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Star · K9V

TIC 88692598

TIC 88692598 is a main-sequence star of spectral type K9V in the constellation Ursa Major, 242.1 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationUrsa Major
Distance242.1 light-years (74.2 pc)
Apparent magnitudemagnitude 13.98
Absolute magnitudemagnitude 9.63
Spectral typeK9V
Surface temperature3,480 K
Luminosity0.0436 L☉
Radius0.532 R☉
Mass0.529 M☉
Right ascension (J2000)9h 56m 50.6s
Declination (J2000)+47° 46′ 14″
Space velocity (relative to the Sun)31.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 13.98. Visible from the whole Northern Hemisphere and south to latitude 42° S. North of latitude 42° N it never sets. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1784. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.3 million years.

The Sun seen from there

From a planet around TIC 88692598, the Sun would look like a star of magnitude 9.18, in the direction where our sky has the constellation Grus. It would be invisible to the naked eye.

Planets

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

Open in the simulation

Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.