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HIP 79431

Red dwarf star in the constellation Scorpius


Red dwarf star in the constellation Scorpius

| r-i = 1.09 | v-r = 0.88 | b-v = 1.486 | u-b =

0.466

0.442 4.815 HIP 79431 is a red dwarf star with a planetary companion in the constellation Scorpius. It has the proper name Sharjah, as selected in the NameExoWorlds campaign by United Arab Emirates, during the 100th anniversary of the IAU. Sharjah is the cultural capital of United Arab Emirates. The star has an apparent visual magnitude of 11.34, which is far too faint to be visible to the naked eye. Based on parallax measurements, this system is located at a distance of 47.4 light-years from the Sun. It is drifting closer with a radial velocity of −5 km/s.

This is an M-type main-sequence star with a stellar classification of M3V. This star is smaller, cooler, dimmer, and less massive than the Sun, but the estimated metal content is 2.5 times as much as the Sun. The level of chromospheric activity does not appear to be unusually high for a star of this class.

In 2010, a superjovian exoplanetary companion was discovered using the radial-velocity method. It is orbiting at a distance of from the host star with a period of 111.7 days and an eccentricity (ovalness) of 0.29. Since the inclination of the orbit is unknown, only a lower bound on the mass can be determined. It has at least 2.1 times the mass of Jupiter.

The star also shows anomalies in its proper motion and radial velocity variations, suggesting the presence of an outer planet between 5 and 12 AU, 11 times more massive than Jupiter.

References

| display-authors=1 | last1=Apps | first1=Kevin

| display-authors=1 | journal=The Astrophysical Journal

| display-authors=1 | last1=Terrien | first1=Ryan C.

| display-authors=1 | journal=The Astronomical Journal

| display-authors=1 | last1=Stassun | first1=Keivan G.

| display-authors=1 | last1=Doyle | first1=L.

| access-date=2020-01-02 | archive-date=2022-12-05 | archive-url=https://web.archive.org/web/20221205123842/http://www.iau.org/news/pressreleases/detail/iau1912/ | url-status=dead

References

  1. (2025). "Imaging a Hidden Super-Jupiter Accelerating its Metal-rich M-dwarf Host". JWST Proposal.
  2. {{Cite Gaia DR3. 6245870673116518784
  3. {{cite XHIP. 79431
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