Phi3 Hydrae

{{Short description|Binary star system in the constellation Hydra}}

{{DISPLAYTITLE:Phi3 Hydrae}}

{{hatnote|For other stars with this Bayer designation, see φ Hydrae}}

{{Starbox begin

| name = Phi3 Hydrae

}}

{{Starbox observe

| epoch = J2000.0

| equinox = J2000.0 (ICRS)

| constell = Hydra

| ra = {{RA|10|38|34.95281}}

| dec = {{DEC|-16|52|35.6665}}

| appmag_v = 4.90

}}

{{Starbox character

| type = red clump

| class = G8 III

| b-v = 0.912

| u-b =

| r-i =

| variable =

}}

{{Starbox astrometry

| radial_v = {{Val|+17.45|0.70}}

| prop_mo_ra = −98.92

| prop_mo_dec = +25.84

| parallax = 15.49

| p_error = 0.57

| parallax_footnote =

| absmag_v = +0.89

}}

{{Starbox orbit

| reference =

| period_unitless = 1200 d

| axis =

| axis_unitless =

| eccentricity = 0.1

| inclination =

| node =

| periastron = 2420760 JD

| periarg = 270

| k1 = 4.0

}}

{{Starbox detail

| source =

| component1 = φ3 Hya

| mass = 2.04

| radius = 9

| luminosity = 48

| temperature = {{Val|4952|17|fmt=commas}}

| gravity = 2.95

| metal_fe = {{Val|−0.22|0.12}}

| rotational_velocity = 3.6

| age_gyr = 1.17

}}

{{Starbox catalog

| names = φ3 Hya, BD−16°3100, FK5 2850, HD 92214, HIP 52085, HR 4171, SAO 156122

}}

{{Starbox reference

| Simbad = phi03+Hya

}}

{{Starbox end}}

Phi3 Hydrae (φ3 Hya) is a binary star in the equatorial constellation of Hydra. It originally received the Flamsteed designation of 2 Crateris before being placed in the Hydra constellation. Based upon an annual parallax shift of 15.49 mas as seen from Earth, it is located around 211 light years from the Sun. It is visible to the naked eye with an apparent visual magnitude of 4.90. It forms a triangle with the fainter φ1 Hydrae and φ2 Hydrae, between μ Hydrae and ν Hydrae.

This is a single-lined spectroscopic binary star system with an orbital period of about 1,200 days and an eccentricity of 0.1. The primary, component A, is an evolved G-type giant star with a stellar classification of G8 III. It is a red clump star, which means it is generating energy through the fusion of helium at its core. The star has twice the mass of the Sun and has expanded to 9 times the Sun's radius. It is 1.17 billion years old and is radiating 48 times the solar luminosity from its photosphere at an effective temperature of 4,952 K.

References

{{reflist|refs=

{{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

| title=A new Large Magellanic Cloud K-band distance from precision measurements of nearby red clump stars

| display-authors=1 | last1=Laney | first1=C. D.

| last2=Joner | first2=M. D. | last3=Pietrzyński | first3=G.

| journal=Monthly Notices of the Royal Astronomical Society

| volume=419 | issue=2 | pages=1637–1641 | date=January 2012

| doi=10.1111/j.1365-2966.2011.19826.x | doi-access=free | bibcode=2012MNRAS.419.1637L

| arxiv=1109.4800 | s2cid=117788450 | postscript=. }}

{{citation

| display-authors=1 | postscript=.

| last1=Massarotti | first1=Alessandro | last2=Latham | first2=David W.

| last3=Stefanik | first3=Robert P. | last4=Fogel | first4=Jeffrey

| title=Rotational and radial velocities for a sample of 761 HIPPARCOS giants and the role of binarity

| journal=The Astronomical Journal

| volume=135 | issue=1 | pages=209–231 | date=January 2008

| doi=10.1088/0004-6256/135/1/209 | bibcode=2008AJ....135..209M | s2cid=121883397

| doi-access=free }}

{{citation

| title=High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances

| journal=The Astrophysical Journal Supplement Series

| volume=74 | pages=1075 | year=1990

| last1=McWilliam | first1=Andrew | postscript=.

| doi=10.1086/191527 | bibcode=1990ApJS...74.1075M | doi-access=free }}

{{citation

| last1=de Bruijne | first1=J. H. J. | last2=Eilers | first2=A.-C.

| title=Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project

| journal=Astronomy & Astrophysics

| volume=546 | id=A61 | pages=14 | date=October 2012

| doi=10.1051/0004-6361/201219219 | bibcode=2012A&A...546A..61D

| arxiv=1208.3048 | s2cid=59451347 | postscript=. }}

{{citation

| title=Abundances in the Local Region. I. G and K Giants

| last1=Luck | first1=R. Earle

| journal=The Astronomical Journal

| volume=150 | issue=3 | id=88 | pages=23 | date=September 2015

| doi=10.1088/0004-6256/150/3/88 | bibcode=2015AJ....150...88L

| arxiv=1507.01466 | s2cid=118505114 | postscript=. }}

{{citation

| display-authors=1 | last1=Pourbaix | first1=D.

| last2=Tokovinin | first2=A. A. | last3=Batten | first3=A. H.

| last4=Fekel | first4=F. C. | last5=Hartkopf | first5=W. I.

| last6=Levato | first6=H. | last7=Morrell | first7=N. I.

| last8=Torres | first8=G. | last9=Udry | first9=S.

| title=SB9: The ninth catalogue of spectroscopic binary orbits

| journal=Astronomy and Astrophysics

| volume=424 | pages=727–732 | date=September 2004

| bibcode=2004A&A...424..727P | doi=10.1051/0004-6361:20041213

| arxiv=astro-ph/0406573 | s2cid=119387088 | postscript=. }}

{{citation

| last=Wagman | first=M. | postscript=.

| title=Flamsteed's Missing Stars

| journal=Journal for the History of Astronomy

| volume=18 | page=216 |date=August 1987

| issue=3 | bibcode=1987JHA....18..209W | doi=10.1177/002182868701800305| s2cid=118445625 }}

{{cite simbad

| title=phi Hya

| access-date=2017-03-17 }}

}}

{{Stars of Hydra|state=collapsed}}

{{DEFAULTSORT:Phi3 Hydrae}}

Category:G-type giants

Category:Horizontal-branch stars

Category:Spectroscopic binaries

Category:Hydra (constellation)

Hydrae, Phi3

Category:Durchmusterung objects

Crateris, 2

092214

052085

4171