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Orion the Hunter
Orion the Hunter

... south. Betelgeuse is a red giant half as far away as Rigel. With an angular size of over 0.1", Betelgeuse’s diameter would encompass the orbit of Jupiter. All three of Orion’s “belt stars” are blue-white suns of very similar spectral types. On transparent nights, look for the large number of 6thand ...
Heliacal Rising of Canopus in Indian Astronomy
Heliacal Rising of Canopus in Indian Astronomy

... HELIACAL RISING OF CANOPUS IN INDIAN ASTRONOMY ...
Comets, historical records and vedic literature
Comets, historical records and vedic literature

... Ketus (in plural), meaning rays of light or fire-smoke combine, have also been discussed in Atharvaveda, and it is very likely that they represented comets or meteors (Kochhar, 2010). Book one of Rigveda has two hymns (1,24,7) and (1,24,8) which have been translated by Griffith (1896) as follows: 7. ...
FOE 2017 Poster Contributions - College of Science | Oregon State
FOE 2017 Poster Contributions - College of Science | Oregon State

... and to identify these components of the model which can be reduced to the linear form. According to our preliminary results, for the considered sample size of 116 GRBs the model produced by GAM has a substantially larger predictive power than the model produced by random forest. It allows extraction ...
Neutrinos and Supernovae
Neutrinos and Supernovae

magnitude handout
magnitude handout

Polaris
Polaris

... nearly still in our sky while the entire northern sky moves around it. That’s because it’s located nearly at the north celestial pole, the point around which the entire northern sky turns. Polaris marks the way due north. As you face Polaris and stretch your arms sideways, your right hand points due ...
Astrophysical explosions: from solar flares to cosmic gamma
Astrophysical explosions: from solar flares to cosmic gamma

17_Testbank
17_Testbank

... 38) What types of stars end their lives with supernovae? A) all stars that are red in color B) all stars that are yellow in color C) stars that are at least several times the mass of the Sun D) stars that are similar in mass to the Sun E) stars that have reached an age of 10 billion years Answer: C ...
October 2016 BRAS Newsletter - The Baton Rouge Astronomical
October 2016 BRAS Newsletter - The Baton Rouge Astronomical

... raw data. She needs descriptions of views of five Messier objects—Pleiades, Orion Nebula, Andromeda Galaxy, Beehive Cluster, Whirlpool Galaxy—together with date and time, and the observing location’s GaN measurement and quality of view. Parameters have been set defining whether each observation yiel ...
1 - Piscataway High School
1 - Piscataway High School

New Double Stars from Asteroidal Occultations, 1971 - 2008
New Double Stars from Asteroidal Occultations, 1971 - 2008

Seeing Red: Will Betelgeuse Go Supernova in
Seeing Red: Will Betelgeuse Go Supernova in

Module3: Life of a Star
Module3: Life of a Star

September - Rose City Astronomers
September - Rose City Astronomers

... under truly dark skies. Unfortunately, this is something Messier couldn’t enjoy with his telescopes. A surprising thing happened while trying a TeleVue Paracorr in the 80mm - I found that they’re not at all compatible. The Paracorr caused enormous distortion across the full fov. Obviously, achromati ...
The Antares Emission Nebula and Mass Loss of α Sco A
The Antares Emission Nebula and Mass Loss of α Sco A

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telling time at night

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classifying stars

Lecture 12: Evolution of the Galaxy
Lecture 12: Evolution of the Galaxy

November News Letter - Boise Astronomical Society
November News Letter - Boise Astronomical Society

Supernovae - University of Texas Astronomy Home Page
Supernovae - University of Texas Astronomy Home Page

... entire galaxy. Estimates of the energy involved in such a process reveal that a major portion of the star, if not the entire star, must be blown to smithereens. Historical records, particularly the careful data recorded by the Chinese, show that seven or eight supernovae have exploded over the last ...
Aldebaran
Aldebaran

The Magnitude System
The Magnitude System

... The magnitude system is invented by Hipparchus in 120 BC, and is still used today, although the magnitude scale itself is not a meaningful “physical quantity” (it is just a scale). Initially this system was arbitrary because Hipparchus decided that all the brightest and most beautiful stars had a ma ...
Chapter 13 Measuring the properties of stars
Chapter 13 Measuring the properties of stars

Section 2
Section 2

... Orion  constellations. For example, a large constellation in the winter sky is named Orion, the Hunter, after a Greek myth. In this constellation, Orion is seen with a sword in his belt and an upraised arm. The ancient Sumerians thought that the stars in Orion formed the outline of a sheep. In anci ...
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SN 1054



SN 1054 is a supernova that was first observed on 4 July 1054 A.D. (hence its name), and that lasted for a period of around two years. The event was recorded in contemporary Chinese astronomy, and references to it are also found in a later (13th-century) Japanese document, and in a document from the Arab world. Furthermore, there are a number of proposed, but doubtful, references from European sources recorded in the 15th century, and perhaps a pictograph associated with the Ancestral Puebloan culture found near the Peñasco Blanco site in New Mexico.The remnant of SN 1054, which consists of debris ejected during the explosion, is known as the Crab Nebula. It is located in the sky near the star Zeta Tauri (ζ Tauri). The core of the exploding star formed a pulsar, called the Crab Pulsar (or PSR B0531+21). The nebula and the pulsar it contains are the most studied astronomical objects outside the Solar System. It is one of the few Galactic supernovae where the date of the explosion is well known. The two objects are the most luminous in their respective categories. For these reasons, and because of the important role it has repeatedly played in the modern era, SN 1054 is the best known supernova in the history of astronomy.The Crab Nebula is easily observed by amateur astronomers thanks to its brightness, and was also catalogued early on by professional astronomers, long before its true nature was understood and identified. When the French astronomer Charles Messier watched for the return of Halley's Comet in 1758, he confused the nebula for the comet, as he was unaware of the former's existence. Due to this error, he created his catalogue of non-cometary nebulous objects, the Messier Catalogue, to avoid such mistakes in the future. The nebula is catalogued as the first Messier object, or M1.
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