Star · G5
TOI-1776
TOI-1776 is a main-sequence star of spectral type G5 in the constellation Ursa Major, 146.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Other names | HIP 53688 |
|---|---|
| Constellation | Ursa Major |
| Distance | 146.0 light-years (44.7 pc) |
| Apparent magnitude | magnitude 8.26 |
| Absolute magnitude | magnitude 5.01 |
| Spectral type | G5 |
| Surface temperature | 5,790 K |
| Luminosity | 0.885 L☉ |
| Radius | 0.936 R☉ |
| Mass | 0.92 M☉ |
| Age | 5.1 billion years |
| Metallicity [Fe/H] | -0.19 |
| Right ascension (J2000) | 10h 59m 06.2s |
| Declination (J2000) | +40° 59′ 01″ |
| Space velocity (relative to the Sun) | 52.0 km/s |
In the sky
Too faint for the naked eye (magnitude 8.26); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° N it never sets. It stands highest at midnight in March, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1880. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.6 million years.
The Sun seen from there
From a planet around TOI-1776, the Sun would look like a star of magnitude 8.08, in the direction where our sky has the constellation Grus. It would be invisible to the naked eye.
Planets
- TOI-1776 b 2.8-day orbit · 1.22 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.