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Star · G0IV

Muphrid

Muphrid is a subgiant star of spectral type G0IV in the constellation Boötes, 37.2 light-years from the Sun.

Other namesη Boo · Gl 534 · HIP 67927
ConstellationBoötes
Distance37.2 light-years (11.4 pc)
Apparent magnitudemagnitude 2.68
Absolute magnitudemagnitude 2.40
Spectral typeG0IV
Surface temperature6,050 K
Luminosity9.79 L☉
Radius2.85 R☉
Mass1.77 M☉ (estimated)
Right ascension (J2000)13h 54m 41.1s
Declination (J2000)+18° 23′ 52″
Space velocity (relative to the Sun)20.3 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 2.68). Visible from the whole Northern Hemisphere and south to latitude 72° S. North of latitude 72° 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 1989. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 659 thousand years.

The Sun seen from there

From a planet around Muphrid, the Sun would look like a star of magnitude 5.11, in the direction where our sky has the constellation Cetus. It would be visible to the naked eye.

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

Open in the simulation

Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.