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Star · M4V

CWISEP J160835.01-244244.7

CWISEP J160835.01-244244.7 is a main-sequence star of spectral type M4V in the constellation Scorpius, 88.1 light-years from the Sun.

ConstellationScorpius
Distance88.1 light-years (27.0 pc)
Apparent magnitudemagnitude 25.16
Absolute magnitudemagnitude 23.00
Spectral typeM4V
Surface temperature2,980 K
Luminosity9.88 × 10⁻⁷ L☉
Radius0.00374 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)16h 08m 34.7s
Declination (J2000)−24° 42′ 44″
Space velocity (relative to the Sun)38.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 25.16. Visible from the whole Southern Hemisphere and north to latitude 65° N. South of latitude 65° S 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 1938. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.6 million years.

The Sun seen from there

From a planet around CWISEP J160835.01-244244.7, the Sun would look like a star of magnitude 6.99, in the direction where our sky has the constellation Taurus. It would be invisible 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.