Star · G2V
TOI-1273
TOI-1273 is a main-sequence star of spectral type G2V in the constellation Ursa Major, 576.4 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Ursa Major |
|---|---|
| Distance | 576.4 light-years (176.7 pc) |
| Apparent magnitude | magnitude 11.05 |
| Absolute magnitude | magnitude 4.81 |
| Spectral type | G2V |
| Surface temperature | 5,690 K |
| Luminosity | 1.07 L☉ |
| Radius | 1.06 R☉ |
| Mass | 1.06 M☉ |
| Age | 3.1 billion years |
| Metallicity [Fe/H] | 0.07 |
| Right ascension (J2000) | 14h 16m 28.9s |
| Declination (J2000) | +58° 23′ 26″ |
| Space velocity (relative to the Sun) | 48.6 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.05. Visible from the whole Northern Hemisphere and south to latitude 32° S. North of latitude 32° 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 1450. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 10 million years.
The Sun seen from there
From a planet around TOI-1273, the Sun would look like a star of magnitude 11.07, in the direction where our sky has the constellation Horologium. It would be invisible to the naked eye.
Planets
- TOI-1273 b 4.63-day orbit · 11.1 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.