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Baris 91: \| Jari-jari terpendek \|[[SDSS J1228+1040 b]] \|[[SDSS J1228+1040 ]] \| 126  km<ref>{{Cite web\|url=http://exoplanet.eu/catalog/sdss_j1228+1040_b/\|title=Planet SDSS J1228+1040 b\|website=exoplanet.eu\|access-date=2019-08-05}}</ref> \| \|- Baris 169: \| [[HD 20782]] \| {{val\|0.956\|0.004}} \| <ref>{{Cite web\|url=http://exoplanet.eu/catalog/hd_20782_b/\|title=The Extrasolar Planet Encyclopaedia — HD 20782 b\|website=exoplanet.eu\|access-date=2019-05-04}}</ref> Record among confirmed planets. Putative satellite of [[VB 10]] may have higher eccentricity of 0.98.<ref>{{Cite web\|url=http://exoplanet.eu/catalog/vb_10_b/\|title=The Extrasolar Planet Encyclopaedia — VB 10 b\|website=exoplanet.eu\|access-date=2020-02-12}}</ref> \|- <!-- "Least eccentric" makes no sense: there are many planets with e = 0 measurements Baris 316: \| {{nowrap\|[[2MASS J1119–1137 ]]}} \| {{Solar mass\|0.0033}} \| The system 2MASS J1119-1137 AB is a pair of binary rogue planets approximately 3.7 Jupiter masses each.<ref>{{cite encyclopedia \| title=Notes for planet 2MASSS J1119-1137 AB \| encyclopedia=The Extrasolar Planets Encyclopaedia \| url=http://exoplanet.eu/catalog/2mass_j11193254_ab/\| accessdate=2017-08-29\| archive-date=2017-08-29\| archive-url=https://web.archive.org/web/20170829203252/http://exoplanet.eu/catalog/2mass_j11193254_ab/\| dead-url=yes}}</ref> The least massive main sequence star with known planets is [[OGLE-2016-BLG-1195L]], at 0.078 {{Solar_mass}}. Baris 345: \|- \| Jari-jari bintang terkecil (katai cokelat) \| [[2M 0746+20 b]]<ref>{{cite web\|url=http://exoplanet.eu/catalog/2m_0746+20_b/\|title=The Extrasolar Planet Encyclopaedia — 2M 0746+20 b\|work=exoplanet.eu\|access-date=2020-08-25\|archive-date=2019-09-04\|archive-url=https://web.archive.org/web/20190904012129/http://exoplanet.eu/catalog/2m_0746+20_b/\|dead-url=yes}}</ref> \| [[2M 0746+20]] \| {{Solar radius\|0.089 (± 0.003)}}