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November - LVAstronomy.com
November - LVAstronomy.com

... known as the Milky Way. We know this glow is the plane of our home galaxy and holds a multitude of open star clusters. Dozens of these galactic clusters are found in Cassiopeia. One of the finest, but often overlooked, is NGC-7789. Cassiopeia is one of the most recognized constellations. The constel ...
SMMP_BISANA - Infinity and Beyond
SMMP_BISANA - Infinity and Beyond

Star Formation
Star Formation

Shining Light on the Stars: The Hertzsprung-Russell
Shining Light on the Stars: The Hertzsprung-Russell

... Sirius’ companion, an Earth-size stellar corpse known as a white dwarf. White dwarfs are extremely dense because they contain as much mass as the Sun but in a volume only the size of the Earth. A teaspoon of white dwarf material would weigh 15 tons on Earth! Within our 25 light year neighborhood, t ...
Lecture 15 Star Formation and Evolution 3/7
Lecture 15 Star Formation and Evolution 3/7

... the Be decays  slows up reaction Larger electric repulsion than p-p as larger electric charge (2 for He and 4 for Be). Therefore need about 100,000,000 degrees K for He burning  Stars like our Sun remain main sequence longer due to this PHYS 162 ...
Lecture 8a Star Formation 10/15/2014
Lecture 8a Star Formation 10/15/2014

Photoelectric Photometry of the Pleiades
Photoelectric Photometry of the Pleiades

... The computer program you will use is a realistic simulation of a UBV photometer attached to a moderate sized research telescope. The telescope is controlled by a computer that allows you to move from star to star and make measurements. Different filters can be selected for each observation, and the ...
Drawing Constellations
Drawing Constellations

Characteristics of Stars
Characteristics of Stars

... Enrich ...
MS Word version
MS Word version

... Question 6: Set the simulator up for an observer at the south pole. Make sure that there are still stars (~20) in the simulator and click animate continuously. Describe the circumpolar stars seen from the south pole. ...
OUR COSMIC NEIGHBORS Story of the Stars
OUR COSMIC NEIGHBORS Story of the Stars

... Polaris is of the third magnitude in brightness and is 250 light-years distant. Polaris is actually 4 stars when seen with larger telescopes. Polaris is called our Pole Star because it is very nearly over the northern axis of the earth—there being a difference of 11/2 degrees. ...
Galaxies, Cosmology and the Accelera`ng Universe
Galaxies, Cosmology and the Accelera`ng Universe

Whiteq
Whiteq

... dwarf yet discovered is type K. No type M stars have been found. This has implications for the age of the universe, since the coolest white dwarves are believed to be the remains of the first stars formed. There may be no class M white dwarves, because no stars have yet had time to cool that much. T ...
Virtual HR Diagram Lab
Virtual HR Diagram Lab

... Draw an arrow showing the direction of increasing mass for main sequence stars on the diagram. Label it M. (Note: this arrow only applies to main sequence stars, but that is over 90% of stars.) ...
Properties of Supernovae
Properties of Supernovae

... Supernova explosions are the most powerful events in the Universe. In less than a second, about 1044 Joules of energy are released---about the same as the Sun has released in its entire lifetime! The explosion results from the death of a massive star which has consumed its entire fuel supply. The ap ...
Today: Magnitude Terminology Photometry Applications Reading
Today: Magnitude Terminology Photometry Applications Reading

... the same object obtained in different filters, usually defined  to that larger positive color index indicates a redder object  ...
Lecture 11: Stars, HR diagram.
Lecture 11: Stars, HR diagram.

... The Main Sequence: summary ...
Theory of Massive Star Formation
Theory of Massive Star Formation

Pallavicini - IASF Milano
Pallavicini - IASF Milano

... • The X-ray emission of late-type stars in clusters is in fact a strong function of magnetic activity as measured e.g. by the Rossby number (a combination of rotation and convection zone properties) • Since late-type stars suffer magnetic braking during their evolutionary history, coronal activity i ...
Determining the Sizes of Stars Using the HR Diagram
Determining the Sizes of Stars Using the HR Diagram

Hertzsprung-Russell Diagrams
Hertzsprung-Russell Diagrams

... different radii stars. ...
Investigating Supernova Remnants - Chandra X
Investigating Supernova Remnants - Chandra X

Oct 06, 2001
Oct 06, 2001

... 13. Which of the statements below is true regarding the two stars marked α and β? A. Star α is hotter than star β. B. Star α is less luminous than star β. C. Star α is larger in radius than star β. D. Star α appears brighter that star β. 14. Which of the statements below is true regarding the two st ...
chapter 2
chapter 2

... known as constellations. These pictures may be of natural objects or characters from mythology. Fig 2.2.2 shows some constellations that can be seen in the sky in the months of February and March around 8 p.m. in the night. ...
Lecture 6: Stellar Distances and Brightness
Lecture 6: Stellar Distances and Brightness

... The light year (ly) is an alternative unit of distance “1 light year is the distance traveled by light in one year” 1 ly is equivalent to ...
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Corona Borealis

Corona Borealis /kɵˈroʊnə bɒriˈælɨs/ is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means ""northern crown"". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from our Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.
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