nu1 Sagittarii

{{short description|Triple star system in the constellation Sagittarius}}

{{DISPLAYTITLE:Nu1 Sagittarii}}

{{other stars by Bayer designation|Nu Sagittarii{{!}}ν Sagittarii}}

{{Starbox begin

| name = Nu1 Sagittarii

}}

{{Starbox image

| image =

File:Sagittarius IAU.svg

| caption = Location of ν1 Sagittarii (circled)

}}

{{Starbox observe

| epoch = J2000.0

| equinox = J2000.0 (ICRS)

| constell = Sagittarius

| ra = {{RA|18|54|10.17695}}

| dec = {{DEC|−22|44|41.4247}}

| appmag_v = +4.86

}}

{{Starbox character

| class = {{nowrap|G2/K1 Ib/II + B9.2p}}

| b-v = +1.43

| u-b = +1.34

| variable =

}}

{{Starbox astrometry

| radial_v = −11.57

| prop_mo_ra = +4.291

| prop_mo_dec = −7.786

| parallax = 2.3170

| p_error = 0.2139

| parallax_footnote =

| absmag_v = −3.91

}}

{{Starbox detail

| source =

| mass =

| radius = 101

| luminosity = 3,464

| temperature = 4,401

| gravity =

| metal_fe =

| rotational_velocity =

| age_gyr =

}}

{{Starbox catalog

| names = {{odlist | name=Ainalrami | B=ν1 Sgr | F=32 Sgr | BD=−22°4907 | HD=174974 | HIP=92761 | HR=7116 | SAO=187426 | WDS=J18542-2245 }}

}}

{{Starbox reference

| Simbad = nu.01+Sgr

}}

{{Starbox end}}

Nu1 Sagittarii (ν1 Sagittarii, abbreviated Nu1 Sgr, ν1 Sgr) is a triple star system about 1,100 light-years from Earth. Its three components are designated Nu1 Sagittarii A (officially named Ainalrami {{IPAc-en|E|n|@l|'|r|ei|m|i}}, the traditional name for the system),{{cite web | url=https://www.iau.org/public/themes/naming_stars/ | title=Naming Stars |publisher=IAU.org |access-date=16 December 2017}} B and C. A and B themselves form a spectroscopic binary. The system is 0.11 degree north of the ecliptic.

Nomenclature

ν1 Sagittarii (Latinised to Nu1 Sagittarii) is the system's Bayer designation.

Nu1 and Nu2 Sagittarii (together designated Nu Sagittarii) bore the traditional name Ain al Rami, which is from the Arabic عين الرامي ʽain al-rāmī meaning 'eye of the archer'. In 2016, the IAU organized a Working Group on Star Names (WGSN){{cite web | url=https://www.iau.org/science/scientific_bodies/working_groups/280/ | title=IAU Working Group on Star Names (WGSN)|access-date=22 May 2016}} to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.{{cite web | url=https://www.iau.org/static/science/scientific_bodies/working_groups/280/wg-starnames-triennial-report-2015-2018.pdf | page=5 | title=WG Triennial Report (2015-2018) - Star Names |access-date=2018-07-14}} It approved the name Ainalrami for the component Nu1 Sagittarii A on 5 September 2017 and it is now so included in the List of IAU-approved Star Names.

Nu1 and Nu2 Sagittarii, together with Tau Sagittarii, Psi Sagittarii, Omega Sagittarii, 60 Sagittarii and Zeta Sagittarii were Al Udḥiyy, the Ostrich's Nest.

Properties

Nu1 Sagittarii A is a spectral type K1 bright giant which has an apparent magnitude of +4.86. It is a microvariable with a frequency of 0.43398 cycles per day and an amplitude of 0.0078 magnitude. In 1982 it was found to have a hotter companion, Nu1 Sagittarii B, a rapidly rotating B9 type star. The pair orbit with a period of around 370 days. A magnitude +11.2 companion, component C, is orbiting further out at an angular separation of 2.5 arcseconds from the primary.

Observation

On 13 February 2008, it was occulted by Jupiter as viewed from East Asia and the Indian Ocean.{{cite book |date=2002 |first=Jan |last=Meeus |chapter=Mutual occultations of planets |pages=174–185 |title=More Mathematical Astronomy Morsels |isbn=0943396743 |url=https://falakmu.id/khgt/dokumen/More%20mathematical%20astronomy%20morsels%20(Jean%20Meeus)%20(Z-Library).pdf}}{{rp|164}}

References

{{reflist|refs=

{{cite book

| last=Allen

| first=R. H.

| year=1963

| author-link=Richard Hinckley Allen

| title=Star Names: Their Lore and Meaning

| url=https://archive.org/details/starnamestheirlo00alle/page/355

| access-date=2012-09-04

| edition=Reprint

| publisher=Dover Publications Inc

| location=New York

| isbn=0-486-21079-0

| page=[https://archive.org/details/starnamestheirlo00alle/page/355 355]

| url-access=registration

}}

{{citation

| title=The early-type component in ν¹ Sagittarii

| display-authors=1 | last1=Kondo | first1=Y.

| last2=McCluskey | first2=G. E. | last3=Wu | first3=C.-C.

| journal=Publications of the Astronomical Society of the Pacific

| volume=94 | pages=647–649 | date=August 1982 | postscript=.

| doi=10.1086/131037 | bibcode=1982PASP...94..647K | doi-access=free }}

{{citation

| title=Mg II chromospheric radiative loss rates in cool active and quiet stars

| last1=Cardini | first1=D. | postscript=.

| journal=Astronomy and Astrophysics

| volume=430 | pages=303–311 | date=January 2005

| doi=10.1051/0004-6361:20041440 | bibcode=2005A&A...430..303C |arxiv = astro-ph/0409683 | s2cid=12136256 }}

{{citation | postscript=.

| title=New periodic variables from the Hipparcos epoch photometry

| journal=Monthly Notices of the Royal Astronomical Society

| last1=Koen | first1=Chris | last2=Eyer | first2=Laurent

| volume=331 | pages=45–59 | year=2002 | issue=1

| arxiv=astro-ph/0112194

| doi=10.1046/j.1365-8711.2002.05150.x | doi-access=free

| bibcode=2002MNRAS.331...45K | s2cid=10505995

}}

{{citation

| last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A.

| title=A catalogue of multiplicity among bright stellar systems

| journal=Monthly Notices of the Royal Astronomical Society

| volume=389 | issue=2 | pages=869–879 | date=September 2008

| bibcode=2008MNRAS.389..869E | doi=10.1111/j.1365-2966.2008.13596.x

| doi-access=free | arxiv=0806.2878 | s2cid=14878976 | postscript=. }}

{{citation

| last1=Lutz | first1=T. E. | last2=Lutz | first2=J. H.|author2-link= Julie Lutz

| title=Spectral classification and UBV photometry of bright visual double stars

| journal=Astronomical Journal | postscript=.

| volume=82 | pages=431–434 |date=June 1977

| doi=10.1086/112066 | bibcode=1977AJ.....82..431L | doi-access=free }}

{{citation

| title=Validation of the new Hipparcos reduction

| last1=van Leeuwen | first1=F.

| journal=Astronomy and Astrophysics

| volume=474 | issue=2 | pages=653–664 | date=2007

| arxiv=0708.1752 | bibcode=2007A&A...474..653V

| doi=10.1051/0004-6361:20078357 | s2cid=18759600 | postscript=. }}

{{citation

| last1=Parsons | first1=Sidney B. | last2=Ake | first2=Thomas B.

| title= Ultraviolet and Optical Studies of Binaries with Luminous Cool Primaries and Hot Companions. V. The Entire IUE Sample

| journal=The Astrophysical Journal Supplement Series

| volume=119 | pages=83 | year=1998 | issue=1 | postscript=.

| bibcode= 1998ApJS..119...83P | doi= 10.1086/313152 | doi-access=free }}

{{cite simbad

| title=nu01 Sgr | access-date=2017-07-06 | postscript=. }}

{{cite web | url=http://ad.usno.navy.mil/wds/ | title=Washington Double Star Catalog | publisher=United States Naval Observatory | access-date=2 January 2018 | archive-url=https://web.archive.org/web/20110214155533/http://ad.usno.navy.mil/wds/ | archive-date=14 February 2011 | url-status=dead }}

{{cite DR2|4075705783885296640}}

}}

{{Stars of Sagittarius|state=collapsed}}

{{DEFAULTSORT:Nu1 Sagittarii}}

Category:K-type bright giants

Category:K-type supergiants

Category:B-type stars

Sagittarii, Nu

Category:Sagittarius (constellation)

BD-22 4907

Sagittarii, 32

174974

092761

7116

Category:Spectroscopic binaries

Ainalrami