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Star · M4V

2MASS J03480772-6022270

2MASS J03480772-6022270 is a main-sequence star of spectral type M4V in the constellation Reticulum, 27.2 light-years from the Sun.

ConstellationReticulum
Distance27.2 light-years (8.33 pc)
Apparent magnitudemagnitude 22.82
Absolute magnitudemagnitude 23.22
Spectral typeM4V
Surface temperature2,980 K
Luminosity8.12 × 10⁻⁷ L☉
Radius0.00339 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)3h 48m 07.7s
Declination (J2000)−60° 22′ 27″
Space velocity (relative to the Sun)35.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.82. Visible from the whole Southern Hemisphere and north to latitude 30° N. South of latitude 30° S it never sets. It stands highest at midnight in November, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1999. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 482 thousand years.

The Sun seen from there

From a planet around 2MASS J03480772-6022270, the Sun would look like a star of magnitude 4.43, in the direction where our sky has the constellation Draco. It would be visible to the naked eye.

Neighbours

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

Open in the simulation

Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.