Star · M4V
SDSS J133257.73+325813.1
SDSS J133257.73+325813.1 is a main-sequence star of spectral type M4V in the constellation Canes Venatici, 300.1 light-years from the Sun.
| Constellation | Canes Venatici |
|---|---|
| Distance | 300.1 light-years (92.0 pc) |
| Apparent magnitude | magnitude 22.07 |
| Absolute magnitude | magnitude 17.25 |
| Spectral type | M4V |
| Surface temperature | 2,980 K |
| Luminosity | 1.98 × 10⁻⁴ L☉ |
| Radius | 0.0529 R☉ |
| Mass | 0.075 M☉ (estimated) |
| Right ascension (J2000) | 13h 32m 57.7s |
| Declination (J2000) | +32° 58′ 13″ |
| Space velocity (relative to the Sun) | 76.5 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 22.07. 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 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 1726. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.3 million years.
The Sun seen from there
From a planet around SDSS J133257.73+325813.1, the Sun would look like a star of magnitude 9.65, in the direction where our sky has the constellation Sculptor. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 67391 17.7 light-years
- HIP 64922 18.1 light-years
- HIP 67384 19.8 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.