unexpected planets beyond pluto their discovery, physical properties, and implications for solar...

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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,

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Page 1: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

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

Page 2: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

Sedna

Quaoar

Orcus

Pluto (2200 km)

2003 EL61 “Santa”

2005 FY9 “Easter Bunny”

2003 UB313 “Xena”

Page 3: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

-120

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x (AU)

y (AU)

Sedna

Xena

Santa

Bunny

Neptune

Uranus

Saturn

Page 4: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

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x (AU)

z (AU)

Sedna Xena

Santa

Bunnyecliptic plane

Neptune

Uranus

Saturn

Page 5: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

QuickTime™ and aTIFF (Uncompressed) decompressor

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NeptuneLe Verrier, Galle

1846, 9”

UranusHerschel, 1781, 6”

PlutoTombaugh,

1930, 13”

“Xena”2005, 48”

Kuiper BeltJewitt, Luu 1992, 86”

Sedna2004, 48”

Page 6: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center
Page 7: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

Beta Pictoris

Page 8: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

M. Liu, Science 303, 2004

AU MicH-band imaging with Keck Adaptive Optics (0.04” seeing)

Page 9: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

(0.1 earth mass)

Where did the mass go ?

Page 10: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center
Page 11: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

QuickTime™ and aTIFF (Uncompressed) decompressor

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Clyde Tombaugh - 1938

Page 12: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

QuickTime™ and aTIFF (Uncompressed) decompressor

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The reflectance spectrum of 2003 UB313

Page 13: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

Type of Surface

Albedo Diameter Pluto Diameters

Fresh snow 90% 2330 km 1.0

Pluto 60% 2860 km 1.3

Charon

(Pluto’s moon)

38% 3550 km 1.5

Most Kuiper Belt Objects

15% 5700 km 2.4

Possible Sizes for “Xena”

Page 14: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

QuickTime™ and aTIFF (Uncompressed) decompressor

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Keck discovery of Xena’s moon, “Gabrielle”

Page 15: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

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Easter Bunny

Charon

Rudolph

Santa

Xena

Gabrielle

Keck Laser Guide Star Observations

Page 16: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

Xena-Gabrielle to Earth-moon

Earth

Moon

Xena Gabrielle

Xena Gabrielle

Page 17: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

Santa (2003 EL61) a squashed planet

Page 18: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

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Satellite Discovered around 2003 EL61 (“Santa”)

“Santa”

“Rudolph”

Page 19: Unexpected planets beyond Pluto their discovery, physical properties, and implications for solar system history David Rabinowitz Yale University, Center

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Radius: 49,000 kmPeriod: 49 days

Rudolph’s orbit

v2/r = MG/r2

M = 4.21x1021 kg