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Astronomy Assignment #1
Astronomy Assignment #1

... The diameter of Alpha Centauri A is 1.71 x 109 meters. The Sun’s diameter is 1.39 x 109 meters as determined from the table in the text’s appendix. Thus, Alpha Centauri A is slightly larger than the Sun with a diameter of 1.23 solar diameters. Alpha Centauri B is (60/85) = 0.706 times smaller than A ...
Emission and Absorption Spectra
Emission and Absorption Spectra

... A. the peak of star A’s spectrum would be at a shorter wavelength than star B and it would be bluer B. the peak of star A’s spectrum would be at a longer wavelength than star B and it would be redder C. the peak of star A’s spectrum would be at a shorter wavelength than star B and it would be redder ...
Black Hole
Black Hole

The Earth--Our Observing Platform
The Earth--Our Observing Platform

... especially difficult. Work on them not only resulted in the birth of modern physical science in the 17 th century, but it had critically important historical ramifications. Most notably, while Columbus knew the correct answer to problem A), his mistaken answer to problem B) (he believed the Earth wa ...
I Cloudy with a Chance of Making a star is no easy thing
I Cloudy with a Chance of Making a star is no easy thing

... another? The standard theory describes individual stars in isolation; it does not say what happens when they form in close proximity, as most stars do. Recent fi ndings suggest that our own sun was born in a cluster, which has since dispersed [see “The Long-Lost Siblings of the Sun,” by Simon F. Por ...
April
April

... as the Black Eye Galaxy, this object has a diameter of about 51,000 LY. Steady seeing will offer viewers a bright irregular shape with uneven brightness and texture. This is as a result of an unusual characteristic: the central portion of the galaxy rotates in one direction out to approximately 3,00 ...
Micro_lect20a
Micro_lect20a

... Sun, it is more massive and over 1000 times larger. If placed at the center of our Solar System, it would extend past the orbit of Jupiter. ...
Vocabulary Terms - Dayton Independent Schools
Vocabulary Terms - Dayton Independent Schools

Chapter 12
Chapter 12

... correlated with its luminosity. The more luminous it is, the more slowly it pulsates. => Measuring a Cepheid’s period, we can determine its absolute magnitude! ...
03jan13.ppt - Institute for Astronomy
03jan13.ppt - Institute for Astronomy

... Axis tilt changes directness of sunlight during the year. ...
Exploring the Outer Solar System Jane Luu When I was
Exploring the Outer Solar System Jane Luu When I was

... the occulting body is; this technique has long been used for astronomers to measure the size of nearby asteroids. In our case, we just wanted to use occultations to indicate the presence of distant objects; size was a secondary issue. The whippoorwills of Arizona quickly put an end to our occultatio ...
Solar
Solar

... area • Sunspots change over a period of days and move across the Sun as it rotates • They have a strong magnetic field associated with them and last from a few days to a few weeks ...
Stars
Stars

... fusion at once. What a star normally takes billions of years to burn, this star burns all at once. BIG explosion! ...
Unit 2 Lesson 1
Unit 2 Lesson 1

... • SC.8.N.1.5 Analyze the methods used to develop a scientific explanation as seen in different fields of science. • SC.8.N.3.1 Select models useful in relating the results of their own investigations. • SC.8.E.5.1 Recognize that there are enormous distances between objects in space and apply our kno ...
New Moons for Pluto!
New Moons for Pluto!

... The newly discovered objects are much smaller than Charon. Charon is about half Pluto’s size. The two new objects are about twice as far away from Pluto as Charon, but still close to the planet. A second image of Pluto taken three days later showed the objects in the same area. Scientists thought th ...
The basic physical properties of a star Hydrostatic equilibrium
The basic physical properties of a star Hydrostatic equilibrium

... Applying Newton’s second law to an element of mass m at the stellar surface (radius R), gives FG=m dv/dt , or ...
Lecture 15 (pdf from the powerpoint)
Lecture 15 (pdf from the powerpoint)

... Space Telescope reveals The Cat's Eye Nebula to be one of the most complex planetary nebulae known. In fact, the features seen in the Cat's Eye are so complex that astronomers suspect the bright central object may actually be a binary star system. ...
The Rotational Period of the Sun (Higher Level)
The Rotational Period of the Sun (Higher Level)

Stellar Evolution after the Main Sequence
Stellar Evolution after the Main Sequence

... The result is a Type II supernova It is up to 100 billion times more luminous than the Sun The light rapidly rises to maximum brightness then gradually decreases over several weeks to months This happens in a galaxy similar to the Milkyway about once every fifty years on the average. ...
Lecture 10: The Milky Way
Lecture 10: The Milky Way

... 1. Distances We only have parallax distance measurements out to about 100pc (Gaia will take us much further in the next few years). This gives us the absolute luminosities of low-mass stars, and using binary systems we can calibrate our models to true masses and radii (see earlier). The trouble is ...
Star Cycle2013
Star Cycle2013

... Star Power Stars are powered by nuclear fusion • At 15 million degrees Celsius in the center of the star, fusion occurs. • Very simplified: 4 Hydrogen  1 Helium + energy! ...
Solutions - Yale Astronomy
Solutions - Yale Astronomy

... electromagnetic spectrum. Stars behave as blackbodies thus, despite peaking in the UV, it emits light at all wavelengths. The amount of flux a star emits is directly proportional to T4 , thus for a star with a high surface temperature will also emit more flux at all wavelengths than a similar star w ...
Main Types of Galaxies
Main Types of Galaxies

... gas, and dust in space that are held together by gravity. • The largest galaxies contain more than a trillion stars. Smaller galaxies may have only a few million. • Scientists estimate the number of stars from the size and brightness of the galaxy. ...
Galaxies, Cosmology and the Accelera`ng Universe
Galaxies, Cosmology and the Accelera`ng Universe

... –  The  stars  just  go  through  each  other,  too  far  apart  to   collide   –  The  gas  collides,  and  creates  new  stars   –  Typical  result:  long  streams  of  new  stars,  large  gravita6onal   distor6on  of  the  galaxies   ...
Galaxies Powerpoint
Galaxies Powerpoint

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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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