Extra Solar Planets
New Planets Discovered
Gliese 876 is a red dwarf star approximately 15 light-years away from Earth in the constellation of Aquarius. As of 2010, it has been confirmed that four extrasolar planets orbit the star. Two of the middle planets are similar to Jupiter, while the closest planet is thought to be similar to a small Neptune or a large terrestrial planet, and the outer planet has mass similar to Uranus. The orbits of all but the closest planet are locked in a rare three-body Laplace resonance.
Distance and visibility
Gliese 876 is located fairly close to our solar system.
According to astrometric measurements made by the Hipparcossatellite, the
star shows a parallax of 213.28 milliarcseconds, which corresponds to
a distance of 4.69 parsecs (15.3 ly). Despite being located so close to
Earth, the star is so faint that it is invisible to the naked eye and can
only be seen using a telescope.
Estimating the age and metallicity of cool stars is difficult due to the formation of diatomic molecules in their atmospheres, which makes the spectrum extremely complex. By fitting the observed spectrum to model spectra, it is estimated that Gliese 876 has a slightly lower abundance of heavy elements compared to the Sun (around 75% the solar abundance of iron). Based on chromospheric activity the star is likely to be around 6.5 to 9.9 billion years old, depending on the theoretical model used. However, the low rotational period of the star as well as its membership among the young disk population suggest that the star is between 0.15 billion years old.
Like many low-mass stars, Gliese 876 is a variable star. Its variable star designation is IL Aquarii and it is classified as a BY Draconis variable. Its brightness fluctuates by around 0.04 magnitudes. This type of variability is thought to be caused by large starspots moving in and out of view as the star rotates. Gliese 876 emits X-rays.
On June 23, 1998, an extrasolar planet was announced in orbit around Gliese 876 by two independent teams led by Geoffrey Marcy and Xavier Delfosse. The planet was designated Gliese 876 b and was detected by making measurements of the star's radial velocity as the planet's gravity pulled it around. The planet, around twice the mass of Jupiter, revolves around its star in an orbit taking approximately 61 days to complete, at a distance of only 0.208 AU, less than the distance from the Sun to Mercury.
Artist depiction of Gliese 876 d, a new Earth-like rocky planet discovered in orbit around star M dwarf Gliese 876 about 15 light years from Earth. Date 13 June 2005(2005-06-13) Source: National Science Foundation Author; Trent Schindler, National Science Foundation
Both of the system's Jupiter-mass planets are located in the 'traditional' habitable zone (HZ) of Gliese 876, which extends between 0.116 to 0.227 AU from the star.
On June 13, 2005, further observations by a team led by Rivera revealed a third planet in the system, inside the orbits of the two Jupiter-size planets. The planet, designated Gliese 876 d, was estimated to have a minimum mass only 5.88 times that of the Earth and may be a terrestrial planet.
In 2008, the system was used as a test case for the migration of 5 Earth-mass planets which had formed inside the orbit of the innermost gas giant of the system. If it formed at (in this test) 0.07 AU from the star, b's gravity would have pulled d into an eccentric orbit. That orbit then would have restabilised to its current location.
In January 2009, the mutual inclination between planets b and c was determined using a combination of radial velocity and astrometric measurements. The planets were found to be almost coplanar, with an angle of only 5.0+3.9?2.3° between their orbital planes. It is the first planetary system around a normal star to have mutual inclination between planets measured (previously the mutual inclination of the planets orbiting the pulsarPSR B1257+12 had been determined by measuring their gravitational interactions). Later measurements reduced the value of the mutual inclination, and in the latest four-planet models the incorporation mutual inclinations does not result in significant improvements relative to coplanar solutions.
On June 23, 2010, astronomers announced the discovery
of a fourth planet (designated Gliese
876 e) in a 1:2:4 Laplace resonance with Gliese 876 b and c. This is
the second known example of a Laplace resonance, the first being Jupiter's
Europa and Io. This discovery better constrains the mass
and orbital properties of the other three planets, including the high eccentricity
of the innermost planet. Numerical integration indicates that the coplanar,
four-planet system is stable for at least another billion years. This planetary
system comes close to a triple conjunction between the three outer planets
once per orbit of the outermost planet.
The Gliese 876 system Wikipedia Gliese 876
Smallest Exoplanet Found
By Jeremy McGovern
Although this exoplanet is the most earthlike extrasolar body yet detected, it is quite different from our home.
In this artist's rendition, the newly discovered planet is shown as a hot, rocky, geologically-active world glowing in the deep red light of its nearby parent star, the M dwarf Gliese 876. Trent Schindler, National Science
Astronomers have discovered more than 150 planets outside our solar system, ranging from 100 to 1,000 times Earth's mass. Today, astronomers announced the 155th exoplanet discovery. So far, this is the most earthlike planet found beyond the solar system.
At the National Science Foundation's headquarters in Arlington, Virginia, an ecstatic team spoke about the serendipitous discovery today. While carefully examining two Jupiter-size planets with the Keck Telescope in Hawaii, the team noticed a wobble that could not be accounted for by the two-planet model they used. Doppler measurements revealed an inner planet. It orbits Gliese 876, an M dwarf star about one-third of the Sun's mass.
"This planet answers an ancient question," says team leader Geoffrey Marcy. "Over 2,000 years ago, the Greek philosophers Aristotle and Epicurus argued about whether there were other earthlike planets. Now, for the first time, we have evidence for a rocky planet around a normal star."
Little is known about the exoplanet, such as its chemical composition or terrain. Team members do recognize it possesses dissimilarities to Earth. First, it is larger than our home planet. Although astronomers believe it could be 6 to 9 times Earth's mass, the team estimates it is 7.5 times larger. Since previously discovered exoplanets are much larger all bigger than Uranus, an ice-giant about 15 times Earth's mass astronomers would place this body in an "earthlike class size."
The exoplanet's orbit around its star is much shorter than Earth's orbit around the Sun. The body makes one trip around Gliese 876 in only 1.94 days. It is located about 2 million miles (3.2 million kilometers) from its star, compared to Earth's position about 93 million miles (150 million km) away.
Furthermore, the exoplanet is much hotter than Earth it's an oven, at 400º to 750º Fahrenheit (244º to 398º Celsius). While those who discovered the exoplanet believe these conditions could not support life, they have not ruled out the existence of water. The hot conditions also make it likely that the planet has not retained much gas, making the planet solid.
"We keep pushing the limits of what we can detect, and we're getting closer and closer to finding Earths," says team member Steven Vogt.
Team member Jack Lissauer admitted this exoplanet won't hold the title of "most earthlike" for long. Astronomers will study this model and search similar star-class systems for even smaller exoplanets. Scheduled for launch in 2007, NASA's Kepler mission is designed to detect earth-size exoplanets..
Found! Rocky world just like ours - Tuesday, 14 June 2005
|Gliese 876 b
is an extrasolar planet orbiting the red dwarf star Gliese 876. It completes
one orbit in approximately 61 days. Discovered in June 1998, Gliese 876
b was the first planet to be discovered orbiting a red dwarf star.
Gliese 876 c is an extrasolar planet orbiting the red dwarf star Gliese 876, taking about 30 days to complete an orbit. The planet was discovered in April 2001 and is the second planet in order of increasing distance from its star.
Gliese 876 d is an extrasolar planet approximately 15 light-years away in the constellation of Aquarius (the Water-bearer). The planet was the third planet discovered orbiting the red dwarf star Gliese 876. At the time of its discovery, the planet had the lowest mass of any known extrasolar planet apart from the pulsar planets orbiting PSR B1257+12. Due to this low mass, it can be categorized as a Super-Earth.
Like the majority of known extrasolar planets, Gliese
876 d was discovered by analysing changes in its star's radial velocity
as a result of the planet's gravity. The radial velocity measurements were
made by observing the Doppler shift in the star's spectral lines. At the
time of discovery, Gliese 876 was known to host two extrasolar planets,
designated Gliese 876 b and c, in a 2:1 orbital resonance. After the two
planets were taken into account, the radial velocity still showed another
period, at around two days. The planet, designated Gliese 876 d, was announced
on June 13, 2005 by a team led by Eugenio Rivera and was estimated to have
a mass approximately 7.5 times that of Earth.
Gliese 876 e is an extrasolar planet orbiting the star Gliese 876 in the constellation of Aquarius. It is in a 1:2:4 Laplace resonance with the planets Gliese 876 c and Gliese 876 b: for each orbit of planet e, planet b completes two orbits and planet c completes four. This configuration is the second known example of a Laplace resonance after Jupiter's moons Io, Europa and Ganymede.
Gliese 876 e has a mass similar to that of the planet
Uranus. Its orbit takes 124 days to complete, or roughly one third of a
year. While the orbital period is longer than that of Mercury around the
Sun, the lower mass of the host star relative to the Sun means the planet's
orbit has a slightly smaller semimajor axis. Unlike Mercury, Gliese 876
e has a nearly circular orbit with an eccentricity of 0.055 ± 0.012.
Home of J-Rod?
J-Rod: A class of EBE from the Zeta Reticulum area.
The J-Rod assocated with Dr Burisch was housed in a pressurized hydrogen
"Clean Sphere" at Level 5 of S4. He had a degenerative neurological condition.
The J-Rod is similar in appearance to that of the "grey" aliens recovered
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