HD 85512 b
|Exoplanet||List of exoplanets|
|Right ascension||(α)||09h 51m 07.1s|
|Declination||(δ)||−43° 30′ 10″|
(11.1 ± 0.1 pc)
|Radius||(r)||0.533 (± 0.04)[note 1] R☉|
|Temperature||(T)||4715 (± 102) K|
|Metallicity||[Fe/H]||−0.33 (± 0.03)|
|Age||5.61 (± 0.61) Gyr|
|Minimum mass||(m sin i)||3.6 (± 0.5) M⊕|
|Stellar flux||(F⊙)||1.85 ⊕|
|Temperature||(T)||298 K (25 °C; 77 °F)|
|Semi-major axis||(a)||(0.26 ± 0.005) AU|
|Eccentricity||(e)||(0.11 ± 0.1)|
|Orbital period||(P)||54.43 (± 0.13) d|
|Orbital speed||(υ)||94.913 ± 0.038 km/s|
|Discovery date||August 17, 2011|
|Discoverer(s)||Pepe et al.|
|Discovery method||Radial velocity (HARPS)|
|Discovery site||La Silla Observatory|
|Open Exoplanet Catalogue||data|
Due to its mass of at least 3.6 times the mass of Earth, HD 85512 b is classified as a rocky Earth-size exoplanet (<5M⊕) and is one of the smallest exoplanets discovered to be just outside the inner edge of the habitable zone. HD 85512 b, along with Gliese 581 d, was once considered to be one of the best candidates for habitability in 2011.
Mass, radius and temperature
The planet has a minimum Earth mass of 3.6 ± 0.5, minimum surface gravity of about 1.4 g and assuming an atmosphere like Earth's despite its far greater mass, an estimated temperature of 298 K (24.85 °C or 76.73 °F) at the top of its atmosphere. The estimated temperature is noted to be similar to temperatures in Southern France, but various atmospheric conditions prevalent in the planet have to be analyzed to estimate the temperature of the surface. An estimated radius of 1.3 R⊕ is possible based on its mass.
The planet orbits a (K-type) star named HD 85512. The star has a mass of 0.69 M☉ and a radius of around 0.53 R☉. It has a surface temperature of 4715 K and is 5.61 billion years old. In comparison, the Sun is about 4.6 billion years old and has a surface temperature of 5778 K.
The star's apparent magnitude, or how bright it appears from Earth's perspective, is 7.43 Therefore, HD 85512 is too dim to be seen with the naked eye, but can be viewed using good binoculars.
Habitability and climate
Models generated by Pepe et al (2011) suggest that for the temperature to be below 270 K (-3.15 °C), for a circular orbit, the planetary albedo should be 0.48 ± 0.05 and for an eccentricity of 0.11, the planetary albedo should be 0.52. If the planet has 50% cloud cover, water may exist in liquid form on the planet provided its atmosphere is similar to our own, thus increasing the planet's habitability potential. Also, if the albedo of the planet is increased due to cloud cover, water could be present in its liquid form on the planet, which would mean that the planet is on the edge of the habitability zone.
However, PHL's new definition of the circumstellar habitable zone classifies this planet in the "too hot" zone, and it considers the planet "not habitable".
The planet would likely be inhospitable because of a runaway greenhouse effect on its surface. Any oceans on its surface would have boiled away due to the high stellar flux, and as this occurred, the temperature would have risen to around 322 K (49 °C; 120 °F). The water vapor would have accumulated in the atmosphere to the point where the surface temperature would rise to around 500 K (227 °C; 440 °F) as the planet would have been overwhelmed by water vapor—a powerful greenhouse gas. Little amounts of carbon dioxide would have been present, as HD 85512 b was probably an ocean planet (with little to no landmasses) very shortly after its star was formed into the main sequence, before the stellar flux increased to its estimated present state. The surface pressure would have also increased to about 100 times Earth's surface pressure (100 kilopascals, 100 atm) because of the amount of water vapor in the atmosphere. Thus, HD 85512 b is likely a desert planet rather than an ocean planet because of the increased stellar flux.
HD 85512 b was discovered by scientists at University of Geneva, Switzerland, led by Swiss astronomer Stéphane Udry of the Guaranteed Time Observations (GTO) program of High Accuracy Radial velocity Planet Searcher (HARPS), a high-precision echelle spectrograph installed on ESO's 3.6 m telescope at La Silla Observatory in Chile. The team used the Doppler spectroscopy technique which determines the minimum mass of the planet through slight changes in motion of the parent star. It was discovered on August 17, 2011.
On August 17, 2011, researchers released a study of the planet. The study makes assumptions about the planet actually having the minimum mass allowed by existing observations, not being tidally locked, and having one specific composition out of the wide parameter set available to conclude that HD 85512 b is the most habitable exoplanet discovered up to that point and one of the most stable exoplanets discovered by the High Accuracy Radial Velocity Planet Searcher.
Possibility as target for interstellar probe
- Carbon planet
- Circumstellar habitable zone
- Earth analog
- Gliese 581 d
- Gliese 581 g
- Gliese 667 Cc
- Habitable zone
- Kepler 22 b
- Planetary habitability
|Wikimedia Commons has media related to HD 85512.|
- Pepe, F; et al. (2011). "The HARPS search for Earth-like planets in the habitable zone: I – Very low-mass planets around HD20794, HD85512 and HD192310". arXiv: . Bibcode:2011yCat..35349058P. doi:10.1051/0004-6361/201117055.
- Kaltenegger, L; Udry, S; Pepe, F (2011). "A Habitable Planet around HD 85512?". arXiv: . Bibcode:2011arXiv1108.3561K.
- "HARPS: Hunting for Nearby Earth-like Planets". centauri-dreams.org. Retrieved 2011-08-25.
- "Researchers find potentially habitable planet" (in French). maxisciences.com. Retrieved 2011-08-31.
- "Italian helps find planet that could sustain life". La Gazzetta del Mezzogiorno. September 2, 2011. Retrieved September 7, 2011.
- Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 19 February 2011.
- Fraser Cain (September 15, 2008). "Temperature of the Sun". Universe Today. Retrieved 19 February 2011.
- "Super Earth circulating in ekosferze?" (in Polish). technologie.gazeta.pl. Retrieved 2011-08-31.
- "Found a planet where life could exist" (in Lithuanian). maxisciences.com. Retrieved 2011-08-31.
- "Exoplanet Looks Potentially Lively". scientificamerican.com. Retrieved 2011-08-25.
- "Is There A Habitable Planet Circling HD 85512?". spaceref.com. Retrieved 2011-08-31.
- "The World's Top 12 Fastest Vehicles". Popular Mechanics.
- From , where is the radius, is the luminosity, is the effective surface temperature and is the Stefan–Boltzmann constant.