Star · G5V
TOI-5335
TOI-5335 is a main-sequence star of spectral type G5V in the constellation Aries, 1,081 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Aries |
|---|---|
| Distance | 1,081 light-years (331.3 pc) |
| Apparent magnitude | magnitude 13.43 |
| Absolute magnitude | magnitude 5.83 |
| Spectral type | G5V |
| Surface temperature | 5,530 K |
| Luminosity | 0.657 L☉ |
| Radius | 0.917 R☉ |
| Mass | 0.945 M☉ |
| Right ascension (J2000) | 3h 07m 48.6s |
| Declination (J2000) | +15° 21′ 33″ |
| Space velocity (relative to the Sun) | 4.0 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 13.43. Visible from the whole Northern Hemisphere and south to latitude 75° S. North of latitude 75° N it never sets. 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 945. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 19 million years.
The Sun seen from there
From a planet around TOI-5335, the Sun would look like a star of magnitude 12.43, in the direction where our sky has the constellation Libra. It would be invisible to the naked eye.
Planets
- TOI-5335 b 3.61-day orbit · 4.02 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.