy (100-150 A.D.) who was a Greek/Egyptian astronomer. He simply advanced the ...
AST301.Ch21.StellarExpl - University of Texas Astronomy
AST301.Ch21.StellarExpl - University of Texas Astronomy

Signs of the Zodiac, Cancer
Signs of the Zodiac, Cancer

... So that, if Cancer one such crystal had, Winter would have a month of one sole day.” Cancer lies between Gemini to the west and Leo to the east, Lynx to the north and Canis Minor and Hydra to the south. Best known among stargazers as the home of Praesepe - Latin for manger - (Messier 44), an open cl ...
Survey of the Solar System - USU Department of Physics
Survey of the Solar System - USU Department of Physics

... • At most, 1 in 3 Sun-like stars harbor a planetary system • At least, 1 in 14 Sun-like stars have one • According to this study ...
The Sun and the Stars
The Sun and the Stars

The H-R Diagram
The H-R Diagram

... you end up doing when you look at the night sky – you see everything above some limiting brightness accessible to your eye or telescope. This is a very Unfair sample! • It’s heavily skewed toward the most luminous stars, which you can see from much farther away and hence sampling a much bigger volum ...
A Star is “Born,” and then How Will it Move
A Star is “Born,” and then How Will it Move

... Young (Embedded) Clusters: Very young (<10 Myr-old) groups of young stars that form together. Future binding depends on cluster mass & velocity, seems that 90% dissolve before ~10 Myr (Lada & Lada 2003). When they unbind but are still seen to move together, they’re known as a “stellar association.” ...
Lecture 3
Lecture 3

... Earth-Sun distance. Transits occur when the planet passes between the Earth and Sun. NB. Transits of Venus are rare, because the orbit of Venus is inclined to the ecliptic (the plane of the Earth’s orbit) by 3.394 degrees. As Venus passes between Earth and Sun, Venus occults (blocks) the light from ...
WORD - hrsbstaff.ednet.ns.ca
WORD - hrsbstaff.ednet.ns.ca

... 12. An imaginary sphere of infinite extent with Earth at its center on which the stars, planets, and other heavenly bodies appear to be located is known as the a. Zodiac. b. celestial sphere. c. atmosphere. d. Valhalla. 13. Which one of the following statements is true about the celestial coordinat ...
STARS
STARS

... STARS Init 2/20/2008 by Daniel R. Barnes ...
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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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