Astronomy:HD 173416 b

From HandWiki
HD 173416 b / Wangshu
Discovery[1]
Discovered byLiu et al.
Discovery dateJanuary 10, 2009
radial velocity
Designations
Wangshu
Orbital characteristics[2]
astron|astron|helion}}1.399 AU (209.3×10^6 km)
astron|astron|helion}}0.917 AU (137.2×10^6 km)
1.158+0.003
−0.004
 astronomical unit|AU
Eccentricity0.208+0.089
−0.094
Orbital period322.03+1.33
−1.52
 d
astron|astron|helion}}2454735.0+23.4
−253.1
 JD
−117.9°+33.7°
−33.1°
Semi-amplitude35.33+4.07
−4.46
 m/s
StarHD 173416
Physical characteristics[2]
Mass≥1.841+0.206
−0.225
 MJ


HD 173416 b, also named Wangshu, is an extrasolar planet located approximately 433 light-years away in the constellation of Lyra, orbiting the 6th magnitude G-type giant star HD 173416. This planet is at least 2.7 times the mass of Jupiter and was discovered on January 10, 2009 by Liu et al. HD 173416 b orbits at 1.16 AU from the star. However, despite the fact that the planet orbits 16% further from the star than Earth does from the Sun, it has an orbital period of only 323.6 days, compared to 365.25 days for Earth. This inverse relationship is caused by the parent star having twice the mass of the Sun, which increases the strength of its gravitational field. This evidence implies that when this star was on the main sequence, it was an A-type star.

The planet HD 173416 b is named Wangshu (望舒). The name was selected in the 2019 NameExoWorlds campaign by China, during the 100th anniversary of the IAU. Wangshu is the goddess who drives for the Moon and also represents the Moon in Chinese mythology.[3][4]

References

  1. Liu (10 January 2009). "A Planetary Companion Orbiting to the Intermediate-Mass G Giant HD 173416" (abstract). Research in Astronomy and Astrophysics 9 (1): 4. doi:10.1088/1674-4527/9/1/001. Bibcode2009RAA.....9....1L. http://www.raa-journal.org/raa/index.php/raa/article/view/76. Retrieved 1 February 2009. 
  2. 2.0 2.1 Teng, Huan-Yu et al. (December 2023). "Revisiting planetary systems in the Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and a multiplicity-metallicity trend around evolved stars". Publications of the Astronomical Society of Japan 75 (6): 1030–1071. doi:10.1093/pasj/psad056. Bibcode2023PASJ...75.1030T. 
  3. "Approved names" (in en). http://www.nameexoworlds.iau.org/final-results. 
  4. "International Astronomical Union | IAU". https://www.iau.org/news/pressreleases/detail/iau1912/. 

Coordinates: Sky map 18h 43m 36.1097s, +36° 33′ 23.777″