| dbo:abstract |
Kepler-1708b (previously known as KIC 7906827.01) is a Jupiter-sized exoplanet orbiting the Sun-like star Kepler-1708, located in the constellation of Cygnus approximately 5,600 light years away from Earth. It was first detected in 2011 by NASA's Kepler mission using the transit method, but was not identified as a candidate planet until 2019. In 2021, a candidate Neptune-sized exomoon in orbit around Kepler-1708b was found by astronomer and colleagues in an analysis using Kepler transit data. (en) ケプラー1708b（以前はKIC 7906827.01として知られていた）とは、地球からはくちょう座の方向に約5,600光年離れた場所に存在する太陽のような恒星ケプラー1708の周囲を公転している木星サイズの太陽系外惑星である。トランジット法を使用してNASAのケプラー宇宙望遠鏡ミッションによって2011年に最初に検出されたが、2019年まで惑星候補として識別されていなかった。2022年にケプラー1708bの存在が確認され、さらにケプラー1708bの周囲を公転している海王星サイズの太陽系外衛星の候補が、ケプラーのトランジット観測データを使用した分析で天文学者のDavid Kippingとその同僚によって発見された。 (ja) Kepler-1708 b è un pianeta extrasolare in orbita attorno alla stella Kepler-1708, una stella simile al Sole di magnitudine 15,9 della costellazione del Cigno, distante 5580 anni luce dal sistema solare. Si tratta di un gigante gassoso simile a Giove situato nella zona abitabile della propria stella, la cui peculiarità consiste nell'avere un candidato satellite naturale, Kepler-1708 b I, il secondo scoperto dopo Kepler-1625 b I. (it) |
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Transit |
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KIC 7906827.01 (en) |
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http://exoplanet.eu/catalog/kepler-1708_b/ https://exoplanetarchive.ipac.caltech.edu/cgi-bin/ICETimeSeriesViewer/nph-ICEtimeseriesviewer%3Fidtype=source&inventory_mode=id_single&id=7906827&dataset=KeplerDV https://news.columbia.edu/news/astronomers-find-evidence-second-exomoon |
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Kepler-1708b (previously known as KIC 7906827.01) is a Jupiter-sized exoplanet orbiting the Sun-like star Kepler-1708, located in the constellation of Cygnus approximately 5,600 light years away from Earth. It was first detected in 2011 by NASA's Kepler mission using the transit method, but was not identified as a candidate planet until 2019. In 2021, a candidate Neptune-sized exomoon in orbit around Kepler-1708b was found by astronomer and colleagues in an analysis using Kepler transit data. (en) ケプラー1708b（以前はKIC 7906827.01として知られていた）とは、地球からはくちょう座の方向に約5,600光年離れた場所に存在する太陽のような恒星ケプラー1708の周囲を公転している木星サイズの太陽系外惑星である。トランジット法を使用してNASAのケプラー宇宙望遠鏡ミッションによって2011年に最初に検出されたが、2019年まで惑星候補として識別されていなかった。2022年にケプラー1708bの存在が確認され、さらにケプラー1708bの周囲を公転している海王星サイズの太陽系外衛星の候補が、ケプラーのトランジット観測データを使用した分析で天文学者のDavid Kippingとその同僚によって発見された。 (ja) Kepler-1708 b è un pianeta extrasolare in orbita attorno alla stella Kepler-1708, una stella simile al Sole di magnitudine 15,9 della costellazione del Cigno, distante 5580 anni luce dal sistema solare. Si tratta di un gigante gassoso simile a Giove situato nella zona abitabile della propria stella, la cui peculiarità consiste nell'avere un candidato satellite naturale, Kepler-1708 b I, il secondo scoperto dopo Kepler-1625 b I. (it) |
| rdfs:label |
Kepler-1708 b (it) Kepler-1708b (en) ケプラー1708b (ja) |
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