Star · M4V
ULAS J135322.83+283408.2
ULAS J135322.83+283408.2 is a main-sequence star of spectral type M4V in the constellation Canes Venatici, 84.8 light-years from the Sun.
| Constellation | Canes Venatici |
|---|---|
| Distance | 84.8 light-years (26.0 pc) |
| Apparent magnitude | magnitude 25.91 |
| Absolute magnitude | magnitude 23.84 |
| Spectral type | M4V |
| Surface temperature | 2,980 K |
| Luminosity | 4.59 × 10⁻⁷ L☉ |
| Radius | 0.00255 R☉ |
| Mass | 0.075 M☉ (estimated) |
| Right ascension (J2000) | 13h 53m 22.8s |
| Declination (J2000) | +28° 34′ 06″ |
| Space velocity (relative to the Sun) | 7.0 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 25.91. Visible from the whole Northern Hemisphere and south to latitude 61° S. North of latitude 61° N it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1941. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.5 million years.
The Sun seen from there
From a planet around ULAS J135322.83+283408.2, the Sun would look like a star of magnitude 6.90, in the direction where our sky has the constellation Fornax. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.