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EntityQ683605· pop 35· linked from 428 articles

Lalande 21185

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Also known as HD 95735, Argelander's second star, Gliese 411, HIP 54035

star in the constellation Ursa Major

In the Vinony graph

Within Vinony's link graph, Lalande 21185 is referenced by 428 other articles, and connects out to list of stars in Ursa Major, star catalogue and year.

It is catalogued under topics including BY Draconis variables, Durchmusterung objects and Gliese and GJ objects.

Its subject is documented across 34 Wikipedia language editions.

Astronomical data · SIMBAD

Object type
PM*
Spectral type
M2+V
Distance
8 light-years
Redshift
z = -0.0002822888066921214
Coordinates
RA 165.8341° · Dec 35.9699°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Key facts

Constellation
Ursa Major
Right ascension
11 03 20.19482
Declination
+35 ° 58 ′ 11.5762 ″
Spectral type
M2V
Apparent magnitude b
8.960 ± 0.007
Apparent magnitude r
~6.6
Apparent magnitude i
~5.8
Apparent magnitude j
4.203 ±0.242
Apparent magnitude h
3.640 ±0.202
Apparent magnitude k
3.254 ±0.306
U b color index
+1.074
B v color index
+1.444
Variable type
BY

via Wikipedia infobox

Wikidata facts

Constellation
Ursa Major
Distance from Earth
2.55
Diameter
611000
Radius
0.393
Mass
0.46
Variable-star type
rotating variable star
Show 21 more facts
spectral class
dM2
catalog code
UBV M 16736
stellar rotational velocity
6.54
time of discovery or invention
1801-00-00
effective temperature
3652
apparent magnitude
6.551172
metallicity
-0.25
absolute magnitude
10.46
parallax
392.7529
discoverer or inventor
Jérôme Lalande
radial velocity
-84.237602
epoch
J2000.0
angular diameter
1.42
surface gravity
52000
luminosity
0.0016
age estimated by a dating method
7.5
right ascension component of proper motion
-565
declination component of proper motion
-4745
Commons category
Lalande 21185
right ascension
165.8341450816425
declination
35.96988227279361
Sources (4)

via Wikidata · CC0

~9 min read

Encyclopedic overview

Lalande 21185 (also known as BD+36 2147, Gliese 411, and HD 95735) 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 (as are all red dwarfs), being only magnitude 7.5 in visible light and thus too faint to be seen with the unaided eye. The star is visible through a small telescope or binoculars.

At 8.304 light-years (2.546 parsecs) away it is one of the stars nearest to the Solar System; only the Alpha Centauri system, Barnard's Star, Wolf 359, and the brown dwarfs Luhman 16 and WISE 0855−0714 are known to be closer. Because of its proximity it is a frequent subject for astronomical surveys and other research and thus is known by numerous other designations, most commonly Gliese 411 and HD 95735. In approximately 19,900 years it will be at its closest, about 4.65 ly (1.43 pc) from the Sun, just over half its present distance.

Excerpted from Wikipedia’s “Lalande 21185” article, available under the CC BY-SA 4.0 licence.

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