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 ...
... 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 ...
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 ...
... 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
... 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 ...
... 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 ...
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 ...
... 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 ...
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. ...
... 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
... 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. ...
... 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. ...
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 ...
... 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
... 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.) ...
... 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
... 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 ...
... 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
... the same object obtained in different filters, usually defined to that larger positive color index indicates a redder object ...
... the same object obtained in different filters, usually defined to that larger positive color index indicates a redder object ...
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 ...
... • 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 ...
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 ...
... 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
... 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. ...
... 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
... 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 ...
... 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 ...