A 16 Hour Transit of Kepler-167 e Observed by the Ground-based Unistellar Telescope Network
More than 5,000 exoplanets have been confirmed and among them almost 4,000 were discovered by the transit method. However, few transiting exoplanets have an orbital period greater than 100 days. Here we report a transit detection of Kepler-167 e, a "Jupiter analog" exoplanet orbiting a K4...
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| creator | Perrocheau, Amaury Esposito, Thomas M Dalba, Paul A Marchis, Franck Avsar, Arin M Carrera, Ero Douezy, Michel Fukui, Keiichi Ryan Gamurot Goto, Tateki Guillet, Bruno Kuossari, Petri Laugier, Jean-Marie Lewin, Pablo Loose, Margaret A Manganese, Laurent Mirwald, Benjamin Mountz, Hubert Mountz, Marti Ostrem, Cory Parker, Bruce Picard, Patrick Primm, Michael Randolph, Justus Runge, Jay Savonnet, Robert Sharon, Chelsea E Shih, Jenny Shimizu, Masao Silvis, George Simard, Georges Simpson, Alan Sivayogan, Thusheeta Meyer, Stein Trudel, Denis Tsuchiyama, Hiroaki Wagner, Kevin Will, Stefan |
| description | More than 5,000 exoplanets have been confirmed and among them almost 4,000 were discovered by the transit method. However, few transiting exoplanets have an orbital period greater than 100 days. Here we report a transit detection of Kepler-167 e, a "Jupiter analog" exoplanet orbiting a K4 star with a period of 1,071 days, using the Unistellar ground-based telescope network. From 2021 November 18 to 20, citizen astronomers located in nine different countries gathered 43 observations, covering the 16 hour long transit. Using a nested sampling approach to combine and fit the observations, we detected the mid-transit time to be UTC 2021 November 19 17:20:51 with a 1\(\sigma\) uncertainty of 9.8 minutes, making it the longest-period planet to ever have its transit detected from the ground. This is the fourth transit detection of Kepler-167 e, but the first made from the ground. This timing measurement refines the orbit and keeps the ephemeris up to date without requiring space telescopes. Observations like this demonstrate the capabilities of coordinated networks of small telescopes to identify and characterize planets with long orbital periods. |
| doi_str_mv | 10.48550/arxiv.2211.01532 |
| format | Article |
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However, few transiting exoplanets have an orbital period greater than 100 days. Here we report a transit detection of Kepler-167 e, a "Jupiter analog" exoplanet orbiting a K4 star with a period of 1,071 days, using the Unistellar ground-based telescope network. From 2021 November 18 to 20, citizen astronomers located in nine different countries gathered 43 observations, covering the 16 hour long transit. Using a nested sampling approach to combine and fit the observations, we detected the mid-transit time to be UTC 2021 November 19 17:20:51 with a 1\(\sigma\) uncertainty of 9.8 minutes, making it the longest-period planet to ever have its transit detected from the ground. This is the fourth transit detection of Kepler-167 e, but the first made from the ground. This timing measurement refines the orbit and keeps the ephemeris up to date without requiring space telescopes. 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However, few transiting exoplanets have an orbital period greater than 100 days. Here we report a transit detection of Kepler-167 e, a "Jupiter analog" exoplanet orbiting a K4 star with a period of 1,071 days, using the Unistellar ground-based telescope network. From 2021 November 18 to 20, citizen astronomers located in nine different countries gathered 43 observations, covering the 16 hour long transit. Using a nested sampling approach to combine and fit the observations, we detected the mid-transit time to be UTC 2021 November 19 17:20:51 with a 1\(\sigma\) uncertainty of 9.8 minutes, making it the longest-period planet to ever have its transit detected from the ground. This is the fourth transit detection of Kepler-167 e, but the first made from the ground. This timing measurement refines the orbit and keeps the ephemeris up to date without requiring space telescopes. Observations like this demonstrate the capabilities of coordinated networks of small telescopes to identify and characterize planets with long orbital periods.</description><subject>Celestial bodies</subject><subject>Extrasolar planets</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Planetary orbits</subject><subject>Space telescopes</subject><subject>Transit</subject><subject>Transit time</subject><subject>Universal time</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotkM1OwzAQhC0kJKrSB-CEJc4J9tr58bGqoEVU9FJOHCI7XouUkAQ7LfTtMS2nkT7NrmaGkBvOUllmGbvX_qc5pACcp4xnAi7IBITgSSkBrsgshB1jDPICskxMyNuc8pyu-r2nW6-70Iy0d_QZhxZ9wvOCIt2YgP6AlpojHd-RLn2_72xidIjstWvCiG2r4z22GOp-QPqC43fvP67JpdNtwNm_Tsn28WG7WCXrzfJpMV8nWmWQSKccVwqM5EagQ3AoZKENRFiX1tZ5JEqbvOQohLVaM5dLBQIscslATMnt-e2peTX45lP7Y_W3QHVaIDruzo7B9197DGO1i4W7mKmCQnDFirIoxS80el0b</recordid><startdate>20221104</startdate><enddate>20221104</enddate><creator>Perrocheau, Amaury</creator><creator>Esposito, Thomas M</creator><creator>Dalba, Paul A</creator><creator>Marchis, Franck</creator><creator>Avsar, Arin M</creator><creator>Carrera, Ero</creator><creator>Douezy, Michel</creator><creator>Fukui, Keiichi</creator><creator>Ryan Gamurot</creator><creator>Goto, Tateki</creator><creator>Guillet, Bruno</creator><creator>Kuossari, Petri</creator><creator>Laugier, Jean-Marie</creator><creator>Lewin, Pablo</creator><creator>Loose, Margaret A</creator><creator>Manganese, Laurent</creator><creator>Mirwald, Benjamin</creator><creator>Mountz, Hubert</creator><creator>Mountz, Marti</creator><creator>Ostrem, Cory</creator><creator>Parker, Bruce</creator><creator>Picard, Patrick</creator><creator>Primm, Michael</creator><creator>Randolph, Justus</creator><creator>Runge, Jay</creator><creator>Savonnet, Robert</creator><creator>Sharon, Chelsea E</creator><creator>Shih, Jenny</creator><creator>Shimizu, Masao</creator><creator>Silvis, George</creator><creator>Simard, Georges</creator><creator>Simpson, Alan</creator><creator>Sivayogan, Thusheeta</creator><creator>Meyer, Stein</creator><creator>Trudel, Denis</creator><creator>Tsuchiyama, Hiroaki</creator><creator>Wagner, Kevin</creator><creator>Will, Stefan</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20221104</creationdate><title>A 16 Hour Transit of Kepler-167 e Observed by the Ground-based Unistellar Telescope Network</title><author>Perrocheau, Amaury ; Esposito, Thomas M ; Dalba, Paul A ; Marchis, Franck ; Avsar, Arin M ; Carrera, Ero ; Douezy, Michel ; Fukui, Keiichi ; Ryan Gamurot ; Goto, Tateki ; Guillet, Bruno ; Kuossari, Petri ; Laugier, Jean-Marie ; Lewin, Pablo ; Loose, Margaret A ; Manganese, Laurent ; Mirwald, Benjamin ; Mountz, Hubert ; Mountz, Marti ; Ostrem, Cory ; Parker, Bruce ; Picard, Patrick ; Primm, Michael ; Randolph, Justus ; Runge, Jay ; Savonnet, Robert ; Sharon, Chelsea E ; Shih, Jenny ; Shimizu, Masao ; Silvis, George ; Simard, Georges ; Simpson, Alan ; Sivayogan, Thusheeta ; Meyer, Stein ; Trudel, Denis ; Tsuchiyama, Hiroaki ; Wagner, Kevin ; Will, Stefan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a952-4f9f1992b41b3efe2fe347ab2199c8ddc62fe9ab681e33ddaa0f649232de14023</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Celestial bodies</topic><topic>Extrasolar planets</topic><topic>Physics - 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However, few transiting exoplanets have an orbital period greater than 100 days. Here we report a transit detection of Kepler-167 e, a "Jupiter analog" exoplanet orbiting a K4 star with a period of 1,071 days, using the Unistellar ground-based telescope network. From 2021 November 18 to 20, citizen astronomers located in nine different countries gathered 43 observations, covering the 16 hour long transit. Using a nested sampling approach to combine and fit the observations, we detected the mid-transit time to be UTC 2021 November 19 17:20:51 with a 1\(\sigma\) uncertainty of 9.8 minutes, making it the longest-period planet to ever have its transit detected from the ground. This is the fourth transit detection of Kepler-167 e, but the first made from the ground. This timing measurement refines the orbit and keeps the ephemeris up to date without requiring space telescopes. Observations like this demonstrate the capabilities of coordinated networks of small telescopes to identify and characterize planets with long orbital periods.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2211.01532</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Celestial bodies Extrasolar planets Physics - Earth and Planetary Astrophysics Physics - Instrumentation and Methods for Astrophysics Planetary orbits Space telescopes Transit Transit time Universal time |
| title | A 16 Hour Transit of Kepler-167 e Observed by the Ground-based Unistellar Telescope Network |
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