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User:Davidbuddy9/Gliese 581 d

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Gliese 581 d
Size comparison of Gliese 581 d with Earth and Neptune.
(Based on selected hypothetical modeled compositions)
Discovery
Discovery siteLa Silla Observatory, Chile
Radial velocity
Orbital characteristics
Epoch JD 2451409.762[1]
0.21847 ± 0.00028[1]
Eccentricity0[1]
66.87 ± 0.13[1]
56 ± 27[1]
StarGliese 581
Physical characteristics
Mass0.31

Gliese 581 d /ˈɡliːzə/ or Gl 581 d is a proposed extrasolar planet orbiting the star Gliese 581 approximately 20.2 light-years[3] away in the constellation of Libra. It was the third planet claimed in the system and (assuming a six-planet model) the fifth in order from the star.

Though not confirmed to be a terrestrial planet and significantly more massive than Earth (at 6.98 Earth masses),[3] the Super-Earth is the first exoplanet of terrestrial mass proposed to orbit within the habitable zone of its parent star.[5]

Assuming its existence, computer climate simulations have confirmed the possibility of the existence of surface water and these factors combine to a relatively high measure of planetary habitability. It would have an Earth Similarity Index of 0.82.[3]

A study in 2014 concluded that Gliese 581 d is "an artifact of stellar activity which, when incompletely corrected, causes the false detection of planet g."[6][7]

A 2014 study study by Paul Robertson, Suvrath Mahadevan, Michael End, and Arpita Roy concluded that the planet is could possibly exist after all, but Gliese 581 g's existence depends on Gliese 581 d's eccentricity.[8]

A 2015 study by Dr Guillem Anglada-Escudé concluded that the planet exists and is significant that is does exist because it was the first Earth-like planet found that would still be in the potentailly habitable catagory.[9]

Proposed discovery

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A team of astronomers led by Stéphane Udry of the Geneva Observatory used the HARPS instrument on the European Southern Observatory 3.6 meter telescope in La Silla, Chile to discover the planet in 2007. Udry's team employed the radial velocity technique, in which the mass of a planet is determined based on the small perturbations it induces in its parent star’s orbit via gravity.[10]

In September 2012, Roman Baluev filtered out the "red noise" from the Keck data and concluded that this planet's existence is probable only to 2.2 standard deviations.[4]

That same year, however, a team from the USNO confirmed the existence of the planet with a much higher probability. [11]

Orbital characteristics

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Gliese 581 d orbits Gliese 581 at 0.21847 AU, approximately a fifth of the distance that the Earth orbits the Sun, though its orbital eccentricity has not been confirmed. There are currently two models for its orbit, a circular one like Earth's, and an eccentric one like Mercury's. These are based on the four planet and six planet model for the Gliese 581 system, respectively. Under the four planet model Gliese 581 d would most probably be in a spin-orbit resonance of 2:1, rotating twice for each orbit of its parent star. Therefore the day on Gliese 581 d should approximately be 67 Earth’s days long.[11][12]

The orbital distance places it at the outer limits of the habitable zone, the distance at which it is believed possible for water to exist on the surface of a planetary body. At the time of its discovery, the planet's orbit was originally believed to be farther out, however in late April 2009 the original discovery team revised its original estimate of the planet's orbital parameters, finding that it orbits closer to its star than originally believed with an orbital period of 66.87 days. They concluded that the planet is within the habitable zone where liquid water could exist.[13][14] However, data [15] also suggests that the proposed exoplanet [16] could have at least one[17] or more large oceans.

Physical characteristics

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The motion of the parent star indicates a minimum mass for Gliese 581 d of 5.6 Earth masses (earlier analyses gave higher values).[1] Dynamical simulations of the Gliese 581 system assuming that the orbits of the three planets are coplanar show that the system becomes unstable if the masses of the planets exceed 1.6 – 2 times the minimum values. Using earlier minimum mass values for Gliese 581 d, this implies an upper mass limit for Gliese 581 d of 13.8 Earth masses.[13] The composition of the planet, however, is not known.

Climate and habitability

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The habitable zone of Gliese 581 compared with our Solar System's habitable zone, showing Gliese 581 d near the outer edge

As the planet is not known to transit from Earth and atmospheric conditions are not observable with current technology, no atmosphere for the planet has been confirmed to date. As such, all climate predictions for the planet are based on predicted orbits, computer modelling of theoretical atmospheric conditions.

Because Gliese 581 d was believed to orbit outside the habitable zone of its star it was originally thought to be too cold for liquid water to be present. With the 2009 revised orbit, climate simulations conducted by researchers in France in 2011 indicated possible temperatures suitable for surface water at sufficient atmospheric pressure[5] According to Stéphane Udry, "It could be covered by a 'large and deep ocean'; it is the first serious ocean planet candidate."[18]

On average, the light that Gliese 581 d receives from its star has about 30% of the intensity of light the Earth receives from the Sun. By comparison, sunlight on Mars has about 40% of the intensity of that on Earth. That might seem to suggest that Gliese 581 d is too cold to support liquid water and hence is inhospitable to life. However, an atmospheric greenhouse effect can significantly raise planetary temperatures. For example, Earth's own mean temperature would be about −18 °C[19] without any greenhouse gases, ranging from around 100 °C on the day side to −150 °C at night, much like that found on the Moon. If the atmosphere of Gliese 581 d produces a sufficiently large greenhouse effect, and the planet's geophysics stabilize the CO2 levels (as Earth's does via plate tectonics), then the surface temperature might permit a liquid water cycle, conceivably allowing the planet to support life.[20][21][22][23] Calculations by Barnes et al. suggest, however, that tidal heating is too low to keep plate tectonics active on the planet, unless radiogenic heating is somewhat higher than expected.[24]

Gliese 581 d is probably too massive to be made only of rocky material. It may have originally formed on a more distant orbit as an icy planet that then migrated closer to its star.[25][26] Its equilibrium temperature is 181 Kelvin.

Messages from Earth

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Artist's impression of Gliese 581 d as a Super-Earth

In October 2008, members of the networking website Bebo beamed A Message From Earth, a high-power transmission at Gliese 581, using the RT-70 radio telescope belonging to the National Space Agency of Ukraine. This transmission is due to arrive in the Gliese 581 system's vicinity by the year 2029; the earliest possible arrival for a response, should there be one, would be in 2049.[27]

As part of the 2009 National Science Week celebrations in Australia, Cosmos Magazine launched a website called Hello From Earth to collect messages for transmission to Gliese 581d. The maximum length of the messages was 160 characters, and they were restricted to the English language. In total, 25,880 messages were collected from 195 countries around the world. The messages were transmitted from the DSS-43 70 m radio telescope at the Canberra Deep Space Communication Complex at Tidbinbilla, Australia on the 28th of August, 2009.[28]

See also

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References

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  1. ^ a b c d e f g Vogt, S. S. (2010). "THE LICK-CARNEGIE EXOPLANET SURVEY: A 3.1 M ⊕PLANET IN THE HABITABLE ZONE OF THE NEARBY M3V STAR GLIESE 581". The Astrophysical Journal. 723: 954–965. arXiv:1009.5733. doi:10.1088/0004-637X/723/1/954. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  2. ^ a b c "Gliese 581 (V* HO Lib -- Variable of BY Dra type)". SIMBAD Astronomical Database. Retrieved 2010-04-10.
  3. ^ a b c d e PHL's Exoplanets Catalog - Planetary Habitability Laboratory @ UPR Arecibo
  4. ^ a b Roman Baluev (2012). "The impact of red noise in radial velocity planet searches: Only three planets orbiting GJ581?". Monthly Notices of the Royal Astronomical Society. 429 (3): 2052–2068. arXiv:1209.3154. Bibcode:2013MNRAS.429.2052B. doi:10.1093/mnras/sts476.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  5. ^ a b Wordsworth, R. (2011). "Gliese 581D is the First Discovered Terrestrial-Mass Exoplanet in the Habitable Zone". The Astrophysical Journal. 733 (2): L48. arXiv:1105.1031. doi:10.1088/2041-8205/733/2/L48. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  6. ^ Robertson, Paul; Mahadevan, Suvrath; Endl, Michael; Roy, Arpita (3 July 2014). "Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581". Science (journal). 345 (6195): 440–444. arXiv:1407.1049. Bibcode:2014Sci...345..440R. doi:10.1126/science.1253253. PMID 24993348. Retrieved 8 July 2014.
  7. ^ Quenqua, Douglas (7 July 2014). "Earthlike Planets May Be Merely an Illusion". New York Times. Retrieved 8 July 2014.
  8. ^ http://www.sciencemag.org/content/345/6195/440
  9. ^ http://astronomynow.com/2015/03/09/reanalysis-of-data-suggests-habitable-planet-gj581d-really-does-exist/
  10. ^ "The HARPS search for southern extra-solar planets", S. Udry. X. Bonfils. X. Delfosse. T. Forveille. M. Mayor. C. Perrier. F. Bouchy. C. Lovis. F. Pepe. D. Queloz. J.-L. Bertaux. The Extrasolar Planets Encyclopaedia. April 4, 2007. Accessed June 10, 2011
  11. ^ a b Makarov, Valeri V.; et al. (2012). "Dynamical evolution and spin-orbit resonances of potentially habitable exoplanets. The case of GJ 581d". The Astrophysical Journal. 761 (2): 83. arXiv:1208.0814. Bibcode:2012ApJ...761...83M. doi:10.1088/0004-637X/761/2/83.
  12. ^ Heller, René; Barnes, Rory; Leconte, Jérémy. (August 2011). "Habitability of extrasolar planets and tidal spin evolution". Origins of Life and Evolution of Biospheres. Onlinefirst (6): 539–543. arXiv:1108.4347. Bibcode:2011OLEB...41..539H. doi:10.1007/s11084-011-9252-3. PMID 22139513.
  13. ^ a b M. Mayor, X. Bonfils, T. Forveille, X. Delfosse, S. Udry, J.-L. Bertaux, H. Beust, F. Bouchy, C. Lovis, F. Pepe, C. Perrier, D. Queloz, N. C. Santos (2009). "The HARPS search for southern extra-solar planets". Astronomy & Astrophysics. 507: 487–494. arXiv:0906.2780. doi:10.1051/0004-6361/200912172.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  14. ^ "Lightest exoplanet yet discovered". eso.org. 2009-04-21. Retrieved 2009-04-21.
  15. ^ R. Stewart, (2013). " First View of Gliese-581 d; A preliminary Surface Survey (Part-1). Publisher-(IJAAR), (Issue 2013). At-http://www.journals-of-science.com/5-feature-research-pap.html
  16. ^ STEWART, R., CELEBONOVIC, V., AGUIAR, O.A.,CHATZITHEODORIDIS, E., ACKERMAN, J., ROMAN, M.,ARTUSO, G., TRENTADUE, W., SAMADI, A., ARISTIZABAL,C.I.O. and others. Gliese 581d; Views of Its atmospheric, topographical, geological, and oceanic conditions (Part 2). Journal of The International Society of Peer Reviewers. Available at: http://www.stewart-research-consulting.com/8-astronomy.html . Which in summary shows its atmosphere geology topography and oceanic conditions.
  17. ^ AGUIAR, O.A., STEWART, R., ARTUSO, G., SAMADI, A., ARISTIZABAL, C.I.O., ACKERMAN, J.R., TRENTADUE, W. The (possible)conrmation of the First exo-oceans. Pluralidade 1: 82-95, 2013. At- http://www.pluralidade.info/Eindex.html .
  18. ^ "Lightest exoplanet yet discovered", European Southern Observatory. April 21, 2009. Accessed June 10, 2011
  19. ^ "Global Warming Frequently Asked Questions". Lwf.ncdc.noaa.gov. 2008-05-08. Retrieved 2009-01-18.
  20. ^ von Bloh, W.; et al. (2008). "Habitability of Super-Earths: Gliese 581c and 581d". Proceedings of the International Astronomical Union. 3: 503–506. arXiv:0712.3219. doi:10.1017/S1743921308017031.
  21. ^ "Centauri Dreams » Blog Archive » Gliese 581d: A Habitable World After All?". Centauri-dreams.org. 2007-12-13. Retrieved 2009-01-18.
  22. ^ Posted at 12:06 AM in Space Exploration (2007-06-15). "New 'Super Earth 2' Discovered in Constellation Libra". Dailygalaxy.com. Retrieved 2009-01-18.{{cite web}}: CS1 maint: numeric names: authors list (link)
  23. ^ Wordsworth, Robin; François Forget; Franck Selsis; Ehouarn Millour; Benjamin Charnay; Jean-Baptiste Madeleine (1970). "Gliese 581D is the First Discovered Terrestrial-Mass Exoplanet in the Habitable Zone". Astrophysical Journal Letters. 733 (2): L48. arXiv:1105.1031. doi:10.1088/2041-8205/733/2/L48.
  24. ^ Barnes, Rory; Jackson, Brian; Greenberg, Richard; Raymond, Sean N. (2009-06-09). "Tidal Limits to Planetary Habitability". The Astrophysical Journal. 700 (1): L30–L33. arXiv:0906.1785. Bibcode:2009ApJ...700L..30B. doi:10.1088/0004-637X/700/1/L30.
  25. ^ SPACE.com - Hopes Dashed for Life on Distant Planet
  26. ^ von Bloh, W.; Bounama, C.; Cuntz, M.; Franck, S. (2007). "The Habitability of Super-Earths in Gliese 581". Astronomy & Astrophysics. 476 (3): 1365–1371. arXiv:0705.3758. Bibcode:2007A&A...476.1365V. doi:10.1051/0004-6361:20077939.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  27. ^ "Zimbio Pilot - Gliese 581c". Zimbio.com. 2008-10-13. Retrieved 2009-04-23.
  28. ^ Jenkins, Simon (2009-08-28). "Earth sends 25,000 hellos to outer space". Brisbane Times. Retrieved 2009-09-16.
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