lambda Librae

{{short description|Binary star system in the constellation Libra}}

{{Starbox begin

| name = Lambda Librae

}}

{{Starbox image

| image = 250px

| caption = A light curve for Lambda Librae, adapted from Wraight et al. (2012)

}}

{{Starbox observe

| epoch = J2000.0

| equinox = J2000.0 (ICRS)

| constell = Libra

| ra = {{RA|15|53|20.05463}}

| dec = {{DEC|−20|10|01.4177}}

| appmag_v = 5.03

}}

{{Starbox character

| class = B3 V

| b-v = −0.023

| u-b = −0.584

| r-i =

| variable = Rotating ellipsoidal

}}

{{Starbox astrometry

| radial_v = {{Val|−2.0|0.5}}

| prop_mo_ra = −9.81

| prop_mo_dec = −26.85

| parallax = 10.54

| p_error = 0.91

| parallax_footnote =

| absmag_v = 0.56

}}

{{Starbox orbit

| reference =

| period_unitless = {{Val|14.4829|0.0004|u=d}}

| eccentricity = {{Val|0.27|0.09}}

| periastron = {{nowrap|2435172.380 ± 0.664 JD}}

| periarg = {{Val|217|17}}

| k1 = {{Val|28.5|3.3}}

}}

{{Starbox detail

| source =

| mass = {{Val|5.01|0.26}}

| radius = 3.9

| luminosity = 743

| temperature = 18,700

| gravity = 4.75

| metal_fe = −0.27

| rotational_velocity = 155

| age_myr = 282

}}

{{Starbox catalog

| names = λ Lib, 45 Lib, BD−19°4249, FK5 1415, HD 142096, HIP 77811, HR 5902, SAO 183895.

}}

{{Starbox reference

| Simbad = lam+Lib

}}

{{Starbox end}}

λ Librae (Latinised as Lambda Librae) is the Bayer designation for a binary star system in the zodiac constellation of Libra. It can be faintly seen with the naked eye, having an apparent visual magnitude of 5.03. With an annual parallax shift of 10.54 mas, it is roughly 310 light years from the Sun. At that distance, the visual magnitude of this system is diminished by an extinction factor of 0.22 due to interstellar dust. It is 0.1 degree north of the ecliptic.

This is a single-lined spectroscopic binary star system with an orbital period of 14.48 days and an eccentricity of 0.27. The visible component is a B-type main sequence star with a stellar classification of B3 V. It is a helium-weak chemically peculiar star and a rotating ellipsoidal variable. The star has an estimated 3.9 times the radius of the Sun and five times the Sun's mass. This is a candidate Vega-like star, meaning that it shows an infrared excess characteristic of a circumstellar debris disk. The system is a source of X-ray emission.

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{{citation

| title=lam Lib -- Spectroscopic binary

| work=SIMBAD Astronomical Database

| publisher=Centre de Données astronomiques de Strasbourg

| url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=lam+Lib

| accessdate=2017-01-30 | postscript=. }}

}}

{{Stars of Libra|state=collapsed}}

{{DEFAULTSORT:Lambda Librae}}

Category:B-type main-sequence stars

Category:Spectroscopic binaries

Category:Helium-weak stars

Category:Libra (constellation)

Librae, Lambda

BD-19 4249

Librae, 45

142096

077811

5902

Category:Rotating ellipsoidal variables