Emiw, CD−66°60, Gaia DR2 4704957491028733824, HD 7199, HIP 5529, SAO 248334, 2MASS J01104719-6611171[7]
Database references
SIMBAD
data
Exoplanet Archive
data
HD 7199 is a star in the constellation Tucana located 118 light years distance from the Sun based on parallax. It has an orange hue but is too dim to be viewed with the naked eye, having an apparent visual magnitude of +8.06.[2] The star is drifting further away from the Sun with a radial velocity of +5.6 km/s.[2]
The star HD 7199 is named Emiw. The name was selected in the NameExoWorlds campaign by Mozambique, during the 100th anniversary of the IAU. Emiw represents love in the local Makhuwa language.[8][9]
This object has a stellar classification of K1IV,[3] matching a K-type subgiant star that is in the process of cooling and expanding off the main sequence, having exhausted the supply of hydrogen at its core. It is around 10[4] billion years old with a low projected rotational velocity of 2.2 km/s.[5] The star looks to be very metal-rich, having more than double the abundance of iron compared to the Sun.[5] Both mass and radius are lower than the Sun's, and it only radiates 70% of the Sun's luminosity.[4] It displays a Sun-like magnetic activity cycle.[6]
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^ abcdefCite error: The named reference Anderson2012 was invoked but never defined (see the help page).
^ abCite error: The named reference Gray2006 was invoked but never defined (see the help page).
^ abcCite error: The named reference Bonfanti2015 was invoked but never defined (see the help page).
^ abcdCite error: The named reference Soto2018 was invoked but never defined (see the help page).
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HD7199 is a star in the constellation Tucana located 118 light years distance from the Sun based on parallax. It has an orange hue but is too dim to...
Quinque Dromedarii), in Arabic العوائد al‑ʿawāʾid. /ɛlˈteɪnᵻn/ Tucana HD7199 Emiw IAU new 2019 Mozambique proposal; represents love in the Makhuwa language...
discoveries from HARPS HARPS spectrograph HARPS spectrograph detail Animation of HD 10180 with its seven planets Similar instruments: HARPS-N is a copy of this...
language HD7199 (Emiw) 0.29 615.0 1.36 radial vel. 2011 117 0.89 5386 2019 NameExoWorlds Mozambique Bagan Bagan, ancient city in Myanmar HD 18742 (Ayeyarwady)...
period of around 567 days. HD 221287 has a spectral type of F7V and lies 173 light-years away, and has a super-Jovian planet. HD7199 has spectral type KOIV/V...
Look up hairu in Wiktionary, the free dictionary. Hairu may refer to: HD7199 b (planet), Star Emiw, Constellation Tucana; aka HIP 5529 b; named after...
Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan...
Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan...
Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan...
Maciejewski, G. (2011). "Substellar-Mass Companions to the K-Giants HD 240237, BD +48 738 and HD 96127". The Astrophysical Journal. 745 (1). 28. arXiv:1110.1641...
Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan...
Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan...
most massive exoplanet candidate is HD 217786 b, which masses 12.98 MJ; the least massive confirmed planet is HD 10180 b, which masses 0.004 MJ or 3.1...
Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts...
ISBN 978-81-8324-179-3. Assam General Knowledge. Bright Publications. p. 26. ISBN 978-81-7199-451-9. Subba, Tanka Bahadur; Ghosh, G.C. (2003). The Anthropology of North-East...
S2CID 13075815. Archived from the original (PDF) on 19 February 2019. Lim HD, van Rijn RM, Ling P, Bakker RA, Thurmond RL, Leurs R (September 2005). "Evaluation...
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