| 词条 | HD 186302 |
| 释义 |
| name = HD 186302 }}{{Starbox image | image={{Location mark |image=HD186302_starmap.png|alt=|float=center|width=320 |label=|position=right |mark=Red circle.svg|mark_width=10|mark_link=HD 186302 |x=480|y=600 }} |caption=Location of HD 186302 (circled) }}{{Starbox observe | epoch=J2000 | ra={{RA|19|49|6.43}} | dec={{DEC|-70|11|16.7}} | appmag_v=8.76 | constell=Pavo }}{{Starbox character | class = G3/5V | b-v = 0.67 }}{{Starbox astrometry | prop_mo_ra =-23.954 | prop_mo_dec =-38.710 | parallax = 17.7148 | p_error = 0.0310 | parallax_footnote = | absmag_v = }}{{Starbox detail | mass = | radius = | gravity = | temperature = 5817 | metal_fe = | age_gyr = }}{{Starbox catalog | names = HD 186302, HIP 97507, 2MASS J19490644-7011167, Gaia DR2 6423349579465419392 }}{{Starbox reference | Simbad = HD+186302 | EPE = | ARICNS = }}{{Starbox end}}HD 186302 (also designated HIP 97507) is a star in the constellation of Pavo. It is about {{convert|184|ly|pc|abbr=off|lk=on}} away from Earth, with an apparent magnitude of 8.76. It was identified in November 2018 as a potential solar sibling to the Sun. It is very similar to the Sun; the Sun is a G2V star. Similar by spectrum and size, it may have formed in the same stellar nursery as the Sun 4.57 billion years ago.[1] See also
References1. ^Did Astronomers Just Find The Sun’s Sister? Bob P. King, November 24, 2018 }} External links
6 : Solar twins|G-type main-sequence stars|Henry Draper Catalogue objects|Hipparcos objects|2MASS objects|Pavo (constellation) |
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