HD 197037#Planetary system
{{short description|Binary star system in the constellation of Cygnus}}
{{Starbox begin
|name=HD 197037
}}
{{Starbox observe 2s
| epoch = J2000
| constell = Cygnus
| component1 = A
| dec1 = {{DEC|+42|14|54.7783}}
| component2 = B
| dec2 = {{DEC|+42|14|51.1696}}
| appmag_v2 =
}}
{{Starbox character
|component1=HD 197037 A
|component2=HD 197037 B
| type = main sequence
}}
{{Starbox astrometry
| component1 = A
| parallax = 30.2286
| p_error = 0.0143
| parallax_footnote = {{cite Gaia DR3|2066437688140905600}}
| component2 = B
| radial_v2 =
| parallax2 = 30.3173
| p_error2 = 0.0339
| parallax_footnote2 = {{cite Gaia DR3|2066437688141580928}}
| absmag_v2=
}}
{{Starbox relpos
| epoch = 2013
| primary = HD 197037 A
| component = HD 197037 B
| angdistsec = 3.676{{±|0.011}}
| angdistmas =
| angdistref =
| posang = 182.21{{±|0.18}}
| posangref =
| projsep = 121
| projsepref =
}}
{{Starbox detail
|component1=HD 197037 A
|component2=HD 197037 B
| mass = 1.063{{±|0.022}}
| mass2 = 0.3412{{±|0.0098|0.0477}}
| radius = 1.105{{±|0.023}}
| luminosity = 1.568{{±|0.074}}
| gravity = 4.37{{±|0.04}}
| metal_fe = −0.16{{±|0.03}}
| rotation = 19.1 d
| rotational_velocity =
| age_gyr = 3.408{{±|0.924}}
}}
{{Starbox catalog
| names = {{odlist|BD=+41 3845|2MASS = J20393296+4214549|HIP=101948|TYC=3161-126-1|LTT=16037|NLTT=49662|UBV=17937}}{{cite simbad|title=HD 197037|access-date=2021-01-19}}
}}
{{Starbox reference
| Simbad = HD+197037
}}
{{Starbox end}}
HD 197037 is a binary star system. Its primary or visible star, HD 197037 A, is a F-type main-sequence star. Its surface temperature is 6150{{±|34}} K. HD 197037 A is depleted in heavy elements compared to the Sun, with a metallicity Fe/H index of −0.16{{±|0.03}}, but is younger at an age of 3.408{{±|0.924}} billion years.
A multiplicity survey detected a red dwarf stellar companion HD 197037 B in 2016, at a projected separation of 121 AU.{{citation |arxiv=1601.01524 |doi=10.1093/mnras/stw049 |title=A lucky imaging multiplicity study of exoplanet host stars – II |year=2016 |last1=Ginski |first1=C. |last2=Mugrauer |first2=M. |last3=Seeliger |first3=M. |last4=Buder |first4=S. |last5=Errmann |first5=R. |last6=Avenhaus |first6=H. |last7=Mouillet |first7=D. |last8=Maire |first8=A.-L. |last9=Raetz |first9=S. |journal=Monthly Notices of the Royal Astronomical Society |volume=457 |issue=2 |pages=2173–2191 |doi-access=free |bibcode=2016MNRAS.457.2173G |s2cid=53626523 }} The existence of other stellar companions at projected separations from 1.62 to 45.26 AU was excluded.
Planetary system
In 2012 one planet, named HD 197037 Ab, was discovered on a wide, eccentric orbit by the radial velocity method.{{citation |arxiv=1202.0265 |doi=10.1088/0004-637X/749/1/39 |last1=Robertson |first1=Paul |last2=Endl |first2=Michael |last3=Cochran |first3=William D. |last4=MacQueen |first4=Phillip J. |last5=Wittenmyer |first5=Robert A. |last6=Horner |first6=J. |last7=Brugamyer |first7=Erik J. |last8=Simon |first8=Attila E. |last9=Barnes |first9=Stuart I. |last10=Caldwell |first10=Caroline |title=THE McDONALD OBSERVATORY PLANET SEARCH: NEW LONG-PERIOD GIANT PLANETS AND TWO INTERACTING JUPITERS IN THE HD 155358 SYSTEM |journal=The Astrophysical Journal |date=2012 |volume=749 |issue=1 |page=39 |bibcode=2012ApJ...749...39R |s2cid=59273311 }}
Another planet in the system was initially suspected, but the radial velocity signal was later attributed to the stellar companion HD 197037 B.
{{OrbitboxPlanet begin
| name = HD 197037 A
}}
{{OrbitboxPlanet
| exoplanet = b
| mass = ≥0.79{{±|0.05}}
| radius =
| semimajor = 2.07{{±|0.05}}
| period = 1035.7{{±|13}}
| eccentricity = 0.22{{±|0.07}}
| inclination =
}}
{{Orbitbox end}}
References
{{Reflist}}
{{Sky|20|39|32.9601|+|42|14|54.7736}}
{{Stars of Cygnus}}
Category:Cygnus (constellation)
Category:Planetary transit variables
Category:F-type main-sequence stars