WASP-35

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

{{Starbox begin

| name = WASP-35

}}

{{Starbox observe

| epoch = J2000

| ra = {{RA|05|04|19.6323}}

| dec = {{DEC|−06|13|47.378}}

| constell = Eridanus

| appmag_v = 10.94

}}

{{Starbox character

| class = G0V

}}

{{Starbox astrometry

| radial_v = 16.96

| prop_mo_ra = {{val|20.758|(15)}}

| prop_mo_dec = {{val|10.963|(11)}}

| pm_footnote =

| parallax = 4.9411

| p_error = 0.0160

| parallax_footnote =

}}

{{Starbox detail

| source = {{citation|arxiv=1309.1998|title=New and updated stellar parameters for 90 transit hosts The effect of the surface gravity|year=2013|doi=10.1051/0004-6361/201322240|last1=Mortier|first1=A.|last2=Santos|first2=N. C.|last3=Sousa|first3=S. G.|last4=Fernandes|first4=J. M.|last5=Adibekyan|first5=V. Zh.|last6=Delgado Mena|first6=E.|last7=Montalto|first7=M.|last8=Israelian|first8=G.|journal=Astronomy and Astrophysics|volume=558|pages=A106|bibcode=2013A&A...558A.106M|s2cid=118750676}}{{citation|arxiv=1704.00373|title=The GAPS Programme with HARPS-N@TNG XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets|year=2017|doi=10.1051/0004-6361/201629882|last1=Bonomo|first1=A. S.|last2=Desidera|first2=S.|last3=Benatti|first3=S.|last4=Borsa|first4=F.|last5=Crespi|first5=S.|last6=Damasso|first6=M.|last7=Lanza|first7=A. F.|last8=Sozzetti|first8=A.|last9=Lodato|first9=G.|last10=Marzari|first10=F.|last11=Boccato|first11=C.|last12=Claudi|first12=R. U.|last13=Cosentino|first13=R.|last14=Covino|first14=E.|last15=Gratton|first15=R.|last16=Maggio|first16=A.|last17=Micela|first17=G.|last18=Molinari|first18=E.|last19=Pagano|first19=I.|last20=Piotto|first20=G.|last21=Poretti|first21=E.|last22=Smareglia|first22=R.|last23=Affer|first23=L.|last24=Biazzo|first24=K.|last25=Bignamini|first25=A.|last26=Esposito|first26=M.|last27=Giacobbe|first27=P.|last28=Hébrard|first28=G.|last29=Malavolta|first29=L.|last30=Maldonado|first30=J.|journal=Astronomy & Astrophysics|volume=A107|page=602|bibcode=2017A&A...602A.107B|s2cid=118923163|display-authors=29}}

| mass = 1.06{{±|0.08}}

| radius = 1.09{{±|0.02}}

| gravity = 4.39{{±|0.02}}

| luminosity =

| temperature = 6072{{±|62}}

| metal_fe = 0.01{{±|0.05}}

| rotation =

| rotational_velocity = 2.4{{±|0.6}}

| age_gyr = 5.0{{±|1.2}}

}}

{{Starbox catalog

| names = {{odlist|BD=-06 1077|TYC=4762-714-1|GSC=04762-00714|2MASS=J05041962-0613473|Gaia DR2=3211188618762023424}}

}}

{{Starbox reference

| Simbad = WASP-35

}}

{{Starbox end}}

WASP-35 is a G-type main-sequence star about 660 light-years away. The star's age cannot be well constrained, but it is probably older than the Sun. WASP-35 is similar in concentration of heavy elements compared to the Sun.{{citation |bibcode=2014A&A...572A..95M |title=Correcting the spectroscopic surface gravity using transits and asteroseismology. No significant effect on temperatures or metallicities with ARES and MOOG in local thermodynamic equilibrium |last1=Mortier |first1=A. |last2=Sousa |first2=S. G. |last3=Adibekyan |first3=V. Zh. |last4=Brandão |first4=I. M. |last5=Santos |first5=N. C. |journal=Astronomy and Astrophysics |year=2014 |volume=572 |pages=A95 |doi=10.1051/0004-6361/201424537 |arxiv=1410.1310 |s2cid=73621824 }}

The star has no detectable starspot activity. An imaging survey in 2015 found no detectable stellar companions,{{citation|arxiv=1506.05456|title=A Lucky Imaging search for stellar sources near 74 transit hosts|year=2015|doi=10.1051/0004-6361/201526525|last1=Wöllert|first1=Maria|last2=Brandner|first2=Wolfgang|journal=Astronomy & Astrophysics|volume=579|pages=A129|bibcode=2015A&A...579A.129W|s2cid=118903879}} although a spectroscopic survey in 2016 yielded a suspected red dwarf companion with a temperature of {{val|3800|1100|ul=K}}.{{citation|arxiv=1603.03274|title=High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). I. Lucky imaging observations of 101 systems in the southern hemisphere|year=2016|doi=10.1051/0004-6361/201527970|last1=Evans|first1=D. F.|last2=Southworth|first2=J.|last3=Maxted|first3=P. F. L.|last4=Skottfelt|first4=J.|last5=Hundertmark|first5=M.|last6=Jørgensen|first6=U. G.|last7=Dominik|first7=M.|last8=Alsubai|first8=K. A.|last9=Andersen|first9=M. I.|last10=Bozza|first10=V.|last11=Bramich|first11=D. M.|last12=Burgdorf|first12=M. J.|last13=Ciceri|first13=S.|last14=d'Ago|first14=G.|last15=Figuera Jaimes|first15=R.|last16=Gu|first16=S.-H.|last17=Haugbølle|first17=T.|last18=Hinse|first18=T. C.|last19=Juncher|first19=D.|last20=Kains|first20=N.|last21=Kerins|first21=E.|last22=Korhonen|first22=H.|last23=Kuffmeier|first23=M.|last24=Mancini|first24=L.|last25=Peixinho|first25=N.|last26=Popovas|first26=A.|last27=Rabus|first27=M.|last28=Rahvar|first28=S.|last29=Schmidt|first29=R. W.|last30=Snodgrass|first30=C.|journal=Astronomy & Astrophysics|volume=589|pages=A58|bibcode=2016A&A...589A..58E|s2cid=14215845|display-authors=29}}