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Astronomy
Astronomy

... The star is now in the “prime of its life”; it is in equilibrium. Over time; temp, luminosity, color change. Our sun is in the main sequence phase It will live for about 10 billion years Our sun is now about 4.6 billion years old – Links: ...
Introduction - Willmann-Bell
Introduction - Willmann-Bell

... at the top of anyone’s observing list, but like its bigger brother, Canis Major, it contains a prominent first-magnitude star, Procyon, with a white dwarf companion nearly hidden in the primary’s glare. The orbit of Procyon B itself is nearly circular, but the periastron and the apastron junctures a ...
Theoretical Problem 3
Theoretical Problem 3

... relationship is fulfilled; however, this is not true. The gas inside normal stars fusing hydrogen is known to behave approximately as an ideal gas. This means that d e , the typical separation between electrons is on the average larger that λe , their typical de Broglie wavelength. If closer, the el ...
Lecture5 - Tufts Institute of Cosmology
Lecture5 - Tufts Institute of Cosmology

... Difference between Newtonian Theory of Gravity and General Theory of Relativity • Newtonian: The Sun creates a gravitational field that exerts a force upon the Earth, which, in turn, causes it to orbit around the Sun rather than move in a straight line • General Relativity: The Mass-Energy Distribu ...
Deep Space (PDF: 224k)
Deep Space (PDF: 224k)

cassiopeia a - Chandra X
cassiopeia a - Chandra X

... debris field of hot gas and energetic particles created when a massive star explodes. WHERE: Cas A, at a distance of 11,000 light years from Earth, is in the constellation Cassiopeia. This constellation is widely known for its “W” shape that Greek and Roman mythology identified as a queen’s throne. ...
eneb_form
eneb_form

... • There are two stars, star A and star B. Star A is approaching the Earth at 100 km/s and Star B is moving away from the Earth at 200 km/s. • Compare the Doppler shift for these two stars by explaining how the spectra will be shifted and by how much. (I am not looking for a number here, just a quali ...
The Milky Way - TCNJ | The College of New Jersey
The Milky Way - TCNJ | The College of New Jersey

... • This is dominated by DARK MATTER, but total mass can be estimated by the velocity of stars at different distances. • Out to solar distance (about 8 kpc) the mass is about 1 x 1011 M (mostly stars) • Out to ~15 kpc, (the visible radius) a good estimate for the mass is nearly 4 x 1011 M (now mostl ...
Stars and Temperature and Color
Stars and Temperature and Color

... surface of the star. • The same is true for the filament in a light bulb or any other hot object. In general, we call radiation from a hot body `black body’ radiation (do demonstration 6B40.10). ...
Astro history notes 1
Astro history notes 1

Distance Measurement in Astronomy
Distance Measurement in Astronomy

Sydney Observatory night sky map June 2014
Sydney Observatory night sky map June 2014

... For more information, check the website at www.sydneyobservatory.com or call (02) 9921 3485. Sydney Observatory is at 1003 Upper Fort Street, Observatory Hill, in the historic Rocks area of Sydney. Sydney Observatory is part of the Powerhouse Museum. The Sydney Observatory night sky map is prepared ...
Star Jeopardy Review #2
Star Jeopardy Review #2

... for 10 million years, yet its iron core can exist for only a ...
November 2013 - Pomona Valley Amateur Astronomers
November 2013 - Pomona Valley Amateur Astronomers

File - Etna FFA Agriculture
File - Etna FFA Agriculture

... were more habitable for life.  Also, increased Earths size and caused thermal energy. ...
HR Diagram Explorer Worksheet
HR Diagram Explorer Worksheet

... HR Diagram Explorer Worksheet Open the HR Diagram Explorer. Begin by familiarizing yourself with the capabilities of the HertzsprungRussell Diagram Explorer through experimentation.  An actual HR Diagram is provided in the upper right panel with an active location indicated by a red x. This active ...
Astrophysics Outline—Option E
Astrophysics Outline—Option E

... State that the luminosity of a star may be estimated from its spectrum. E.3.10 Explain how stellar distance may be determined using apparent brightness and luminosity. E.3.11 State that the method of spectroscopic parallax is limited to measuring stellar distances less than about 10 Mpc. E.3.12 Solv ...
Experimental Low Earth Orbit Surveillance Stereoscope
Experimental Low Earth Orbit Surveillance Stereoscope

THE CHANGING SKY
THE CHANGING SKY

... → These buttons allow you to change the time of your observation. → E : Enter any time and date. → 1 , 5 , 10 : Advance time by 1, 5, or 10 minutes (left mouse button = forward in time, right mouse button = backward in time). → H , D , W , M , Y : Advance time by one hour, day, week, month, year (le ...
1. a) Astronomers use the parallax method to measure
1. a) Astronomers use the parallax method to measure

... distance to stars in other galaxies. In particular, we use the standard candle method to measure the distances to Cepheid variable stars in other galaxies. What is special about Cepheid variable stars that makes them useful for this purpose? We can figure out their luminosities from their periods of ...
Topic Outline - Physics Rocks!
Topic Outline - Physics Rocks!

... E.3.11 State that the method of spectroscopic parallax is limited to measuring stellar distances ...
Volume 20 Number 10 September 2012
Volume 20 Number 10 September 2012

... same as the spectacular Perseids shower which peaks in mid-August and is one of the year's highlights. They both appear to radiate from the same constellation but are not related - they were formed by different comets. September has five minor showers with three or less per hour. ------------------- ...
Introduction to Accretion Phenomena in Astrophysics
Introduction to Accretion Phenomena in Astrophysics

What we can measure
What we can measure

... and watch one orbit the other. These are called visual binaries. We need to be careful here, since some stars only appear to be close due to our perspective. These are called “optical doubles” and not real binary systems at all. We can tell the difference by watching these over time or by noting tha ...
Young Stars
Young Stars

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Hipparcos



Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993. It was the first space experiment devoted to precision astrometry, the accurate measurement of the positions of celestial objects on the sky. This permitted the accurate determination of proper motions and parallaxes of stars, allowing a determination of their distance and tangential velocity. When combined with radial-velocity measurements from spectroscopy, this pinpointed all six quantities needed to determine the motion of stars. The resulting Hipparcos Catalogue, a high-precision catalogue of more than 118,200 stars, was published in 1997. The lower-precision Tycho Catalogue of more than a million stars was published at the same time, while the enhanced Tycho-2 Catalogue of 2.5 million stars was published in 2000. Hipparcos‍ '​ follow-up mission, Gaia, was launched in 2013.The word ""Hipparcos"" is an acronym for High precision parallax collecting satellite and also a reference to the ancient Greek astronomer Hipparchus of Nicaea, who is noted for applications of trigonometry to astronomy and his discovery of the precession of the equinoxes.
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