Beyond Point Masses. II. Non-Keplerian Shape Effects are Detectable in Several TNO Binaries

About 40 transneptunian binaries (TNBs) have fully determined orbits with about 10 others being solved except for breaking the mirror ambiguity. Despite decades of study almost all TNBs have only ever been analyzed with a model that assumes perfect Keplerian motion (e.g., two point masses). In reali...

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Veröffentlicht in:arXiv.org 2024-03
Hauptverfasser: Proudfoot, Benjamin C N, Ragozzine, Darin A, Thatcher, Meagan L, Grundy, Will, Spencer, Dallin J, Alailima, Tahina M, Sawyer, Allen, Bowden, Penelope C, Byrd, Susanne, Camacho, Conner D, Campbell, Gibson H, Carlisle, Edison P, Christensen, Jacob A, Christensen, Noah K, Clement, Kaelyn, Derieg, Benjamin J, Dille, Mara K, Dorrett, Cristian, Ellefson, Abigail L, Fleming, Taylor S, Freeman, N J, Gibson, Ethan J, Giforos, William G, Guerrette, Jacob A, Haddock, Olivia, S Ashton Hammond, Hampson, Zachary A, Hancock, Joshua D, Harmer, Madeline S, Henderson, Joseph R, Jensen, Chandler R, Jensen, David, Jensen, Ryleigh E, Jones, Joshua S, Kubal, Cameron C, Lunt, Jacob N, Martins, Stephanie, McKenna Matheson, Maxwell, Dahlia, Morrell, Timothy D, Myckowiak, McKenna M, Nelsen, Maia A, Neu, Spencer T, Nuccitelli, Giovanna G, Reardon, Kayson M, Reid, Austin S, Richards, Kenneth G, Robertson, Megan R W, Rydalch, Tanner D, Scoresby, Conner B, Scott, Ryan L, Shakespear, Zacory D, Silveira, Elliot A, Steed, Grace C, Suggs, Christiana Z, Suggs, Garrett D, Tobias, Derek M, Toole, Matthew L, Townsend, McKayla L, Vickers, Kade L, Wagner, Collin R, Wright, Madeline S, Zappala, Emma M A
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