KOI-5
KOI-5 | ||
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はくちょう | ||
1+1? | ||
19h 18m 57.5s[1] | ||
44° 38′ 51″[1] | ||
-35.16 km/s[2] | ||
1.7436 ± 0.0666ミリ ( | ||
1870 ± 70 (570 ± 20 パーセク[ | ||
A:1.840±0.017 R☉[3] | ||
A:1.13 M☉[4] B:1.09 M☉[4] | ||
A:4.19 cgs[5] | ||
A:3.86±0.17 L☉[3] | ||
A:5861 K[5] | ||
A:34.9±4.1 | ||
TOI-1241 2MASS J19185753+4438507 KIC 8554498 Gaia EDR3 2126945668448657664 |
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■Template (■ノート ■ |
KOI-5とは、
KOI-5A
惑星 系 [編集 ]
ケプラー
( |
( |
( |
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b | 56.89157 M⊕ | — | 4.780327766±8.76e-07 | — | 82.51° | 7.07531±0.16815 R⊕ |
脚注 [編集 ]
注釈 [編集 ]
出典 [編集 ]
- ^ a b c “Catalog”.
太陽系 外 惑星 エンサイクロペディア. 2020年 1月 18日 閲覧 。 - ^ a b c d Gaia Early Data Release 3: Summary of the contents and survey properties
- ^ a b c Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy, (2018), arXiv:1812.06979
- ^ a b c d e AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE
- ^ a b Planetary Candidates Observed by Kepler III: Analysis of the First 16 Months of Data, (2012), arXiv:1202.5852
- ^ THE KEPLER FOLLOW-UP OBSERVATION PROGRAM. I. A CATALOG OF COMPANIONS TO KEPLER STARS FROM HIGH-RESOLUTION IMAGING, (2016), arXiv:1612.02392
- ^ a b ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH-RESOLUTION IMAGING OF Kepler OBJECTS OF INTEREST, (2017), arXiv:1701.06577