WASP-67#Planetary system

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

{{Starbox begin}}

{{Starbox observe

| epoch = J2000

| constell = Sagittarius

| ra = {{RA|19|42|58.5218}}

| dec = {{DEC|-19|56|58.521}}

| appmag_v = 12.54

}}

{{Starbox character

| type=Main sequence

| class = K0V

}}

{{Starbox astrometry

| radial_v = {{val|-0.76|0.80}}

| prop_mo_ra = +1.647

| prop_mo_dec = −33.032

| parallax = 5.2720

| p_error = 0.0123

| parallax_footnote = {{cite Gaia DR3|6868476691490044672}}

}}

{{Starbox detail

| source =

| mass = {{val|0.91|0.28}}

| radius = {{val|0.88|0.08}}

| gravity = {{val|4.35|0.15}}

| luminosity = 0.51{{cite journal

| title=Revised Exoplanet Radii and Habitability Using Gaia Data Release 2

| last1=Johns | first1=Daniel | last2=Marti | first2=Connor

| last3=Huff | first3=Madison | last4=McCann | first4=Jacob

| last5=Wittenmyer | first5=Robert A. | last6=Horner | first6=Jonathan

| last7=Wright | first7=Duncan J. | display-authors=1

| journal=The Astrophysical Journal Supplement Series

| volume=239 | issue=1 | id=14 | date=November 2018

| page=14 | arxiv=1808.04533 | doi=10.3847/1538-4365/aae5fb

| bibcode=2018ApJS..239...14J | doi-access=free }}

| temperature = {{val|5200|100}}

| metal_fe = −0.07

| rotation =

| rotational_velocity = {{val|2.1|0.4}}

| age_gyr = {{val|4.3|3.1}}{{cite journal |bibcode=2022ApJ...925..164H |title=Beyond Spectroscopy. I. Metallicities, Distances, and Age Estimates for over 20 Million Stars from SMSS DR2 and Gaia EDR3 |last1=Huang |first1=Yang |last2=Beers |first2=Timothy C. |last3=Wolf |first3=Christian |last4=Lee |first4=Young Sun |last5=Onken |first5=Christopher A. |last6=Yuan |first6=Haibo |last7=Shank |first7=Derek |last8=Zhang |first8=Huawei |last9=Wang |first9=Chun |last10=Shi |first10=Jianrong |last11=Fan |first11=Zhou |journal=The Astrophysical Journal |date=2022 |volume=925 |issue=2 |page=164 |doi=10.3847/1538-4357/ac21cb |doi-access=free |arxiv=2104.14154 }}

}}

{{Starbox catalog

| names = {{odlist|WASP=67|TYC=6307-1388-1|2MASS=J19425852-1956585|Gaia DR2=6868476691490044672}}

}}

{{Starbox reference

| Simbad = WASP-67

}}

{{Starbox end}}

WASP-67 is a K-type main-sequence star about 620 light-years away. The star's age is poorly constrained. WASP-67 is slightly depleted in heavy elements, having 85% of the solar abundance of iron.

A multiplicity survey in 2016 has found one candidate stellar companion to WASP-67 at a projected separation of {{val|4.422|0.018|ul="}}.{{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}} Nonetheless, follow-up observations in 2017 failed to find any bound stellar companions.{{citation|arxiv=1709.07476|title=High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016|year=2018|doi=10.1051/0004-6361/201731855|last1=Evans|first1=D. F.|last2=Southworth|first2=J.|last3=Smalley|first3=B.|last4=Jørgensen|first4=U. G.|last5=Dominik|first5=M.|last6=Andersen|first6=M. I.|last7=Bozza|first7=V.|last8=Bramich|first8=D. M.|last9=Burgdorf|first9=M. J.|last10=Ciceri|first10=S.|last11=d'Ago|first11=G.|last12=Figuera Jaimes|first12=R.|last13=Gu|first13=S.-H.|last14=Hinse|first14=T. C.|last15=Henning|first15=Th.|last16=Hundertmark|first16=M.|last17=Kains|first17=N.|last18=Kerins|first18=E.|last19=Korhonen|first19=H.|last20=Kokotanekova|first20=R.|last21=Kuffmeier|first21=M.|last22=Longa-Peña|first22=P.|last23=Mancini|first23=L.|last24=MacKenzie|first24=J.|last25=Popovas|first25=A.|last26=Rabus|first26=M.|last27=Rahvar|first27=S.|last28=Sajadian|first28=S.|last29=Snodgrass|first29=C.|last30=Skottfelt|first30=J.|journal=Astronomy & Astrophysics|volume=610|pages=A20|bibcode=2018A&A...610A..20E|s2cid=53400492|display-authors=29}}