Star · M
KMT-2025-BLG-0975L
KMT-2025-BLG-0975L is a main-sequence star of spectral type M in the constellation Scorpius, 25,800 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Scorpius |
|---|---|
| Distance | 25,800 light-years (7,923 pc) |
| Apparent magnitude | magnitude 33.44 |
| Absolute magnitude | magnitude 18.95 |
| Spectral type | M |
| Surface temperature | 5,780 K |
| Luminosity | 2.45 × 10⁻⁶ L☉ |
| Radius | 0.00156 R☉ |
| Mass | 0.1 M☉ (estimated) |
| Right ascension (J2000) | 17h 50m 17.8s |
| Declination (J2000) | −30° 35′ 15″ |
In the sky
A telescope is needed to see it: its apparent magnitude is 33.44. Visible from the whole Southern Hemisphere and north to latitude 59° N. South of latitude 59° S 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 26 thousand years ago. At that time Homo sapiens was spreading out of Africa; there was no farming yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 458 million years.
The Sun seen from there
From a planet around KMT-2025-BLG-0975L, the Sun would look like a star of magnitude 19.32, in the direction where our sky has the constellation Auriga. It would be invisible to the naked eye.
Planets
- KMT-2025-BLG-0975L b 5.97 R⊕
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.