Wanderlust
10-24-2010, 05:59 PM
A post to spotlight the star System Gliese 667 ABC!! I have an intrest spike in it right now and I want to share it!! (as you may know Alpha Centuari is a triple system as well, though the third star is .2 ly away from the main 2)
I made a short youtube video for my channel.
Gliese A and B go around each other while C goes around A and B. There is a confirmed Super Earth around planet C.
Gliese 667 (also HR 6426 and MLO 4) is a triple star system in the constellation of Scorpius (http://en.wikipedia.org/wiki/Scorpius). The star system lies at a distance of about 6.97 pc (http://en.wikipedia.org/wiki/Parsec) (22.7 ly (http://en.wikipedia.org/wiki/Light_year)). There is a 12th magnitude star close to the other three, but it is not gravitationally bound to the system. To the naked eye, the system appears to be a single faint star of magnitude 5.89.
The system has a relatively high proper motion, exceeding 1 second of arc per year.
The two brightest components, Gl 667 A and Gl 667 B, are separated by an average distance of about 12.6 AU (http://en.wikipedia.org/wiki/Astronomical_unit), but have an eccentric orbit, which takes them as close as about 5 AU, or as far as 20 AU. The orbit takes approximately 42.15 years to complete. The orbital distance translates to an average separation of 1.8" (http://en.wikipedia.org/wiki/Arcsecond).
Gl 667 C orbits further out, between about 56 and 215 AU, equating to an angular separation of about 30".
Gliese 667 A
Gliese 667 A is an orange dwarf star of spectral class (http://en.wikipedia.org/wiki/Stellar_classification) K3V. The star has a lower concentration of heavy elements (metals) than the Sun (http://en.wikipedia.org/wiki/Sun). The star has a mass of around 75% of that of the Sun and a luminosity of around 12 or 13% of that of the Sun. The apparent magnitude (http://en.wikipedia.org/wiki/Apparent_magnitude) is 6.29, giving an absolute magnitude (http://en.wikipedia.org/wiki/Absolute_magnitude) of around 7.07.
Gliese 667 B
Gliese 667 B is an orange dwarf star of spectral class K5V, with a mass of about 65% of that of the Sun, and only about 5% of the Sun's luminosity. The apparent magnitude is 7.24, giving an absolute magnitude (http://en.wikipedia.org/wiki/Absolute_magnitude) of around 8.02.
Gliese 667 C
Gliese 667 C is a red dwarf star of spectral class of M2V. It has a mass of around 38% of that of the Sun and only 0.3% of the Sun's luminosity. The apparent magnitude is 10.25, giving an absolute magnitude of around 11.03.
The Planet around Gliese C
Gliese 667 Cb is an extrasolar planet (http://en.wikipedia.org/wiki/Extrasolar_planet) which orbits Gliese 667 C. This planet has at least 5.7 times the mass of Earth (http://en.wikipedia.org/wiki/Earth) (classifying as super-Earth (http://en.wikipedia.org/wiki/Super-Earth)) and takes a week to orbit the star at a semimajor axis (http://en.wikipedia.org/wiki/Semimajor_axis) of approximately 0.05 AU (http://en.wikipedia.org/wiki/Astronomical_unit). This planet was announced by HARPS (http://en.wikipedia.org/wiki/HARPS) on October 19, 2009, together with 29 other planets. No discovery paper has yet been made available.
http://www.youtube.com/watch?v=joBbHq5KBN4
In this image A and B are in the distnace while C is off screen to the left.
http://www.avatar-forums.com/images/imported/2010/10/317.jpg (http://upload.wikimedia.org/wikipedia/commons/7/72/Gliese_667.jpg)
I made a short youtube video for my channel.
Gliese A and B go around each other while C goes around A and B. There is a confirmed Super Earth around planet C.
Gliese 667 (also HR 6426 and MLO 4) is a triple star system in the constellation of Scorpius (http://en.wikipedia.org/wiki/Scorpius). The star system lies at a distance of about 6.97 pc (http://en.wikipedia.org/wiki/Parsec) (22.7 ly (http://en.wikipedia.org/wiki/Light_year)). There is a 12th magnitude star close to the other three, but it is not gravitationally bound to the system. To the naked eye, the system appears to be a single faint star of magnitude 5.89.
The system has a relatively high proper motion, exceeding 1 second of arc per year.
The two brightest components, Gl 667 A and Gl 667 B, are separated by an average distance of about 12.6 AU (http://en.wikipedia.org/wiki/Astronomical_unit), but have an eccentric orbit, which takes them as close as about 5 AU, or as far as 20 AU. The orbit takes approximately 42.15 years to complete. The orbital distance translates to an average separation of 1.8" (http://en.wikipedia.org/wiki/Arcsecond).
Gl 667 C orbits further out, between about 56 and 215 AU, equating to an angular separation of about 30".
Gliese 667 A
Gliese 667 A is an orange dwarf star of spectral class (http://en.wikipedia.org/wiki/Stellar_classification) K3V. The star has a lower concentration of heavy elements (metals) than the Sun (http://en.wikipedia.org/wiki/Sun). The star has a mass of around 75% of that of the Sun and a luminosity of around 12 or 13% of that of the Sun. The apparent magnitude (http://en.wikipedia.org/wiki/Apparent_magnitude) is 6.29, giving an absolute magnitude (http://en.wikipedia.org/wiki/Absolute_magnitude) of around 7.07.
Gliese 667 B
Gliese 667 B is an orange dwarf star of spectral class K5V, with a mass of about 65% of that of the Sun, and only about 5% of the Sun's luminosity. The apparent magnitude is 7.24, giving an absolute magnitude (http://en.wikipedia.org/wiki/Absolute_magnitude) of around 8.02.
Gliese 667 C
Gliese 667 C is a red dwarf star of spectral class of M2V. It has a mass of around 38% of that of the Sun and only 0.3% of the Sun's luminosity. The apparent magnitude is 10.25, giving an absolute magnitude of around 11.03.
The Planet around Gliese C
Gliese 667 Cb is an extrasolar planet (http://en.wikipedia.org/wiki/Extrasolar_planet) which orbits Gliese 667 C. This planet has at least 5.7 times the mass of Earth (http://en.wikipedia.org/wiki/Earth) (classifying as super-Earth (http://en.wikipedia.org/wiki/Super-Earth)) and takes a week to orbit the star at a semimajor axis (http://en.wikipedia.org/wiki/Semimajor_axis) of approximately 0.05 AU (http://en.wikipedia.org/wiki/Astronomical_unit). This planet was announced by HARPS (http://en.wikipedia.org/wiki/HARPS) on October 19, 2009, together with 29 other planets. No discovery paper has yet been made available.
http://www.youtube.com/watch?v=joBbHq5KBN4
In this image A and B are in the distnace while C is off screen to the left.
http://www.avatar-forums.com/images/imported/2010/10/317.jpg (http://upload.wikimedia.org/wikipedia/commons/7/72/Gliese_667.jpg)