Proxima Centauri b: Perbedaan antara revisi

{{Planetbox image

| image = Artist's impression of the planet orbiting Proxima Centauri.jpg

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{{Planetbox star

|dec = {{DEC|−62|40|46.1631}}

|dist_ly = 4.224

|class = M6Ve<ref name=aaa460_3_695>{{cite journal

|last=Torres | first=C. A. O.

|first6=M. }}</ref>

|app_mag = 11.13

|radius = 0.141 (± 0.007)<ref name=aaa505_1_205>{{cite journal |last1=Demory |first1=B.-O. |last2=Ségransan |first2=D. |last3=Forveille | first3=T. |last4=Queloz |first4=D. |last5=Beuzit |first5=J.-L. |last6=Delfosse |first6=X. |last7=Di Folco |first7=E. |last8=Kervella |first8=P. |last9=Le Bouquin |first9=J.-B. |date=October 2009 |title=Mass-radius relation of low and very low-mass stars revisited with the VLTI | journal=Astronomy and Astrophysics |volume=505 |issue=1 |pages=205–215 |doi=10.1051/0004-6361/200911976 |bibcode=2009A&A...505..205D |arxiv = 0906.0602 }}</ref>

|temperature = 3042 (± 117)<ref name=aaa397>{{cite journal |last1=Ségransan |first1=D. |last2=Kervella |first2=P. |last3=Forveille |first3=T. |last4=Queloz |first4=D. |title=First radius measurements of very low mass stars with the VLTI |journal=Astronomy and Astrophysics |date=2003 |volume=397 |issue=3 |pages=L5–L8 |doi=10.1051/0004-6361:20021714 |bibcode=2003A&A...397L...5S |arxiv = astro-ph/0211647 }}</ref>

|age = 4.85<ref name=aaa519_A105>{{cite journal |last1=Schlaufman |first1=K. C. |last2=Laughlin |first2=G. |title=A {{Sic|hide=y|physically|-}}motivated photometric calibration of M dwarf metallicity |journal=Astronomy and Astrophysics |volume=519 |date=September 2010 |doi=10.1051/0004-6361/201015016 |bibcode=2010A&A...519A.105S |arxiv = 1006.2850 |pages=A105}}</ref>

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{{Planetbox character

| temperature = {{convert|234|K|C F}}

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{{Planetbox orbit

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{{Planetbox discovery

| discovery_date = 24 August 2016

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{{Planetbox reference