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Star · M4V

VHS J192934.18-442550.5

VHS J192934.18-442550.5 is a main-sequence star of spectral type M4V in the constellation Sagittarius, 110.9 light-years from the Sun.

ConstellationSagittarius
Distance110.9 light-years (34.0 pc)
Apparent magnitudemagnitude 24.64
Absolute magnitudemagnitude 21.98
Spectral typeM4V
Surface temperature2,980 K
Luminosity2.53 × 10⁻⁶ L☉
Radius0.00599 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)19h 29m 34.1s
Declination (J2000)−44° 25′ 50″
Space velocity (relative to the Sun)20.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 24.64. Visible from the whole Southern Hemisphere and north to latitude 46° N. South of latitude 46° S it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1915. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.0 million years.

The Sun seen from there

From a planet around VHS J192934.18-442550.5, the Sun would look like a star of magnitude 7.49, in the direction where our sky has the constellation Lynx. 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.