Star · F0V
HAT-P-41
HAT-P-41 is a main-sequence star of spectral type F0V in the constellation Aquila, 1,145 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Aquila |
|---|---|
| Distance | 1,145 light-years (351.2 pc) |
| Apparent magnitude | magnitude 11.40 |
| Absolute magnitude | magnitude 3.67 |
| Spectral type | F0V |
| Surface temperature | 6,390 K |
| Luminosity | 4.25 L☉ |
| Radius | 2.05 R☉ |
| Mass | 2.56 M☉ |
| Age | 2.2 billion years |
| Metallicity [Fe/H] | 0.21 |
| Right ascension (J2000) | 19h 49m 17.4s |
| Declination (J2000) | +4° 40′ 21″ |
| Space velocity (relative to the Sun) | 34.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.40. Visible from the whole Northern Hemisphere and south to latitude 85° S. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 881. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 20 million years.
The Sun seen from there
From a planet around HAT-P-41, the Sun would look like a star of magnitude 12.56, in the direction where our sky has the constellation Monoceros. It would be invisible to the naked eye.
Planets
- HAT-P-41 b 2.69-day orbit · 23 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.