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EntityQ4052871· pop 6· linked from 401 articles

Also known as BD+00 316, Mpingo

WASP-71, also named Mpingo, is an ordinary star with a close-orbiting planetary companion in the equatorial constellation of Cetus. With an apparent visual magnitude of 10.56, it is too faint to be visible to the naked eye. This star is located at a distance of 1,160 light-years based on parallax measurements, and is drifting further away with a heliocentric radial velocity of 7.7 km/s.

In the Vinony graph

Vinony's link graph records 401 inbound references to WASP-71, and connects out to list of NGC objects (1–1000), year and light-year.

It sits within the topics Cetus, Durchmusterung objects and F-type main-sequence stars.

Vinony links it to 6 Wikipedia language editions.

Wikidata facts

Distance from Earth
200
Radius
2.32
Mass
1.572
Show 15 more facts
catalog code
BD+00 316
effective temperature
6050
apparent magnitude
10.568543
radial velocity
5.28
metallicity
0.15
parallax
2.8158
surface gravity
9300
name
Mpingo
luminosity
5.8674645
spectral class
F8IV
age estimated by a dating method
2000000000
right ascension component of proper motion
23.418
declination component of proper motion
-6.844
right ascension
29.26334978377
declination
0.75885418136
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Encyclopedic overview

3 sections
Contents
  • Nomenclature
  • Planetary system
  • References

WASP-71, also named Mpingo, is an ordinary star with a close-orbiting planetary companion in the equatorial constellation of Cetus. With an apparent visual magnitude of 10.56, it is too faint to be visible to the naked eye. This star is located at a distance of 1,160 light-years based on parallax measurements, and is drifting further away with a heliocentric radial velocity of 7.7 km/s.

This is classified as an F-type star with a stellar classification of F8. It is more than double the diameter of the Sun with 1.5 times the Sun's mass. The star is younger than the Sun at about 3.6 billion years, yet is already evolving away from the main sequence. BD+00 316 is enriched in heavy elements, having 140% of the solar abundance of iron. Imaging surveys in 2015 and 2020 failed to find any stellar companions for BD+00 316.

Excerpted from Wikipedia’s “WASP-71” article, available under the CC BY-SA 4.0 licence.

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