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Star · M4V

2MASSI J1553022+153236

2MASSI J1553022+153236 is a main-sequence star of spectral type M4V in the constellation Serpens, 43.4 light-years from the Sun.

ConstellationSerpens
Distance43.4 light-years (13.3 pc)
Apparent magnitudemagnitude 23.33
Absolute magnitudemagnitude 22.71
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.30 × 10⁻⁶ L☉
Radius0.00429 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)15h 53m 02.2s
Declination (J2000)+15° 32′ 37″
Space velocity (relative to the Sun)26.5 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 23.33. Visible from the whole Northern Hemisphere and south to latitude 74° S. North of latitude 74° N it never sets. It stands highest at midnight in May, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1983. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 771 thousand years.

The Sun seen from there

From a planet around 2MASSI J1553022+153236, the Sun would look like a star of magnitude 5.45, in the direction where our sky has the constellation Eridanus. 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.