OGLE-2005-BLG-390Lb

OGLE-2005-BLG-390Lb
Exoplanet List of exoplanets

Artist's impression of OLGE-2005-BLG-390Lb, one of the most distant exoplanets discovered.
Parent star
Star OGLE-2005-BLG-390L
Constellation Scorpius
Right ascension (α) 17h 54m 19.2s
Declination (δ) −30° 22′ 38″
Apparent magnitude (mV) 15.7
Distance21,500 ±3,300 ly
(6,600 ±1,000 pc)
Spectral type M4V
Mass (m) 0.22 M☉
Radius (r) ~0.16 R☉
Temperature (T) ~3000 K
Age 9.587[1] Gyr
Physical characteristics
Mass(m)5.5+5.5
−2.7 M⊕
Radius(r)1.69 R⊕
Temperature (T) 50 K (−220 °C; −370 °F)
Orbital elements
Semi-major axis(a) 2.0–4.1 AU
Orbital period(P) 3500 d
(~10 y)
Observed separation
Projected separation (d) 2.6 AU
Source-lens
closest approach		 (t0) 2,453,582.73 ± 0.005 JD
Angle of source motion (α) 157.9 ± 0.2°
Discovery information
Discovery date 10 August 2005
Discoverer(s) PLANET/RoboNet,
OGLE, MOA
Discovery method Gravitational microlensing
Discovery site La Silla Observatory
Discovery status Published
Other designations
EWS 2005-BUL-390Lb, EWS 2005-BLG-390Lb

OGLE-2005-BLG-390Lb (known sometimes as Hoth by NASA[2]) is a super-Earth exoplanet orbiting OGLE-2005-BLG-390L, a star 21,500 ± 3,300 light years from Earth near the center of the Milky Way. It is one of the most distant planets known. On 25 January 2006, Probing Lensing Anomalies NETwork/Robotic Telescope Network (PLANET/Robonet), Optical Gravitational Lensing Experiment (OGLE), and Microlensing Observations in Astrophysics (MOA) made a joint announcement of the discovery. The planet does not appear to meet conditions presumed necessary to support life.[3]

Characteristics

OGLE-2005-BLG-390L's location in the night sky

Mass, radius and temperature

The planet is estimated to be about five times Earth's mass (5.5+5.5
−2.7 M⊕). Some astronomers have speculated that it may have a rocky core like Earth, with a thin atmosphere. Its distance from the star, and the star's relatively low temperature, means that the planet's likely surface temperature is around 50 K (−220 °C; −370 °F), making it one of the coldest known. If it is a rocky world, this temperature would make it likely that the surface would be made of frozen volatiles, substances which would be liquids or gases on Earth: water, ammonia, methane and nitrogen would all be frozen solid. If it is not a rocky planet, it would more closely resemble an icy gas planet like Uranus, although much smaller.[4]

The planet is not so much notable for its size (which is estimated to be around 1.69 R⊕[5]), or possible composition—although these are unusual—but for the fact that such a relatively small exoplanet was detected at such a relatively large distance from its star. Prior to this, "small" exoplanets such as Gliese 876 d, which has a "year" of less than 2 Earth-days, were detected very close to their stars. OGLE-2005-BLG-390Lb shows a combination of size and orbit that would not make it out of place in the Solar System.

"The team has discovered the most Earthlike planet yet", said Michael Turner,[6] assistant director for the mathematical and physical sciences directorate at the National Science Foundation, which supported the work. At 5.5 Earth masses, the planet was less massive than the previous candidate for lowest-mass exoplanet around a main-sequence star, the 7.5 Earth mass Gliese 876 d. Since 2013, many Earth-sized or smaller planets around main-sequence stars have been detected by the Kepler spacecraft and others.

Host star

OGLE-2005-BLG-390L (located in the constellation Scorpius, RA 17:54:19.2, Dec −30°22′38″, J2000, 6.6 ± 1.0 kpc distance)[7] is thought to likely be a cool red dwarf (95% probability), or a white dwarf (4% probability), with a very slight chance that it is a neutron star or black hole (<1% probability). Regardless of the star's classification, its radiant energy output would be significantly less than that of the Sun. It has a mass of 0.22 M☉, but an unknown radius. If it is a red dwarf, it would likely have a radius of 0.17 R☉. The age is estimated to be around 9.587 billion years old.[1]

Orbit

OGLE-2005-BLG-390Lb orbits its star every 3,500 days (about 10 years) at an average distance of 2.0 to 4.1 AU, or an orbit that would fall between the orbits of Mars and Jupiter in the Solar System (This range of distances is the range of error in measurement and calculation; it does not represent the planet's orbital eccentricity, as its orbital elements are not known, other than its orbital period.). Until this discovery, no small exoplanet had been found farther than 0.15 AUs from a main-sequence star. The planet takes approximately 10 Earth years to orbit its star, OGLE-2005-BLG-390L.[7]

Discovery

An illustration of gravitational microlensing. Light from a distant star is bent due to the gravitational field of an intervening foreground star and its orbiting planet, resulting in at least three (unresolved) distorted images. The change of their solid angle subtained on the sky corresponds to an observable brightening of the observed source star.

OGLE-2005-BLG-390Lb's signature was first detected on August 10, 2005 by observations at the Danish 1.54-m telescope at ESO La Silla Observatory in Chile. The telescope was part of a network of telescopes used by the PLANET/RoboNet gravitational microlensing campaign. Much of the follow-up observational data was gathered by a 0.6-m telescope at the Perth Observatory in Western Australia.

Gravitational lensing occurs when light from a distant star is bent and magnified by the gravitational field of a foreground star. A gravitational microlensing event occurs when a planet accompanying this foreground star can cause an additional small increase in the intensity of magnified light as it passes between the background star and the observer as well.

The PLANET/RoboNet campaign regularly investigates promising microlensing event alerts that are issued by the Polish OGLE or the Japanese–New Zealand MOA survey.[8] The observation of just such an event led to the discovery of OGLE-2005-BLG-390Lb. OGLE detected the microlensing effect produced by the star OGLE-2005-BLG-390L, and it was the PLANET team's follow-up observations and analysis which uncovered evidence of the planet itself.

The PLANET team conducted close observation of the OGLE-2005-BLG-390 microlensing event over a period of about two weeks. During this series of observations, a 15% "spike" in intensity occurred, lasting approximately 12 hours. From the intensity of the increase, and its length, the PLANET astronomers were able to derive the planet's mass, and its approximate displacement from the star.[3]

The paper submitted to Nature bears the names of all members of PLANET, RoboNet, OGLE, and MOA.

The planet has been given the unofficial name of Hoth by NASA due to its resemblance to the planet with the same name from the Star Wars franchise.[2]

See also

References

  1. 1 2 Safonova, M.; Murthy, J.; Shchekinov, Yu. A. (2014). "Age Aspects of Habitability". International Journal of Astrobiology. 15 (2): 93–105. arXiv:1404.0641Freely accessible. doi:10.1017/S1473550415000208.
  2. 1 2 Pat Brennan (15 December 2015). "8 planets that make you think Star Wars is real". NASA. Retrieved 26 July 2016.
  3. 1 2 PLANET collaboration (2006-01-26). "Discovery of OGLE 2005-BLG-390Lb, the first cool rocky/icy exoplanet". Retrieved 2006-06-11.
  4. ↑ "Discovery of OGLE 2005-BLG-390Lb, the first cool rocky/icy exoplanet". 25 January 2006..
  5. ↑ http://phl.upr.edu/projects/habitable-exoplanets-catalog/top10
  6. ↑ Henderson, Mark (2006-01-25). "Freezing cold Earth-like planet is discovered". Times Online.
  7. 1 2 Beaulieu, J.-P.; et al. (January 2006). "Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing". Nature. 439 (7075): 437–440. arXiv:astro-ph/0601563Freely accessible. Bibcode:2006Natur.439..437B. doi:10.1038/nature04441. PMID 16437108.
  8. ↑ Dominik, M.; et al. (2002). "The PLANET microlensing follow-up network: results and prospects for the detection of extra-solar planets". Planetary and Space Science. 50 (3): 299–307. Bibcode:2002P&SS...50..299D. doi:10.1016/S0032-0633(01)00126-X.
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Coordinates: 17h 54m 19s, −30° 22′ 38″

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