The Death of Stars
... b. produced by a supernova explosion. c. produced by a nova explosion. d. a nebula within which planets are forming. e. a cloud of hot gas surround a planet 3. The Chandrasekhar limit tells us that a. accretion disks can grow hot through friction. b. neutron stars of more than 3 solar masses are not ...
... b. produced by a supernova explosion. c. produced by a nova explosion. d. a nebula within which planets are forming. e. a cloud of hot gas surround a planet 3. The Chandrasekhar limit tells us that a. accretion disks can grow hot through friction. b. neutron stars of more than 3 solar masses are not ...
Formation and Evolution of Infalling Disks Around Protostars
... Summary part2: Star Formation Triggered by First Supernovae Supernovae of first stars ...
... Summary part2: Star Formation Triggered by First Supernovae Supernovae of first stars ...
educator guide - Michigan Science Center
... The Sun is humanity’s star. It is classified as a G2V star (see stellar classification) along the main sequence. The Sun was once considered to be a fairly dim star compared to most other stars in the universe. Recent discoveries have shown, however, that there are many more red dwarf stars than exp ...
... The Sun is humanity’s star. It is classified as a G2V star (see stellar classification) along the main sequence. The Sun was once considered to be a fairly dim star compared to most other stars in the universe. Recent discoveries have shown, however, that there are many more red dwarf stars than exp ...
Positions in the Solar System
... The Universe contains billions of galaxies, each containing millions or billions of stars. Therefore, the galaxy in which our solar system and essentially all of us live, is just one of billions. ...
... The Universe contains billions of galaxies, each containing millions or billions of stars. Therefore, the galaxy in which our solar system and essentially all of us live, is just one of billions. ...
Habitable Zones around Evolved Stars
... Factors determining the location of the habitable zone in evolved stars • L changes dramatically as a star evolves beyond the main sequence • ap is altered by changing M* or in extreme cases by tidal or gas drag • The albedoratio depends on planetary atmosphere, surface properties, => and the stell ...
... Factors determining the location of the habitable zone in evolved stars • L changes dramatically as a star evolves beyond the main sequence • ap is altered by changing M* or in extreme cases by tidal or gas drag • The albedoratio depends on planetary atmosphere, surface properties, => and the stell ...
astronomy webquest…… explore the universe
... http://outreach.atnf.csiro.au/education/everyone/pulsars/ ...
... http://outreach.atnf.csiro.au/education/everyone/pulsars/ ...
Big idea # 5 * Earth in space in time
... Milky Way Galaxy – where our solar system is located ...
... Milky Way Galaxy – where our solar system is located ...
Slide 1
... The Universe contains billions of galaxies, each containing millions or billions of stars. Therefore, the galaxy in which our solar system and essentially all of us live, is just one of billions. ...
... The Universe contains billions of galaxies, each containing millions or billions of stars. Therefore, the galaxy in which our solar system and essentially all of us live, is just one of billions. ...
PPS
... The key discovery that led to the development of spectroscopy was made by the German physicist Josef von Fraunhofer (1787-1826) in 1814. He was the first person to study the rainbow pattern produced by passing light through a prism in detail under intense magnification. He was actually interested in ...
... The key discovery that led to the development of spectroscopy was made by the German physicist Josef von Fraunhofer (1787-1826) in 1814. He was the first person to study the rainbow pattern produced by passing light through a prism in detail under intense magnification. He was actually interested in ...
PSF - ESO
... The program starts off by considering the first input list as a "master" list. Taking each star in turn from the second input list, it applies the provisional transformations derived to determine the star's position in the coordinate system of the master list. It then goes through the master list, l ...
... The program starts off by considering the first input list as a "master" list. Taking each star in turn from the second input list, it applies the provisional transformations derived to determine the star's position in the coordinate system of the master list. It then goes through the master list, l ...
Note
... • The line opacity in the wings is significant compared to kn • Line strength depends (approximately) on the square root of the abundance ...
... • The line opacity in the wings is significant compared to kn • Line strength depends (approximately) on the square root of the abundance ...
document
... • Sum of all light emitted over all wavelengths is the luminosity – brightness per unit surface area – luminosity is proportional to T4: L = T4 Joules ...
... • Sum of all light emitted over all wavelengths is the luminosity – brightness per unit surface area – luminosity is proportional to T4: L = T4 Joules ...
The Southern Fall PDF - Treasures of the Southern Sky
... The cluster is rather more compact than the Jewel Box Cluster, and there are traces of blue reflection nebulosity associated with the brighter stars and the red emission nebula surrounding part of the cluster, which are both indications of youth. Open clusters such as NGC 3293 are excellent laborato ...
... The cluster is rather more compact than the Jewel Box Cluster, and there are traces of blue reflection nebulosity associated with the brighter stars and the red emission nebula surrounding part of the cluster, which are both indications of youth. Open clusters such as NGC 3293 are excellent laborato ...
Astronomy Glossary Key
... Astronomy is the study of space, including asteroids, planets, stars and galaxies. According to many astronomers, there just is not enough visible matter in the universe to explain how it behaves. This has lead them to believe there is more matter out there that cannot be seen. This is what they cal ...
... Astronomy is the study of space, including asteroids, planets, stars and galaxies. According to many astronomers, there just is not enough visible matter in the universe to explain how it behaves. This has lead them to believe there is more matter out there that cannot be seen. This is what they cal ...
The Sun - GeoScience
... 14. Diagram and label the positions of the Sun, Earth, and Moon during a Solar Eclipse. 15. When does a Total Solar Eclipse occur during the Moon’s phase cycle? Click on “Recent and Future Eclipses” under Related Links 16. What is the date of the next Eclipse that will be able to be seen from the W ...
... 14. Diagram and label the positions of the Sun, Earth, and Moon during a Solar Eclipse. 15. When does a Total Solar Eclipse occur during the Moon’s phase cycle? Click on “Recent and Future Eclipses” under Related Links 16. What is the date of the next Eclipse that will be able to be seen from the W ...
Q3.2.a The gravitational force exerted by a planet on one of its
... itself in a block of mass 0.50 kg that is sitting at rest on a very slippery sheet of ice. Which equation will correctly give the final speed vf_BLOCK of the block? 1) (0.04 kg)*(800 m/s) = (0.50 kg) *vf_BLOCK 1) (0.04 kg)*(800 m/s) = (0.04 kg) *vf_BLOCK 1) (0.04 kg)*(800 m/s) = (0.50 kg) *vf_BLOCK ...
... itself in a block of mass 0.50 kg that is sitting at rest on a very slippery sheet of ice. Which equation will correctly give the final speed vf_BLOCK of the block? 1) (0.04 kg)*(800 m/s) = (0.50 kg) *vf_BLOCK 1) (0.04 kg)*(800 m/s) = (0.04 kg) *vf_BLOCK 1) (0.04 kg)*(800 m/s) = (0.50 kg) *vf_BLOCK ...
The Sculptor dwarf irregular galaxy SDIG: present and past
... galactic H I (Burstein & Heiles 1984). Given that SDIG is more than 10° away from the Sculptor dwarf spheroidal, a direct measurement is preferable. Thus, the authors adopt the RC3 value, namely E(B - v)gal = 0.00 mag. The internal extinction in SDIG is unknown. Based on model fits to optical surfac ...
... galactic H I (Burstein & Heiles 1984). Given that SDIG is more than 10° away from the Sculptor dwarf spheroidal, a direct measurement is preferable. Thus, the authors adopt the RC3 value, namely E(B - v)gal = 0.00 mag. The internal extinction in SDIG is unknown. Based on model fits to optical surfac ...
Slide 1
... Estimates of planetary numbers still varies widely from team to team. However, all are suggesting that planets are common… Analyses of Kepler data suggest that stars in the galaxy have, on average, 1.6 planets. Therefore, about 160 billion planets exist in the galaxy. 500 million of these planets ma ...
... Estimates of planetary numbers still varies widely from team to team. However, all are suggesting that planets are common… Analyses of Kepler data suggest that stars in the galaxy have, on average, 1.6 planets. Therefore, about 160 billion planets exist in the galaxy. 500 million of these planets ma ...
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.