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Lalande 21185

Star · Star in the constellation Ursa Major

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Lalande 21185
Picture: IAU and Sky & Telescope magazine (Roger Sinnott & Rick Fienberg), CC BY 3.0, via Wikimedia Commons.

About Lalande 21185

Lalande 21185 is about 8.31 light-years from the Sun, so the light we see from it left about 8.31 years ago.

At apparent magnitude 7.49 it is too faint for the naked eye but within reach of binoculars.

It gives out 5.7 × 10⁻³ times as much light as the Sun.

It has 2 known planets.

The map lists it as a star and shows it among the stars around the Sun, drawn on the plane of the Milky Way.

Key numbers

Distance8.31 light-years (2.55 pc)
Spectral typeM2V
Apparent magnitude7.49
Absolute magnitude10.46
Luminosity5.7 × 10⁻³ × the Sun
ConstellationUMa
Known planets2

Planets: NASA Exoplanet Archive (Planetary Systems Composite Parameters).

Known planets

PlanetMass (Earth = 1)Radius (Earth = 1)Orbit (days)Found
GJ 411 b2.691.4512.93942019, radial velocity
HD 95735 c13.63.7629462021, radial velocity

Where it is

Its place in the universe, from the inside out: Solar neighbourhood › Local Bubble › Orion–Cygnus Arm (Local Arm) › Milky Way › Local Group › Virgo Supercluster › Laniakea Supercluster › Observable universe.

Zoom out to see it in context: Nearest stars, a view about 24 light-years across.

From Wikipedia

Lalande 21185 is a star in the south of Ursa Major. It is the apparent brightest red dwarf in the northern hemisphere. Despite this, and being relatively close by, it is very dim, being only magnitude 7.5 in visible light and thus too faint to be seen with the unaided eye.

Excerpt from the Wikipedia article Lalande 21185, licensed CC BY-SA 4.0.

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