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Star · M4

Ross 128

Ross 128 is a main-sequence star of spectral type M4 in the constellation Virgo, 11.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesGl 447 · HIP 57548
ConstellationVirgo
Distance11.0 light-years (3.37 pc)
Apparent magnitudemagnitude 11.12
Absolute magnitudemagnitude 13.48
Spectral typeM4
Surface temperature3,190 K
Luminosity0.00362 L☉
Radius0.197 R☉
Mass0.168 M☉
Age5.0 billion years
Metallicity [Fe/H]-0.02
Right ascension (J2000)11h 47m 44.5s
Declination (J2000)+0° 48′ 17″
Space velocity (relative to the Sun)38.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.12. Visible from the whole Northern Hemisphere and south to latitude 89° S. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 2015. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 195 thousand years.

The Sun seen from there

From a planet around Ross 128, the Sun would look like a star of magnitude 2.47, in the direction where our sky has the constellation Pisces. It would be visible to the naked eye.

Planets

Neighbours

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

Open in the simulation

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