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T
T

... The long-term precision of the instrument cannot be checked easily because it requires a long time base on one hand, and the knowledge of stable stellar sources on the other hand. Especially the latter point represents a new challenge since the intrinsic stability of the stars has never been studied ...
Heliacal Rising of Canopus in Indian Astronomy
Heliacal Rising of Canopus in Indian Astronomy

Summer 2004 ISP 205: Visions of the Universe Professor: ER Capriotti Sample Questions
Summer 2004 ISP 205: Visions of the Universe Professor: ER Capriotti Sample Questions

... Ptolemy's view of the universe, the Sun moved in an elliptical orbit. the Moon could have craters but not mountains. Kepler's Harmonic Law still worked. Jupiter had four satellites. Venus would never be close to the full phase ...
Chemical Evolution
Chemical Evolution

Surface  Gravity  as  a  Diagnostic ... Youth Cameron Higby-Naquin Advisor:  Eric  Jensen
Surface Gravity as a Diagnostic ... Youth Cameron Higby-Naquin Advisor: Eric Jensen

... so at some point in their evolution, T Tauri stars lose their disks. This is part of the transition between the TTS phase and the post T Tauri phase. While a great many TTS have been found simply by looking at known star-forming regions, post-T Tauri Stars (PTTS) are more difficult to locate. These ...
1: Properties of Pulsars
1: Properties of Pulsars

... from the central "strange" star, identifying it as a pulsar. It turned out later, that these "giant pulses" which they observed, occur every two minutes or so, and that the true pulse period was in fact as short as 33 milliseconds. The short period of 33 milliseconds ruled out white dwarfs for being ...
A Universe of Galaxies - Pennsylvania State University
A Universe of Galaxies - Pennsylvania State University

... What can outshine ~1000 supernovae for millions of years, and be just slightly larger than our Solar System? Theoretically, not much – only a very, very big black hole. • Start with a black hole with a mass of 10,000,000,000 Mʘ • Have a star come close enough to be tidally disrupted • Have the mater ...
Lecture17-ASTA01
Lecture17-ASTA01

Introduction - Cambridge University Press
Introduction - Cambridge University Press

Lives of the Stars Lecture 5: Star birth
Lives of the Stars Lecture 5: Star birth

... easily destroyed. Helium-4 is the only really stable one, so lots of Helium-4 was formed in the next few seconds. But apart from tiny amounts of Lithium-7, no other element can be easily formed. So when the era of fusion ended, about 3½ minutes after the Big Bang, the universe consisted of lots of h ...
Lab 7
Lab 7

... declination (think of this as a space latitude). The declination runs from -90° (celestial south pole) to +90° (celestial north pole). Both of these coordinates are laminated to the metal pole bases. In addition, the stars have been colored according to their spectral classes; blue balls represent O ...
10 Measuring The Stars
10 Measuring The Stars

WHAT MAKES A STAR SO SPECIAL Abstract
WHAT MAKES A STAR SO SPECIAL Abstract

... luminosity, or 1000 red stars from class M with low luminosity. This statistics shows that the formation of stars with low masses is a very common process. If we plot the spectral classes (or the temperature, which is the same) along the x-axis and the luminosity (or stars’ absolute magnitude) along ...
Chapter 16--Properties of Stars
Chapter 16--Properties of Stars

Local Horizon View
Local Horizon View

... Meridian is SETTING, just like the Sun does. (In the southern hemisphere, your large area of sky is facing north, stars rise in the east (on your right) and set in the west (on your left). Everything on your Meridian has therefore reached its HIGHEST point in the sky tonight, and is therefore at its ...
D ASTROPHYSICS
D ASTROPHYSICS

... isolation but the majority of them occur in groups known as clusters that have anything from a few dozen to a few thousand members. The Milky Way is part of a cluster of about 30 galaxies called the “Local Group” which includes Andromeda (figure 7) and Triangulum. Regular clusters consist of a conce ...
Extrasolar planets - Astronomisk Ungdom
Extrasolar planets - Astronomisk Ungdom

sections 12-15 instructor notes
sections 12-15 instructor notes

Star formation in galaxies over the last 10 billion
Star formation in galaxies over the last 10 billion

and heliacal visibility of star agastya in 1350
and heliacal visibility of star agastya in 1350

Star 1 A star is a massive, luminous ball of plasma held together by
Star 1 A star is a massive, luminous ball of plasma held together by

... 11th century, the Persian polymath scholar Abu Rayhan Biruni described the Milky Way galaxy as a multitude of fragments having the properties of nebulous stars, and also gave the latitudes of various stars during a lunar eclipse in 1019.[21] The Andalusian astronomer Ibn Bajjah proposed that the Mil ...
a wide-field survey for variable stars
a wide-field survey for variable stars

... The orange star at the center of the image is T Tauri, prototype of the class of T Tauri variable stars. The nearby dusty, yellow cloud is Hind’s Variable Nebula (NGC 1555/1554). Over 400 light-years away, at the edge of a molecular cloud, both star and nebula are seen to vary significantly in brigh ...
16_Testbank
16_Testbank

... D) 30 E) 200 Answer: E 37) Which of the following discoveries, if they existed, would necessitate a reevaluation of our ideas of stellar formation? A) a cluster of stars that appeared to be 13 billion years old B) a 100-solar-mass star C) a 0.01-solar-mass star D) a molecular cloud without any stars ...
PDF - Department of Statistics
PDF - Department of Statistics

... phase of the early evolution of the solar system. This belt is the source of most short–period comets, those with periods of 200 years or less [Edgeworth, 1949], [Kuiper, 1951], [Fernandez, 1980]. Observational success was first achieved with the discovery of 1992QB1 [Jewitt and Luu, 1993]. Major ob ...
11-Massive Stars
11-Massive Stars

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Lyra



Lyra (/ˈlaɪərə/; Latin for lyre, from Greek λύρα) is a small constellation. It is one of 48 listed by the 2nd century astronomer Ptolemy, and is one of the 88 constellations recognized by the International Astronomical Union. Lyra was often represented on star maps as a vulture or an eagle carrying a lyre, and hence sometimes referred to as Aquila Cadens or Vultur Cadens. Beginning at the north, Lyra is bordered by Draco, Hercules, Vulpecula, and Cygnus. Lyra is visible from the northern hemisphere from spring through autumn, and nearly overhead, in temperate latitudes, during the summer months. From the southern hemisphere, it is visible low in the northern sky during the winter months.The lucida or brightest star—and one of the brightest stars in the sky—is the white main sequence star Vega, a corner of the Summer Triangle. Beta Lyrae is the prototype of a class of stars known as Beta Lyrae variables, binary stars so close to each other that they become egg-shaped and material flows from one to the other. Epsilon Lyrae, known informally as the Double Double, is a complex multiple star system. Lyra also hosts the Ring Nebula, the second-discovered and best-known planetary nebula.
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