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Binary Stars (Professor Powerpoint)
Binary Stars (Professor Powerpoint)

... that the stars pass in front of each other as seen from the Earth. Each eclipse will cause the total light from the system to decrease. The amount of the decrease will depend on how much of each star is covered up. The period is from one large dip to the next and with the period you can get the mass ...
AAS/AAPT meeting consolidated synopses by Richard Berry PDF
AAS/AAPT meeting consolidated synopses by Richard Berry PDF

... Solar System Formation. (Doug Lin) Described the dynamics of planetary formation in the proto-planetary disk. Perturbations lead to instabilities and eccentricities, thus migration of planet inward or outward is possible. Stable orbit is prerequisite to forming life. Solar System Formation Simulatio ...
Intro to Spectroscopy
Intro to Spectroscopy

... Stanford University Solar Center ...
Chapter 29 Notes
Chapter 29 Notes

... – Apparent magnitude: how bright the star appears from Earth – Absolute magnitude: how bright a star would look if it were 10 parsecs away ...
Fingerprints in Sunlight - VCI
Fingerprints in Sunlight - VCI

... Stanford University Solar Center ...
Models of the Solar System
Models of the Solar System

... also known as “The Observatory,” is located on the Yucatan peninsula. It is thought that the Mayans used El Caracol for astronomical ...
The Night Sky May 2016 - Bridgend Astronomical Society
The Night Sky May 2016 - Bridgend Astronomical Society

... lie within its boundaries. Spica is, in fact, an exceedingly close double star with the two B type stars orbiting each other every 4 days. Their total luminosity is 2000 times that of our Sun. In the upper right hand quadrant of Virgo lies the centre of the Virgo Cluster of galaxies. There are 13 ga ...
6 Very High Energy Gamma Ray Astronomy with CTA - UZH
6 Very High Energy Gamma Ray Astronomy with CTA - UZH

–1– AST104 Sp2006: EXAM 1 Multiple Choice Questions: Mark the
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... 32. In addition to lens quality, which are MOST important for the effectiveness of an optical tele- due to rapid rotation scope? c. It is a force induced by orbital revolution a. light-gathering power, resolving power, d. It results from the differential gravitastability of mounting and positioning ...
SALT/SAAO introduction
SALT/SAAO introduction

... SALT will be the largest single optical-infrared telescope in the southern hemisphere. SALT will detect objects one billion times dimmer than the faintest visible to the unaided eye. It will gather 23 times ax much light as the 1.9-m telescope at Sutherland, currently the largest in Africa. SALT wil ...
PHYS 2410 General Astronomy Homework 5
PHYS 2410 General Astronomy Homework 5

... Which star in the table above would appear the faintest in the night sky? ...
The Epic of Gilgamesh is, perhaps, the oldest written story on Earth
The Epic of Gilgamesh is, perhaps, the oldest written story on Earth

... The Epic of Gilgamesh is, perhaps, the oldest written story on Earth. It comes to us from Ancient Sumeria, and was originally written on 12 clay tablets in cuneiform script. It is about the adventures of the historical King of Uruk (somewhere between 2750 and 2500 BCE). The Epic speaks of “fire, bri ...
The Epic of Gilgamesh is, perhaps, the oldest written story on Earth
The Epic of Gilgamesh is, perhaps, the oldest written story on Earth

... The Epic of Gilgamesh is, perhaps, the oldest written story on Earth. It comes to us from Ancient Sumeria, and was originally written on 12 clay tablets in cuneiform script. It is about the adventures of the historical King of Uruk (somewhere between 2750 and 2500 BCE). The Epic speaks of “fire, bri ...
August 2014 - Hermanus Astronomy
August 2014 - Hermanus Astronomy

... When Comet ISON was discovered in the autumn of 2012, scientists and amateur astronomers alike hoped for a ‘comet of the century’. On 28 November 2013, only 1.8 million km would separate ISON from the Sun. Due to its brightness, the comet promised to be a unique research object and, should it surviv ...
Telescopes: More Than Meets the Eye
Telescopes: More Than Meets the Eye

... Lens: A spherical shaped piece of glass or crystal that bends light together to a single point at a set distance from where the light enters the lens. A magnifying glass is a single lens. Refracting telescopes often use multiple lenses. Light Gathering: This term refers to the ability of a telescope ...
Stellar Formation 1) Solar Wind/Sunspots 2) Interstellar Medium 3) Protostars
Stellar Formation 1) Solar Wind/Sunspots 2) Interstellar Medium 3) Protostars

... travel outward from the Sun responsible for comet’s tail and for blowing away primary atmospheres of inner planets pushes interstellar dust out of the Solar System ...
STARS
STARS

... • Most stars are between 1 billion and 10 billion years old. Some stars may even be close to 13.7 billion years old—the observed age of the universe. The oldest star yet discovered, HE 1523-0901, is an estimated 13.2 billion years old. • The more massive the star, the shorter its lifespan, primarily ...
PHYSICS 1500 - ASTRONOMY TOTAL: 100 marks Section A Please
PHYSICS 1500 - ASTRONOMY TOTAL: 100 marks Section A Please

... highlands. The planets of the solar system formed in an accretion disk around the infant Sun. Nuclear reaction rates inside stars increase rapidly with temperature. Stars lose significant amounts of mass during their lifetime. ...
Lab Writeup
Lab Writeup

... eyepiece of our refractor telescopes. At least two eyepieces will be used. The first will have a fairly large field of view. The second will have higher magnification, and has a scale which allows you to fairly accurately measure small angles. The focal length of the Orion 80 “short tube” refractor ...
Big Island Discussions II 08 03 06 - Alt
Big Island Discussions II 08 03 06 - Alt

... active primary mirror would require some sort of on-line wavefront sensor, such as a Shack-Hartmann sensor. Although Gemini does utilize an on-line wavefront sensor for primary mirror adjustments, Subaru does not. Subaru calibrates their system offline with a wavefront sensor on bright stars with 30 ...
Properties of Stars
Properties of Stars

... Measuring Distance to Stars • Parallax is determined by taking a picture of a star at one time, and another picture six months later; using the angle between its apparent shift, astronomers can determine how far away it is • The nearest stars have large parallax angles, while those of distant stars ...
Introduction to Lookback
Introduction to Lookback

... early part of the 1600s that Galileo and others proposed experiments to determine its speed. Some of these experiments were tried, but they failed to determine a speed of light since the distances used were too small (a few miles). It was not until 1676 that an actual measurement of the speed of lig ...
space tech - Project Jugaad
space tech - Project Jugaad

SO FAR:
SO FAR:

... • Coordinate systems • Spherical coordinates centered on Sun: Galactic latitude (lII) , longitude (bII) ...
Gravitation and the Motion of the Planets
Gravitation and the Motion of the Planets

... • Ancient astronomers believed the Earth to be at the center of the universe • They invented a complex system of epicycles and deferents to explain the direct and retrograde motions of the planets on the celestial sphere ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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