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Star · M3.5 V

TOI-4438

TOI-4438 is a main-sequence star of spectral type M3.5 V in the constellation Hercules, 98.1 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationHercules
Distance98.1 light-years (30.1 pc)
Apparent magnitudemagnitude 13.74
Absolute magnitudemagnitude 11.35
Spectral typeM3.5 V
Surface temperature3,500 K
Luminosity0.0171 L☉
Radius0.365 R☉
Mass0.345 M☉
Age4.8 billion years
Metallicity [Fe/H]0.07
Right ascension (J2000)18h 01m 16.1s
Declination (J2000)+35° 35′ 41″
Space velocity (relative to the Sun)81.5 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 13.74. Visible from the whole Northern Hemisphere and south to latitude 54° S. North of latitude 54° N it never sets. It stands highest at midnight in June, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1928. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.7 million years.

The Sun seen from there

From a planet around TOI-4438, the Sun would look like a star of magnitude 7.22, in the direction where our sky has the constellation Columba. It would be invisible to the naked eye.

Planets

Neighbours

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

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