Star · K4V
TOI-1435
TOI-1435 is a main-sequence star of spectral type K4V in the constellation Draco, 303.6 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Draco |
|---|---|
| Distance | 303.6 light-years (93.1 pc) |
| Apparent magnitude | magnitude 10.74 |
| Absolute magnitude | magnitude 5.90 |
| Spectral type | K4V |
| Surface temperature | 5,140 K |
| Luminosity | 0.427 L☉ |
| Radius | 0.824 R☉ |
| Mass | 0.87 M☉ |
| Right ascension (J2000) | 13h 34m 08.9s |
| Declination (J2000) | +67° 37′ 18″ |
| Space velocity (relative to the Sun) | 61.6 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 10.74. Visible from the whole Northern Hemisphere and south to latitude 22° S. North of latitude 22° 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 1722. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.4 million years.
The Sun seen from there
From a planet around TOI-1435, the Sun would look like a star of magnitude 9.67, in the direction where our sky has the constellation Hydrus. It would be invisible to the naked eye.
Planets
- TOI-1435 b 0.686-day orbit · 1.08 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 65287 12.3 light-years
- TOI-1174 13.5 light-years
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.