Biography:Mikko Tuomi

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Short description: Finnish astronomer
Mikko Tuomi
Born
Espoo, Finland [1]
CitizenshipFinland
Alma materUniversity of Turku
Known for
Scientific career
InstitutionsUniversity of Turku
University of Hertfordshire
ThesisMultidata inverse problems and Bayesian solution methods in astronomy (2013)
Doctoral advisorHarry Lehto
Esko Valtaoja
InfluencesEsko Valtaoja[1]

Mikko Tuomi is a Finnish astronomer from the University of Hertfordshire, most known for his contributions to the discovery of a number of exoplanets, among them the Proxima Centauri b which orbits the closest star to the Sun. Mikko Tuomi was the first to find indications of the existence of Proxima Centauri b in archival observation data.[2] Other exoplanets to whose discovery or study Tuomi has contributed include HD 40307,[3] HD 154857 c,[4] Kapteyn c,[5] Gliese 682 c,[6] HD 154857,[4] Gliese 221,[7] Gliese 581 g[8] and the planetary system orbiting Tau Ceti.[9] He has led the development of new data analysis techniques for distinguishing observations caused by natural activity of the star and those caused by planets orbiting them.[10]

Publications

Mikko Tuomi has contributed to many cosmologist research articles including:

  • "A Super-Earth in the Habitable Zone"[11]
  • "Two planets around Kapteyn's star: A cold and a temperate super-Earth orbiting the nearest halo red dwarf"[12]
  • "Bayesian search for low-mass planets around nearby M. draws. Estimates for occurrence rate based on global detestability statistics"[13]
  • "A dynamically-packed planetary system around GJ667C with three super-Earths in its habitable zone"[14]

Discoveries

Mikko Tuomi helped discover the Proxima Centauri b planet by observing the gravitational tug of Proxima Centauri's star, Proxima Centauri.[2]

See also

References

  1. ↑ 1.0 1.1 Milla Ollikainen (February 10, 2017). "Elämää avaruudessa? Mikko Tuomi löysi planeetan" (in fi). https://seura.fi/viihde/julkkikset/elamaa-avaruudessa-mikko-tuomi-loysi-planeetan/. Retrieved February 21, 2020. 
  2. ↑ 2.0 2.1 Astronomer, Dr Sten Odenwald; Consortium, NASA Heliophysics Education (2016-08-26). "Proxima Centauri b: Earth-sized? Earth-like? Or Habitable?". http://www.huffingtonpost.com/dr-sten-odenwald/proxima-centauri-b-earths_b_11705746.html. 
  3. ↑ Tuomi, Mikko; Anglada-Escude, Guillem; Gerlach, Enrico; Jones, Hugh R. R.; Reiners, Ansgar; Rivera, Eugenio J.; Vogt, Steven S.; Butler, R. Paul (2012). "Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307". Astronomy 549: A48. doi:10.1051/0004-6361/201220268. Bibcode: 2013A&A...549A..48T. 
  4. ↑ 4.0 4.1 The Anglo-Australian Planet Search. XXIII. Two New Jupiter Analogs: Robert A. Wittenmyer, Jonathan Horner, C.G. Tinney, R.P. Butler, H.R.A. Jones, Mikko Tuomi, G.S. Salter, B.D. Carter, F. Elliott Koch, S.J. O'Toole, J. Bailey, D. Wright
  5. ↑ Guillem Anglada-Escudé, Pamela Arriagada, Mikko Tuomi, Mathias Zechmeister, James S. Jenkins, Aviv Ofir, Stefan Dreizler, Enrico Gerlach, Chris J. Marvin, Ansgar Reiners, Sandra V. Jeffers, R. Paul Butler, Steven S. Vogt, Pedro J. Amado, Cristina Rodríguez-López, Zaira M. Berdiñas, Julian Morin, Jeff D. Crane, Stephen A. Shectman, Ian B. Thompson, Matías Díaz, Eugenio Rivera, Luis F. Sarmiento, Hugh R.A. Jones, Two planets around Kapteyn's star : a cold and a temperate super-Earth orbiting the nearest halo red-dwarf. (Cornell University 3 June 2014).
  6. ↑ Mikko Tuomi, Hugh R. A. Jones, John R. Barnes, Guillem Anglada-Escudé, James S. Jenkins, Bayesian search for low-mass planets around nearby M dwarfs. Estimates for occurrence rate based on global detectability statistics (Submitted on 3 Mar 2014).
  7. ↑ A new cold sub-Saturnian candidate planet orbiting GJ 221: Mikko Tuomi, January 16, 2014
  8. ↑ Mikko Tuomi (2011). "Bayesian re-analysis of the radial velocities of Gliese 581. Evidence in favour of only four planetary companions". Astronomy & Astrophysics 528: L5. doi:10.1051/0004-6361/201015995. Bibcode: 2011A&A...528L...5T. 
  9. ↑ Tuomi, M. (March 2013). "Signals embedded in the radial velocity noise: Periodic variations in the Tau Ceti velocities". Astronomy & Astrophysics 551 (preprint): A79. doi:10.1051/0004-6361/201220509. Bibcode: 2012yCat..35510079T. http://www.aanda.org/articles/aa/full_html/2013/03/aa20509-12/aa20509-12.html. 
  10. ↑ Stephens, Tim: Four Earth-sized planets detected orbiting the nearest sun-like star. Phys.org, August 9, 2017.
  11. ↑ Wittenmyer, Robert A.; Tuomi, Mikko; Butler, R. P.; Jones, H. R. A.; Anglada-Escude, Guillem; Horner, Jonathan; Tinney, C. G.; Marshall, J. P. et al. (2014-06-21). "GJ 832c: A Super-Earth in the Habitable Zone". The Astrophysical Journal 791 (2): 114. doi:10.1088/0004-637X/791/2/114. ISSN 0004-637X. Bibcode: 2014ApJ...791..114W. https://www.researchgate.net/publication/263352191. 
  12. ↑ Anglada-Escude, G.; Arriagada, P.; Tuomi, M.; Zechmeister, M.; Jenkins, J. S.; Ofir, A.; Dreizler, S.; Gerlach, E. et al. (2014-06-03). "Two planets around Kapteyn's star: a cold and a temperate super-Earth orbiting the nearest halo red dwarf". Monthly Notices of the Royal Astronomical Society: Letters 443 (1): L89–L93. doi:10.1093/mnrasl/slu076. ISSN 1745-3925. Bibcode: 2014MNRAS.443L..89A. https://www.researchgate.net/publication/262840914. 
  13. ↑ Tuomi, M.; Jones, H. R. A.; Barnes, J. R.; Anglada-Escude, G.; Jenkins, J. S. (2014-03-03). "Bayesian search for low-mass planets around nearby M dwarfs - estimates for occurrence rate based on global detectability statistics". Monthly Notices of the Royal Astronomical Society 441 (2): 1545–1569. doi:10.1093/mnras/stu358. ISSN 0035-8711. Bibcode: 2014MNRAS.441.1545T. https://www.researchgate.net/publication/260483215. 
  14. ↑ Anglada-Escudé, Guillem; Tuomi, Mikko; Gerlach, Enrico; Barnes, Rory; Heller, René; Jenkins, James S.; Wende, Sebastian; Vogt, Steven S. et al. (2013-06-25). "A dynamically-packed planetary system around GJ 667C with three super-Earths in its habitable zone". Astronomy & Astrophysics 556: A126. doi:10.1051/0004-6361/201321331. ISSN 0004-6361. Bibcode: 2013A&A...556A.126A. https://www.researchgate.net/publication/241689403. 






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