29 Arietis

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

{{Starbox begin}}

{{Starbox observe

| epoch = J2000.0

| equinox = J2000.0 (ICRS)

| constell = Aries

| ra = {{RA|02|32|54.14202}}

| dec = {{DEC|+15|02|04.3103}}

| appmag_v = 6.00

}}

{{Starbox character

| class = {{nowrap|F7 V + G5 V}} + ?

| b-v = {{Val|0.572|0.006}}

| u-b =

| r-i =

| variable =

}}

{{Starbox astrometry

| radial_v = {{Val|9.1|2.5}}

| prop_mo_ra = −20.557

| prop_mo_dec = +50.206

| parallax = 34.8568

| p_error = 0.1313

| parallax_footnote =

| absmag_v = 4.2/5.0

}}

{{Starbox orbit

| reference =

| period_unitless = {{Val|19.4161|0.0005|u=days}}

| eccentricity = {{Val|0.4096|0.0033}}

| node = {{Val|179.09|0.44}}

| periastron = {{Val|2454101.914|0.018|ul=JD|fmt=commas}}

| k1 = {{Val|23.36|0.09}}

}}

{{Starbox detail

| component1 = 29 Ari A

| mass = 1.14

| radius = {{Val|1.59|0.07|0.05}}

| luminosity = 3.27

| temperature = {{Val|6063|114|fmt=commas}}

| metal_fe = 0.09

| gravity = 4.12

| rotational_velocity =

| age_gyr = {{Val|3.0|1.8}}

| component2 = 29 Ari B

| mass2 = 0.88

| temperature2 = {{Val|5270|170|fmt=commas}}

}}

{{Starbox catalog

| names = {{odlist | F=29 Ari | BD=+14°419 | FK5=2176 | GJ=3161 | HD=15814 | HIP=11843 | HR=741 | SAO=92998 | WDS=J02329+1502 }}

}}

{{Starbox reference

| Simbad = 29+Ari

}}

{{Starbox end}}

29 Arietis is a triple star system in the northern constellation of Aries. 29 Arietis is the Flamsteed designation. Its annual parallax shift of {{val|34.86|0.13|ul=mas}} indicates a distance of about {{Convert|94|ly|pc|abbr=off|lk=on}} from Earth. The system is barely visible to the naked eye with an apparent visual magnitude of 6.0; it is 0.02 degree north of the ecliptic. It is moving further from Earth with a heliocentric radial velocity of 9 km/s.

The core of the system is formed by a close spectroscopic binary with an angular separation of 3.892 mas, a semimajor axis of {{Val|0.15692|0.00086|ul=AU}}, an orbital period of 19.4 days, and an eccentricity of 0.4. The larger member of this pair has 114% of the mass of the Sun, while its companion has 88% of the Sun's mass. Orbiting the pair at an angular separation of 1.422 arcseconds over a period of 164 years, the tertiary component has 52% of the Sun's mass.

References

{{Reflist|refs=

{{cite DR2|75349600571311744}}

{{cite simbad | title=29 Ari | access-date=2019-06-02}}

{{citation

| title=XHIP: An extended hipparcos compilation

| last1=Anderson | first1=E. | last2=Francis | first2=Ch.

| journal=Astronomy Letters | postscript=.

| volume=38 | issue=5 | pages=331 | year=2012

| bibcode=2012AstL...38..331A | arxiv=1108.4971

| doi=10.1134/S1063773712050015 | s2cid=119257644 }}

{{citation | display-authors=1

| last1=Tokovinin | first1=A. | last2=Thomas | first2=S.

| last3=Sterzik | first3=M. | last4=Udry | first4=S.

| title=Tertiary companions to close spectroscopic binaries

| journal=Astronomy and Astrophysics

| volume=450 | issue=2 | pages=681–693 | date=May 2006

| doi=10.1051/0004-6361:20054427 | postscript=.

| bibcode=2006A&A...450..681T | arxiv=astro-ph/0601518 | s2cid=8899546 }}

{{citation

| title=Determination of Orbital Elements of Spectroscopic Binaries Using High-dispersion Spectroscopy

| display-authors=1

| last1=Katoh | first1=Noriyuki | last2=Itoh | first2=Yoichi

| last3=Toyota | first3=Eri | last4=Sato | first4=Bun'ei

| journal=The Astronomical Journal | postscript=.

| volume=145 | issue=2 | id=41 | pages=12 | date=February 2013

| doi=10.1088/0004-6256/145/2/41 | bibcode=2013AJ....145...41K | doi-access=free }}

{{citation

| last1=Casagrande | first1=L. | last2=Schönrich | first2=R.

| last3=Asplund | first3=M. | last4=Cassisi | first4=S.

| last5=Ramírez | first5=I. | last6=Meléndez | first6=J.

| last7=Bensby | first7=T. | last8=Feltzing | first8=S.

| title=New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey

| display-authors=1 | journal=Astronomy and Astrophysics

| volume=530 | page=A138 | date=June 2011

| doi=10.1051/0004-6361/201016276 | postscript=.

| bibcode=2011A&A...530A.138C | arxiv=1103.4651 | s2cid=56118016 }}

{{citation

| title=The spectroscopic orbit of the double-lined binary 29 ARIETIS

| last1=Lu | first1=W. | postscript=.

| journal= Publications of the Astronomical Society of the Pacific

| volume=98 | pages=468–470 | date=April 1986

| doi=10.1086/131780 | bibcode=1986PASP...98..468L | doi-access=free }}

}}