Russell Diagram
... • Supergiants -- cool, bright, red, large stars • Giants -- cool, bright red, less large stars • Main Sequence -- spans range from hot, bright stars to cool, dim stars. • White dwarfs -- hot, small, dim stars. ...
... • Supergiants -- cool, bright, red, large stars • Giants -- cool, bright red, less large stars • Main Sequence -- spans range from hot, bright stars to cool, dim stars. • White dwarfs -- hot, small, dim stars. ...
HERE
... The pulsations can be regular or irregular, ranging from more than a year to only a few hours between pulsations. The change in size by about 15% of their radius. For more info in Pulsating Variable Stars, you can visit: http://faculty.rmwc.edu/tmichalik/pulsvar.htm ...
... The pulsations can be regular or irregular, ranging from more than a year to only a few hours between pulsations. The change in size by about 15% of their radius. For more info in Pulsating Variable Stars, you can visit: http://faculty.rmwc.edu/tmichalik/pulsvar.htm ...
LAB #6 - GEOCITIES.ws
... of zero and an effective temperature of 10,000 degrees Kelvin [The Kelvin temperature scale is like the Celsius scale, but offset by 273. Thus something that is 273 Kelvins is 0 degrees Celsius.] PRE-LAB WARMUP QUESTION: A star gives out more blue light than yellow. Thus its B-V is (positive, negati ...
... of zero and an effective temperature of 10,000 degrees Kelvin [The Kelvin temperature scale is like the Celsius scale, but offset by 273. Thus something that is 273 Kelvins is 0 degrees Celsius.] PRE-LAB WARMUP QUESTION: A star gives out more blue light than yellow. Thus its B-V is (positive, negati ...
formation of stars
... (b) A nova [new star] forms from a white dwarf that has flared up brilliantly, brightening a hundred a hundred to a million times. A nova may be the result of the bombardment by a companion star. Novas fade to their former luminosity in a few years at most. (c) The sun is thought to be 5 billion yea ...
... (b) A nova [new star] forms from a white dwarf that has flared up brilliantly, brightening a hundred a hundred to a million times. A nova may be the result of the bombardment by a companion star. Novas fade to their former luminosity in a few years at most. (c) The sun is thought to be 5 billion yea ...
Final Exam Earth science
... sunspot-areas of gas on the sun that are cooler than the gases around them 9. The name of our galaxy is the Milky Way. It is a spiral galaxy, which means it has spiral arms radiating out from a center. It contains lots of dust and gases. ...
... sunspot-areas of gas on the sun that are cooler than the gases around them 9. The name of our galaxy is the Milky Way. It is a spiral galaxy, which means it has spiral arms radiating out from a center. It contains lots of dust and gases. ...
The Hidden Lives of Galaxies NSTA 2001
... • Gravitational attraction of Clumps attracts more material. • Contraction causes Temperature and Pressure to slowly increase. ...
... • Gravitational attraction of Clumps attracts more material. • Contraction causes Temperature and Pressure to slowly increase. ...
Stars - Montville.net
... 10. When a supergiant runs out of fuel it can suddenly explode. This explosion is called a super nova. ...
... 10. When a supergiant runs out of fuel it can suddenly explode. This explosion is called a super nova. ...
April - Bristol Astronomical Society
... Constellation of the Month catalogue, “It is double, each has a bright centre, which are separated 4'35". The two atmospheres touch each other; the one is even fainter than the other.” This galaxy was the first one where the spiral structure was discovered, in spring 1845 by Lord Rosse, who made a ...
... Constellation of the Month catalogue, “It is double, each has a bright centre, which are separated 4'35". The two atmospheres touch each other; the one is even fainter than the other.” This galaxy was the first one where the spiral structure was discovered, in spring 1845 by Lord Rosse, who made a ...
Seasonal Motion
... They move from East to West and also from near to the horizon to higher up in the sky ...
... They move from East to West and also from near to the horizon to higher up in the sky ...
Topic E: Astrophysics
... ellipses and moons orbit planets. (Details of Kepler’s laws are not required.) Students should also know the names of the planets, their approximate comparative sizes and comparative distances from the Sun, the nature of comets, and the nature and position of the asteroid belt. ...
... ellipses and moons orbit planets. (Details of Kepler’s laws are not required.) Students should also know the names of the planets, their approximate comparative sizes and comparative distances from the Sun, the nature of comets, and the nature and position of the asteroid belt. ...
MULTIPLE CHOICE. Choose the one alternative that best
... A) mass on the horizontal axis and luminosity on the vertical axis B) surface temperature on the horizontal axis and radius on the vertical axis C) mass on the horizontal axis and stellar age on the vertical axis D) interior temperature on the horizontal axis and mass on the vertical axis E) surface ...
... A) mass on the horizontal axis and luminosity on the vertical axis B) surface temperature on the horizontal axis and radius on the vertical axis C) mass on the horizontal axis and stellar age on the vertical axis D) interior temperature on the horizontal axis and mass on the vertical axis E) surface ...
Star Life Guided Notes
... star _________ yet…. Expanded surface is actually “_______” so appears _____ ...
... star _________ yet…. Expanded surface is actually “_______” so appears _____ ...
Stars - Lauer Science
... Small stars use up their Hydrogen slower than large stars. Small stars can live for up to 200 billion years. Medium stars (sun) live for about 10 billion years. Larger stars can live for a few million years. ...
... Small stars use up their Hydrogen slower than large stars. Small stars can live for up to 200 billion years. Medium stars (sun) live for about 10 billion years. Larger stars can live for a few million years. ...
10 September: Faint Stars and Bright Stars
... Absolute Magnitude: a measure of the intrinsic brilliance of a star • Pick a star (any star) • Imagine moving it to a distance of 10 parsecs • The apparent magnitude it would have is its absolute magnitude • The absolute magnitude is a distanceindependent quantity • Look at Appendix 12 and Appendix ...
... Absolute Magnitude: a measure of the intrinsic brilliance of a star • Pick a star (any star) • Imagine moving it to a distance of 10 parsecs • The apparent magnitude it would have is its absolute magnitude • The absolute magnitude is a distanceindependent quantity • Look at Appendix 12 and Appendix ...
Chapter 21
... within the next 100,000 years. Even at its relatively remote distance, it normally ranks as the tenth brightest star in the sky. ...
... within the next 100,000 years. Even at its relatively remote distance, it normally ranks as the tenth brightest star in the sky. ...
Ursa Minor
Ursa Minor (Latin: ""Smaller She-Bear"", contrasting with Ursa Major), also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the name Little Dipper. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor has traditionally been important for navigation, particularly by mariners, due to Polaris being the North Star.Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging from apparent magnitude 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and magnitude 3 Gamma Ursae Minoris have been called the ""guardians of the pole star"". Planets have been detected orbiting four of the stars, including Kochab. The constellation also contains an isolated neutron star—Calvera—and H1504+65, the hottest white dwarf yet discovered with a surface temperature of 200,000 K.