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Explore the discovery, physical properties, and implications of planets beyond Pluto, including Easter Bunny, Santa, Xena, and more. Learn about the solar system's history and the fascinating findings from the Yale University, Indiana University, Caltech, and Gemini Observatory collaborations.
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Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center for Astronomy and Astrophysics Yale: Charles Baltay, Nancy Ellman, Will Emmet, Tom Hurteau, Rochelle Lauer, Suzanne Tourtellote Indiana University: Jim Musser, Brice Adams, Mark Gebhard Caltech: Michael E. Brown, Kristina Barkume, Henry Roe, A.H. Bouchez, R. Sari, M. van Dam, R. Campbell, J. Chin, S. Hartman, E. Johansson, R. Lafon, D. LeMignant, P. Stomski, D. Summers, P. Wizinowich Gemini Observatory : Chad Trujillo
2005 FY9 “Easter Bunny” 2003 EL61 “Santa” 2003 UB313 “Xena” Sedna Orcus Pluto (2200 km) Quaoar
Saturn Uranus Neptune
Saturn Uranus Neptune ecliptic plane
“Xena” 2005, 48” Sedna 2004, 48” Kuiper Belt Jewitt, Luu 1992, 86” Uranus Herschel, 1781, 6” Pluto Tombaugh, 1930, 13” Neptune Le Verrier, Galle 1846, 9”
AU Mic H-band imaging with Keck Adaptive Optics (0.04” seeing) M. Liu, Science 303, 2004
Where did the mass go ? (0.1 earth mass)
Keck Laser Guide Star Observations Easter Bunny Charon Rudolph Xena Gabrielle Santa
Gabrielle Xena Xena Gabrielle Xena-Gabrielle to Earth-moon Moon Earth
Santa (2003 EL61) a squashed planet
Satellite Discovered around 2003 EL61 (“Santa”) “Santa” “Rudolph”
v2/r = MG/r2 M = 4.21x1021 kg Rudolph’s orbit Radius: 49,000 km Period: 49 days