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... measure the speed of light. His attempt involved two observers positioned in two towers that were about 10km apart. The idea was that the first observer opens a shutter in a lantern and then as soon as the second observer sees the light from the first lantern, opens his shutter. Galileo would then m ...
B. protostar - University of Maryland Astronomy
B. protostar - University of Maryland Astronomy

... 24. Which of the following changes occurs immediately after the development of a hydrogen burning shell inside a star like the Sun? A. The star collapses to a neutron star and then it blows up. B. The star ejects a planetary nebula and new planets form. C. The star emits strongly in the infrared and ...
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Sun - TeacherWeb

... Super-giant stars such as Polaris end their lives in supernova explosions. Small to medium stars like the Sun end their lives as white dwarfs. ...
Name - MIT
Name - MIT

... are white dwarfs that have finally ceased all nuclear reactions. are white dwarfs that have cooled and no longer produce visible light. are the end products of stars like the sun. are a name given to matter so compressed that even light can't escape. ...
Neutron Stars - Otterbein University
Neutron Stars - Otterbein University

... through the star and blows off the outer layers, including the heavy elements – a supernova • A million times brighter than a nova!! • The actual explosion takes less than a second ...
PH507 - University of Kent
PH507 - University of Kent

... Depending on their initial masses and the rate of mass loss, they may explode as yellow hypergiants or luminous blue variables, or they may become Wolf-Rayet stars before exploding in a core collapse supernova. Identifying whether Deneb is currently evolving towards a red supergiant or is currently ...
Online STUDY QUESTIONS #8 — ANSWERS 1. Mercury moves
Online STUDY QUESTIONS #8 — ANSWERS 1. Mercury moves

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16. Properties of Stars

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Signs of the Zodiac, Cancer
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epsilon Aur
epsilon Aur

... Epsilon Aurigae is not the brightest eclipsing binary, nor is it the one with the deepest eclipses. What makes it distinctive is its long period of over 27 years, coupled with the mystery surrounding the nature of the secondary object in the system. The last primary eclipse took place during 1982-84 ...
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mam.evolution

... period P and separation a that obeys Kepler’s 3rd Law must have a total mass of 1 solar mass. c) Since we also know MA/MB = rA/rB, we can solve for masses. ...
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Astronomy Power Point

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jodrell_bank_wms - Faulkes Telescope Project

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astr100_finalexam

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The Milky Way - 清華大學物理系歡迎頁 Welcome to
The Milky Way - 清華大學物理系歡迎頁 Welcome to

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Jupiter-Sized Star Smallest Ever Detected
Jupiter-Sized Star Smallest Ever Detected

... At this moment, exact values of the radii are known The astronomers find that OGLE-TR-122b weighs only for four stars with masses less than one-third one-eleventh of the mass of the Sun and has a of the mass of the Sun and none at all for masses diameter that is only one-eighth of the solar one. bel ...
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2007-8 Astronomy Outline

... coming in from other houses aka light pollution) Location: where you are and the direction you are facing Observation: (verbally describe what you see with the naked eye; make sketch(s)) *first night sky journal will be due on __Friday, August 19th__* Chapter 1 I. Astronomy  Study of the universe  ...
1st EXAM VERSION C - Department of Physics and Astronomy
1st EXAM VERSION C - Department of Physics and Astronomy

... charged particles from the sun accelerated/guided by magnetic field lines C. richer in heavier elements than other mass ejections D. nothing to be feared by spacecraft and humans in space E. never going to achieve escape velocity 24. An eclipsing binary system is A. two stars whose spectral lines mo ...
Stellar Evolution (Powerpoint) 17
Stellar Evolution (Powerpoint) 17

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HR Diagram
HR Diagram

... It has been shown through observational data of many stars that the more massive a star, the more luminous it is. If you observe the H-R diagram on the cover of the lab, it is clear that there are fewer luminous stars as compared to the less luminous ones. In terms of the diagram, there are more sta ...
Reach for the Stars B
Reach for the Stars B

... 79. Parallax depends on measuring angles on the sky. How much smaller is the parallax angle for an object 400 light years away, as compared to one that is 100 light years away? 80. How many times brighter/dimmer would the Sun appear from a colony on Mars (which orbits at 1.5 AU) than it does from Ea ...
celestial equator
celestial equator

... The brightest stars were called stars of the first magnitude. Fainter stars were classified as being of second, third, fourth, or fifth magnitude. Now stars can be measured to +/- 0.01 magnitude. We have also expanded the scale to include negative values, and much larger positive values. Sirius, fo ...
The Solar System
The Solar System

... – supernova remnants, expanding at 10,000 km/s – may trigger future star formation? – Neutron stars: mass star but just 10 km across. • Teaspoon weighs 100 million tons! • Seen as Pulsars, flashing beacons in space. ...
1) The following questions refer to the HR diagram
1) The following questions refer to the HR diagram

... A) it amplifies the contrast with red giants. B) they are both very hot and very small. C) they are supported by electron degeneracy pressure. D) they are the end-products of small, low-mass stars. E) they are the opposite of black holes. 22) What happens to the surface temperature and luminosity wh ...
universe.pps - Prophet Muhammad For All
universe.pps - Prophet Muhammad For All

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Perseus (constellation)



Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.
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