Alpha Equulei

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

{{Starbox begin

| name = α Equulei

}}

{{Starbox image

| image=

{{Location mark

|image=Equuleus constellation map.svg|alt=|float=center|width=260

|label=|position=right

|mark=Red circle.svg|mark_width=12|mark_link=α Equ

|x=449|y=701

}}

|caption=Location of α Equulei (circled)

}}

{{Starbox observe

| epoch = J2000.0

| constell = Equuleus

| ra = {{RA|21|15|49.43192}}

| dec = {{DEC|+05|14|52.2430}}

| appmag_v = +3.919{{cite journal|bibcode=1984SAAOC...8...59C|title=Standardization of Broadband Photometry of Equatorial Standards|journal=South African Astronomical Observatory Circulars|volume=8|pages=59|last1=Cousins|first1=A. W. J.|year=1984}}(4.49/4.96)

}}

{{Starbox character

| class = G7III + kA3hA4mA9

| b-v = +0.529

| u-b = +0.284

| variable=

}}

{{Starbox astrometry

| radial_v = −15.71 ± 0.05

| prop_mo_ra = {{nowrap|+59.88 ± 0.23}}

| prop_mo_dec = {{nowrap|−94.09 ± 0.18}}

| parallax = 17.14

| p_error = 0.21

| parallax_footnote = {{cite journal | title=Validation of the new Hipparcos reduction | url=http://www.aanda.org/articles/aa/full/2007/41/aa8357-07/aa8357-07.html | last1=van Leeuwen | first1=F. | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | year=2007 | arxiv=0708.1752 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 | s2cid=18759600 }}[http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=I/311/hip2&recno=117056 Vizier catalog entry ]

| dist_pc =

| absmag_v = +0.17 (0.71 + 1.18)

}}

{{Starbox orbit

| reference = {{cite journal|bibcode=2002MNRAS.330..288G|title=Composite spectra Paper 11: α Equulei, an astrometric binary with an Am secondary|journal=Monthly Notices of the Royal Astronomical Society|volume=330|issue=2|pages=288|last1=Griffin|first1=R. E. M.|last2=Griffin|first2=R. F.|year=2002|doi=10.1046/j.1365-8711.2002.05030.x|doi-access=free}}

| period_unitless = 98.8098 days

| eccentricity = 0

| k1 = 16.34 ± 0.07

| k2 = 17.9 ± 0.3

}}

{{Starbox detail

| component1 = A

| mass = 2.3

| radius = 9.2

| luminosity = 52.5

| temperature = 5,100

| metal_fe =

| gravity =

| rotational_velocity = 20.0

| component2 = B

| mass2 = 2.0

| radius2 = 2.6

| luminosity2 = 26.3

| temperature2 = 8.150

| age_myr2 =740

}}

{{Starbox catalog

| names = Kitalphar, 8 Equulei, HR 8131, HD 202447, BD+04 4635, HIP 104987, SAO 126662, FK5 800, GC 29735

}}

{{Starbox reference

| Simbad = Alpha+Equulei

}}

{{Starbox end}}

Alpha Equulei (α Equulei, abbreviated Alpha Equ, α Equ), officially named Kitalpha {{IPAc-en|k|I|'|t|æ|l|f|@}},{{cite book

|last1=Kunitzsch |first1=Paul

|last2=Smart |first2=Tim

|date = 2006 |edition = 2nd rev.

|title = A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations

|publisher = Sky Pub |location = Cambridge, Massachusetts

|isbn = 978-1-931559-44-7

}}{{cite web | url=http://www.pas.rochester.edu/~emamajek/WGSN/IAU-CSN.txt | title=IAU Catalog of Star Names |accessdate=28 July 2016}} is a star in the constellation of Equuleus. It is a high proper-motion star only 190 light-years away.

Nomenclature

α Equulei (Latinised to Alpha Equulei) is the star's Bayer designation.

It bore the traditional name Kitalpha (rarely Kitel Phard or Kitalphar), a contraction of the Arabic name قطعة الفرس qiṭ‘a(t) al-faras—"a piece of the horse". In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN){{citation

| url=https://www.iau.org/science/scientific_bodies/working_groups/280/

| title=IAU Working Group on Star Names (WGSN)

| publisher=International Astronomical Union

| accessdate=22 May 2016 | postscript=. }} to catalogue and standardize proper names for stars. The WGSN approved the name Kitalpha for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.

In Chinese, {{lang|zh|虚宿}} ({{lang|zh-Latn|Xū Sù}}), meaning Emptiness, is an asterism consisting of Alpha Equulei and Beta Aquarii.{{in lang|zh}} 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, {{ISBN|978-986-7332-25-7}}. Consequently, the Chinese name for Alpha Equulei itself is {{lang|zh|虛宿二}} ({{lang|zh-Latn|Xū Sù èr}}, {{langx|en|the Second Star of Emptiness}}).{{in lang|zh}} [http://www.lcsd.gov.hk/CE/Museum/Space/Research/StarName/c_research_chinengstars_h_l.htm 香港太空館 - 研究資源 - 亮星中英對照表] {{webarchive|url=https://web.archive.org/web/20110129031951/http://www.lcsd.gov.hk/CE/Museum/Space/Research/StarName/c_research_chinengstars_h_l.htm |date=2011-01-29 }}, Hong Kong Space Museum. Accessed on line November 23, 2010.

Properties

The overall appearance of α Equulei is a G-type giant{{cite journal|bibcode=1999A&AS..134..473G|title=Spectral classifications in the near infrared of stars with composite spectra. III. Study of a sample of 137 objects with the Aurelie spectrograph|journal=Astronomy and Astrophysics Supplement|volume=134|issue=3|pages=473|last1=Ginestet|first1=N.|last2=Carquillat|first2=J. M.|last3=Jaschek|first3=C.|year=1999|doi=10.1051/aas:1999444|doi-access=free}} with an apparent magnitude of +3.92, but it is a spectroscopic binary consisting of two individual stars.

The primary star is a G7 giant about fifty times more luminous than the Sun. It has an effective temperature of {{val|5100|ul=K|fmt=commas}} and a radius of 9.2 times greater than the Sun.

The secondary is an A-type dwarf about 26 times as luminous as the sun. It has an effective temperature of 8,150 K and a radius 2.6 times greater than the sun. It is a chemically peculiar Am star.

The two stars revolve in a circular orbit every 98.8 days. Their respective orbital velocities allow their masses to be calculated at {{solar mass|2.3}} and {{solar mass|2.0}}, respectively.

References

{{reflist|refs=

{{citation | last1=Pizzolato | first1=N. | last2=Maggio | first2=A. | last3=Sciortino | first3=S. | title=Evolution of X-ray activity of 1-3 Msun late-type stars in early post-main-sequence phases | journal=Astronomy and Astrophysics | volume=361 | pages=614–628 |date=September 2000 | bibcode=2000A&A...361..614P }}

}}

{{Stars of Equuleus}}

{{Authority control}}

{{DEFAULTSORT:Alpha Equulei}}

Equulei, Alpha

Category:Equuleus

Category:G-type giants

Category:A-type main-sequence stars

Category:Spectroscopic binaries

Kitalpha

104987

Equulei, 08

8131

202447

BD+04 4635