Star · M2.5 V
TOI-2095
TOI-2095 is a main-sequence star of spectral type M2.5 V in the constellation Draco, 136.7 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).
| Constellation | Draco |
|---|---|
| Distance | 136.7 light-years (41.9 pc) |
| Apparent magnitude | magnitude 12.85 |
| Absolute magnitude | magnitude 9.74 |
| Spectral type | M2.5 V |
| Surface temperature | 3,760 K |
| Luminosity | 0.0348 L☉ |
| Radius | 0.44 R☉ |
| Mass | 0.44 M☉ |
| Age | 1.0 billion years |
| Metallicity [Fe/H] | -0.24 |
| Right ascension (J2000) | 19h 02m 32.8s |
| Declination (J2000) | +75° 25′ 07″ |
| Space velocity (relative to the Sun) | 45.5 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.85. Visible from the whole Northern Hemisphere and south to latitude 15° S. North of latitude 15° N it never sets.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1889. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.4 million years.
The Sun seen from there
From a planet around TOI-2095, the Sun would look like a star of magnitude 7.94, in the direction where our sky has the constellation Mensa. It would be invisible to the naked eye.
Planets
- TOI-2095 b 17.7-day orbit · 1.25 R⊕
- TOI-2095 c 28.2-day orbit · 1.33 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.