Summer Triangle (Winter in the south hemisphere) Lyra
... brightest star in the sky. It is three times larger than our Sun, and 60 times more luminous. Vega was the first star to be photographed in the 1850's. It was also one of the first stars discovered to have a disk of proto-planetary dust orbiting around it, by the IRAS satellite in 1983. This discove ...
... brightest star in the sky. It is three times larger than our Sun, and 60 times more luminous. Vega was the first star to be photographed in the 1850's. It was also one of the first stars discovered to have a disk of proto-planetary dust orbiting around it, by the IRAS satellite in 1983. This discove ...
Slide 1 - Personal.psu.edu
... When looking at just a few atoms, the gravitational force is nowhere near strong enough to overcome the random thermal motion: ...
... When looking at just a few atoms, the gravitational force is nowhere near strong enough to overcome the random thermal motion: ...
Stellar Physics - Craigie High School
... The development of what we know about the Earth, Solar System and Universe is a fascinating study in its own right. From earliest times Man has wondered at and speculated over the ‘Nature of the Heavens’. It is hardly surprising that most people (until around 1500 A.D.) thought that the Sun revolved ...
... The development of what we know about the Earth, Solar System and Universe is a fascinating study in its own right. From earliest times Man has wondered at and speculated over the ‘Nature of the Heavens’. It is hardly surprising that most people (until around 1500 A.D.) thought that the Sun revolved ...
The Hertzsprung-Russell Diagram
... The orbital period comes from watching the stars, or the periodic variation of their velocity or brightness. To get orbital semimajor axis, you need either the parallax to a visual system or the velocity from a spectroscopic system. In a spectroscopic system, you only have a lower limit unless you k ...
... The orbital period comes from watching the stars, or the periodic variation of their velocity or brightness. To get orbital semimajor axis, you need either the parallax to a visual system or the velocity from a spectroscopic system. In a spectroscopic system, you only have a lower limit unless you k ...
Study Guide for the Comprehensive Final Exam
... Describe or identify changes in a star during its main sequence lifetime. Describe how shell fusion in a star causes the star to become giants. Identify the “ashes” of H-burning and He-burning Mass loss and Death of Low-Mass Stars Match the stage of the Sun’s future evolution with the mechanism of e ...
... Describe or identify changes in a star during its main sequence lifetime. Describe how shell fusion in a star causes the star to become giants. Identify the “ashes” of H-burning and He-burning Mass loss and Death of Low-Mass Stars Match the stage of the Sun’s future evolution with the mechanism of e ...
14-1 Reading Questions: Neutron Stars
... 1. A neutron star, containing a little more than _________ solar mass, compressed to a radius of about __________, can be left as a remnant after a type ______ supernova explosion. A neutron star’s density is so high that physicists calculate that this material is stable only as a __________________ ...
... 1. A neutron star, containing a little more than _________ solar mass, compressed to a radius of about __________, can be left as a remnant after a type ______ supernova explosion. A neutron star’s density is so high that physicists calculate that this material is stable only as a __________________ ...
EF Eri: Its White Dwarf Primary and L Dwarf Secondary
... nova, nova-like (IP). These binaries contain an accretion disk. • If the white dwarf has a ~10 to 250MG field --> Polar or AM Herculis type. These contain no accretion disk. ...
... nova, nova-like (IP). These binaries contain an accretion disk. • If the white dwarf has a ~10 to 250MG field --> Polar or AM Herculis type. These contain no accretion disk. ...
Sample Stellar Evolution TEST QUESTIONS
... 11. The Orion region contains young main sequence stars and an emission nebula. 12. The thermal motions of the atoms in a gas cloud can make it collapse to form a protostar. 13. The pressure of a gas generally depends on its temperature and its density. 14. Stars swell into giants when hydrogen is e ...
... 11. The Orion region contains young main sequence stars and an emission nebula. 12. The thermal motions of the atoms in a gas cloud can make it collapse to form a protostar. 13. The pressure of a gas generally depends on its temperature and its density. 14. Stars swell into giants when hydrogen is e ...
Neutron Stars
... Novae: white dwarf re-ignition in binary system • Nova is a faint star suddenly brightens by a factor of 104 to 108 over a few days or hours • It reaches a peak luminosity of about 105 Lsun • A nova is different from supernova (luminosity of 109 Lsun) • Material from an ordinary star in a close bin ...
... Novae: white dwarf re-ignition in binary system • Nova is a faint star suddenly brightens by a factor of 104 to 108 over a few days or hours • It reaches a peak luminosity of about 105 Lsun • A nova is different from supernova (luminosity of 109 Lsun) • Material from an ordinary star in a close bin ...
ASTR-264-Lecture
... moons. Solar systems, planets, moons, and asteroids and comets are all in it Nebula-an interstellar cloud of gas and/or dust Galaxy- a great island of stars in space, held together by gravity and orbiting a common center Universe-the sum total of all matter and energy; that is, everything within it ...
... moons. Solar systems, planets, moons, and asteroids and comets are all in it Nebula-an interstellar cloud of gas and/or dust Galaxy- a great island of stars in space, held together by gravity and orbiting a common center Universe-the sum total of all matter and energy; that is, everything within it ...