Lambda Arae

{{Short description|Star in the constellation Ara}}

{{Starbox begin

| name = Lambda Arae

}}

{{Starbox image

| image=

{{Location mark

|image=Ara constellation map.svg|alt=|float=center|width=240

|label=|position=right

|mark=Red circle.svg|mark_width=10|mark_link=λ Arae

|x=428|y=434

}}

|caption=Location of λ Arae (circled)

}}

{{Starbox observe

| epoch = J2000

| ra = {{RA|17|40|23.826}}

| dec = {{DEC|-49|24|56.10}}

| appmag_v = 4.77

| constell = Ara

}}

{{Starbox character

| class = F4 V

| r-i = +0.22

| v-r =

| b-v = +0.40

| u-b = −0.04

| variable = 3.10

}}

{{Starbox astrometry

| radial_v = +3.3{{±|0.3}}

| prop_mo_ra = +104.233

| prop_mo_dec = −175.956

| pm_footnote =

| parallax = 47.7045

| p_error = 0.1368

| parallax_footnote =

| absmag_v = +3.06

}}

{{Starbox detail

| mass = 1.37{{±|0.04}}

| radius = 1.711{{±|0.035}}

| luminosity = 4.69{{±|0.03|0.05}}

| temperature = 6,495{{±|3|7}}

| gravity = 4.064{{±|0.005|0.003}}

| metal_fe = −0.24

| rotational_velocity = 15.5

| age_gyr = 2.44{{±|0.39}}

}}

{{Starbox catalog

| names = {{odlist | B=λ Ara, λ Arae | CD=−49°11616 | GJ=686.2 | GJ2=9597 | HD=160032 | HIP=86486 | HR=6569 | NSV=23218 | NLTT=45187 | SAO=228257 | GC=23918 | PPM=323240 }}

}}

{{Starbox reference

| Simbad=lam+Ara

}}

{{Starbox end}}

Lambda Arae is a star in the southern constellation of Ara. Its name is a Bayer designation that is Latinized from λ Arae, and abbreviated Lambda Ara or λ Ara. The apparent visual magnitude of this star is 4.77, making it bright enough to be seen with the naked eye. Based on parallax measurements, it is located at a distance of {{Convert|68|ly|pc|abbr=off|lk=on}} from Earth. This star is drifting further away from the Sun with a radial velocity of +3 km/s.

The spectrum of this star matches a stellar classification of F4 V, which places it among the category of F-type main sequence stars. It is an estimated 2.4 billion years old, and is spinning with a projected rotational velocity of 15.5 km/s. This star has 40% more mass than the Sun and a 70% greater radius. It shines with 4.7 times the luminosity of the Sun. The outer atmosphere is radiating this energy at an effective temperature of 6,495 K, giving it the yellow-white hue of an F-type star. There is some evidence that this may be a binary star system consisting of two stars with identical masses.

Examination of Lambda Arae with the Spitzer Space Telescope shows an excess of infrared emission at a wavelength of 70 μm. This suggests it may be orbited by a disk of dust at a radius of more than 15 astronomical units

References

{{Reflist|30em|refs=

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{{cite simbad | title=lam Ara | accessdate=2010-07-30 | mode=cs2 | postscript=. }}

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}}