2018년 2월 19일 월요일

HAT-P-14b

HAT-P-14b

HAT - P - 14 bis to revolve around. It was discovered by the transit method and published in the paper on March 10, 2010.

HAT-P-14b

Comparison of size of HAT-P-14b (gray) and Jupiter

Main star *| | *| () | 17 h 20 m 28 s | (δ ) | + 38 ° 14 '32 " *| ( m V ) | 9.98 | 670 ± 36 (205 ± 11) *| F | ( m ) | 1.386 ± 0.045 M ☉ *| (r) | 1.468 ± 0.054 | (T) | 6600 ± 90 *| [Fe / H] | 0.11 ± 0.08 | | 1.3 ± 0.4 *| (a) | 0.0606 ± 0.0007 (~ 9.06) | ~ ~ 0.295 | (q) | 0.0541 ± 0.0014 (~ 8.09) *| (Q) | 0.0671 ± 0.0016 (~ 10.03) | (e) | 0.107 ± 0.013 *| (P) | 4.6267669 ± 5e - 06 | (~ 111.0424) | (i ) | 83.5 ± 0.3 ° Physical property *| ( m ) | 2.232 ± 0.059 | (r) | 1.150 ± 0.052 Discovery Discovery date| March 10, 2010 Discover| Torres _ et al. _ *| *Current status| Preprint Reference database *| | *| |

This planet is located at a distance of about 205 light years in the direction of, and it is turning around HAT - P - 14 of 10 grade.

Related item

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Source

1. ****Torres, G. (2010). "HAT - P - 14b: A 2 Jupiter - mass exoplanet transiting a bright F star".

External link

There is a category related to****in Wikimedia Commons.

  • ". .Exoplanets. Browsing June 15, 2010.

:! [Star chart] (//upload.wikimedia.org/wikipedia/commons/thumb/8/83/Celestia.png/20px- Celestia.png)

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Post Date : 2018-02-19 23:00

This article is taken from the Japanese Wikipedia HAT-P-14b

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