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Star · F4V

WASP-66

WASP-66 is a main-sequence star of spectral type F4V in the constellation Antlia, 1,634 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationAntlia
Distance1,634 light-years (500.9 pc)
Apparent magnitudemagnitude 11.65
Absolute magnitudemagnitude 3.15
Spectral typeF4V
Surface temperature6,600 K
Luminosity4.34 L☉
Radius1.76 R☉
Mass1.33 M☉
Age3.7 billion years
Metallicity [Fe/H]-0.31
Right ascension (J2000)10h 32m 54.0s
Declination (J2000)−34° 59′ 23″
Space velocity (relative to the Sun)43.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.65. Visible from the whole Southern Hemisphere and north to latitude 55° N. South of latitude 55° S it never sets. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 392. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 29 million years.

The Sun seen from there

From a planet around WASP-66, the Sun would look like a star of magnitude 13.33, in the direction where our sky has the constellation Pegasus. It would be invisible to the naked eye.

Planets

Open in the simulation

Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.