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Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

... • Usually leaves neutron star For high mass stars • fusion continues beyond C,O to Iron • if Mass(core) > 1.4 M(Sun) core collapses in SUPERNOVA (II) • leaves either Neutron Star or Black Hole • Most SN are this type PHYS 162 ...
- Scholieren.com
- Scholieren.com

... Astronomers now know that the earth completes its orbit in a shorter period of time than the planets outside its orbit. As a result, earth periodically overtakes the outer planets, like a faster car on a multi lane highway. When this occurs, the planet earth is passing will first appear to stop its ...
Astron 104 Laboratory #9 Cepheid Variable Stars
Astron 104 Laboratory #9 Cepheid Variable Stars

observingnebulaeclusters-1
observingnebulaeclusters-1

... taken with the 4-meter telescope at Kitt Peak National Observatory. A spectacular cloud of gas surrounds several very hot stars in the star cluster deep within the nebula. The nebula's constituent gases include hydrogen, helium, oxygen, carbon, neon, nitrogen, sulphur, argon, and chlorine; the densi ...
NCEA Level 2 Earth and Space Science (91192) 2015
NCEA Level 2 Earth and Space Science (91192) 2015

... Molecular Cloud (GMC). The dust and gas can be caused to condense together by an outside force, such as a nearby star going supernova, or just the gravity of a near star. As the GMC condenses under gravity, it forms a protostar. As the protostar condenses, the particles become hotter (due to frictio ...
NCEA Level 2 Earth and Space Science (91192) 2015
NCEA Level 2 Earth and Space Science (91192) 2015

Session: [B5B-3] S3 : Stars, Exoplanets and Stellar Systems Date
Session: [B5B-3] S3 : Stars, Exoplanets and Stellar Systems Date

... The common-envelope process is known as one complicated phase in binary evolution. A lot of efforts have been dedicatedto study this common-envelope stage, but the many questions related to this process are yet to be answered. If one binary survives the common-envelope, the binary will emerge asa wh ...
Astronomy Assignment #1
Astronomy Assignment #1

... with a diameter of 1.23 solar diameters. Alpha Centauri B is (60/85) = 0.706 times smaller than Alpha Centauri A. based on the ratio of their angular sizes (and the fact that they are at the same distance). So Alpha Centauri B is slightly smaller than the Sun with a diameter of 0.867 solar diameters ...
In class Review Notes(5-20-14)
In class Review Notes(5-20-14)

... remaining isotope of carbon 14 or uranium 238 to find the age of rock… scientists must know the half life to do the calculations. ...
Subject- Geography Class- VI Chapter 1
Subject- Geography Class- VI Chapter 1

... hydrogen as well as helium and smaller amounts of other elements. The Sun is the closest star to Earth. THE SUN: The Sun is a star and the biggest object in the Solar System, it burns brightly in the center as planets and other objects orbit around it. It has a diameter around 110 times bigger than ...
Mar - Wadhurst Astronomical Society
Mar - Wadhurst Astronomical Society

star
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... Orbit = path that a planet follows as it travels around sun Period of revolution = the time it takes for a planet to make one trip in its orbit around the sun = the length of that planet’s year Planets revolve around the sun counter-clockwise if watching from Polaris ...
Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

... • fusion continues beyond C,O to Iron • if Mass(core) > 1.4 M(Sun) core collapses in SUPERNOVA (II) • leaves either Neutron Star or Black Hole • Most SN are this type PHYS 162 ...
Lab 1: The Celestial Sphere
Lab 1: The Celestial Sphere

Today: Magnitude Terminology Photometry Applications Reading
Today: Magnitude Terminology Photometry Applications Reading

... Vega); typically obtained by calculating differential  magnitude w.r.t. a known standard star. ...
Latitude and Longitude - Northside Middle School
Latitude and Longitude - Northside Middle School

... Polaris is located directly over the tropic of cancer b) Polaris is the brightest and most easily located star c) The altitude of Polaris is equal to the observers latitude d) The position of Polaris changes with the seasons a) ...
July - Westchester Amateur Astronomers
July - Westchester Amateur Astronomers

... Strange but true: When it comes to finding new extrasolar planets, or exoplanets, stars can be an incredible nuisance. It’s a matter of luminosity. Stars are bright, but their planets are not. Indeed, when an astronomer peers across light years to find a distant Earth-like world, what he often finds ...
Astrophysics - Florence
Astrophysics - Florence

... times, they can erupt,escaping the Sun's atmosphere. http://www.nasa.gov/multimedia/imagegallery/image_feature_21.html ...
Nebula Beginnings - University of Dayton
Nebula Beginnings - University of Dayton

... This image from NASA's Hubble Space Telescope shows for the first time the inner region of a 200-billion mile diameter dust disk around the star Beta Pictoris. This region has long been hidden from ground-based telescopes because of the glare from the central star. The disk is slightly warped. If th ...
Lecture 2+3 - University of Texas Astronomy Home Page
Lecture 2+3 - University of Texas Astronomy Home Page

... Stars: Energy Generation Death of Stars: Planetary Nebulae, Supernovae Remnants Why is human life ‘star stuff’? Different types of Nebulae Planets, Brown Dwarfs, Moons and our Solar system Galaxies and the Milky Way The Local Group, Clusters of Galaxies Superclusters, voids and filaments -- Distance ...
The Sun: Example of Radiation Laws
The Sun: Example of Radiation Laws

... in Type II supernovae was confirmed by SN 1987a in the Large Magellenic Cloud, a nearby galaxy, on February 23, 1987. Neutrino detectors in Ohio and Japan detected a total of about 20 neutrinos even though this supernova was 180,000 lt.-yrs. from the Earth. Radiactive Ni, Co and Ti nuclei were also ...
Lecture12
Lecture12

... A certain star has 100 times the luminosity of the Sun and a surface temperature of 3500 K. What type of star is it? A. A high-mass main-sequence star B. A low-mass main-sequence star C. A red giant D. A red dwarf E. A white dwarf ...
Ch. 22 Honors Study Guide Name 1. How did Eratosthenes
Ch. 22 Honors Study Guide Name 1. How did Eratosthenes

... 7. Even though Copernicus was right about the Heliocentric model, the planets did not line up where he thought they should. What was wrong with Copernicus’ model? 8. Why were Tycho Brahe’s observations so important in Astronomy? 9. Why didn’t Tycho Brahe believe the Sun was the center of the Solar S ...
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TCE Syllabus Summary Blank

Shocking Truth about Massive Stars Lidia Oskinova Chandra’s First Decade of Discovery
Shocking Truth about Massive Stars Lidia Oskinova Chandra’s First Decade of Discovery

... ’’A very energetic explosion of a massive star is likely to create a ... fireball.... the inner core of a massive, rapidly rotating star collapses into a ~10 M Kerr black hole ... A superstrong ~10 15 G magnetic field is needed to make the object ... a microquasar. Such events must be vary rare...to ...
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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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