Star · M4V
CWISEP J042455.68+000221.4
CWISEP J042455.68+000221.4 is a main-sequence star of spectral type M4V in the constellation Eridanus, 88.1 light-years from the Sun.
| Constellation | Eridanus |
|---|---|
| Distance | 88.1 light-years (27.0 pc) |
| Apparent magnitude | magnitude 27.17 |
| Absolute magnitude | magnitude 25.01 |
| Spectral type | M4V |
| Surface temperature | 2,980 K |
| Luminosity | 1.55 × 10⁻⁷ L☉ |
| Radius | 0.00148 R☉ |
| Mass | 0.075 M☉ (estimated) |
| Right ascension (J2000) | 4h 24m 55.5s |
| Declination (J2000) | +0° 02′ 23″ |
| Space velocity (relative to the Sun) | 26.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 27.17. Visible from the whole Southern Hemisphere and north to latitude 90° N. It stands highest at midnight in November, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1938. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.6 million years.
The Sun seen from there
From a planet around CWISEP J042455.68+000221.4, the Sun would look like a star of magnitude 6.99, in the direction where our sky has the constellation Ophiuchus. 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.
