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Star · G6V

WASP-48

WASP-48 is a main-sequence star of spectral type G6V in the constellation Cygnus, 1,507 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationCygnus
Distance1,507 light-years (462.1 pc)
Apparent magnitudemagnitude 11.72
Absolute magnitudemagnitude 3.40
Spectral typeG6V
Surface temperature5,920 K
Luminosity3.8 L☉
Radius1.58 R☉
Mass0.88 M☉
Age7.9 billion years
Metallicity [Fe/H]-0.12
Right ascension (J2000)19h 24m 39.0s
Declination (J2000)+55° 28′ 23″
Space velocity (relative to the Sun)65.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.72. Visible from the whole Northern Hemisphere and south to latitude 35° S. North of latitude 35° N it never sets. 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 519. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 27 million years.

The Sun seen from there

From a planet around WASP-48, the Sun would look like a star of magnitude 13.15, in the direction where our sky has the constellation Carina. 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.