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Star · M1V

SDSS J171049.35+332325.2

SDSS J171049.35+332325.2 is a main-sequence star of spectral type M1V in the constellation Hercules, 162.8 light-years from the Sun.

ConstellationHercules
Distance162.8 light-years (49.9 pc)
Apparent magnitudemagnitude 21.21
Absolute magnitudemagnitude 17.72
Spectral typeM1V
Surface temperature3,520 K
Luminosity3.88 × 10⁻⁵ L☉
Radius0.0167 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)17h 10m 49.1s
Declination (J2000)+33° 23′ 26″
Space velocity (relative to the Sun)41.5 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.21. Visible from the whole Northern Hemisphere and south to latitude 57° S. North of latitude 57° N it never sets. It stands highest at midnight in June, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1863. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.9 million years.

The Sun seen from there

From a planet around SDSS J171049.35+332325.2, the Sun would look like a star of magnitude 8.32, in the direction where our sky has the constellation Columba. 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.