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SEDNA: New Planet or Interstellar Menace? Steven Gibson The University of Calgary March 30, 2004.

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Presentation on theme: "SEDNA: New Planet or Interstellar Menace? Steven Gibson The University of Calgary March 30, 2004."— Presentation transcript:

1 SEDNA: New Planet or Interstellar Menace? Steven Gibson The University of Calgary March 30, 2004

2 Sedna, Innuit Goddess of the Sea

3 Discovery of 2003 VB12 Sedna (“Mickey”)

4

5 Why Study the Outer Solar System? ● Structure and formation history of solar system – coalescence, collisions, scattering, migration ● Composition of Solar Nebula material – Are objects primordial or evolved? ● Probe for gravitational evidence of large bodies – Planet X, Nemesis,... ? ● Near-interstellar environment beyond heliopause ● Because it's there! (What else do you need?)

6 Methods of Exploration ● Direct (difficult and still untried) – Voyager 1 (opted for Titan pass instead) – Pluto-Kuiper Express (cancelled) – New Horizons (launch 2006, flyby 2015) – TAU (1000 AU; 50 yr mission; concept only) ● Observation – Early discoveries came very slowly ● Uranus (1791), Neptune (1846), Pluto (1930) ● 2060 Chiron (1977), Charon (Pluto moon; 1978) – CCDs and computers have helped enormously ● 1992 QB1 until today : 831 TNOs!

7 Taxa of Sun-Orbiting Bodies, Part 1 ● (Major) Planets - large substellar objects orbiting the sun – terrestrial (Mercury, Venus, Earth, Mars) – jovian (Jupiter, Saturn, Uranus, Neptune) – ice dwarfs (Pluto et al.) - not planets by some definitions ● Planet definitions vary – historical (classical 9 with no future changes) – by mass or size (Pluto may be outclassed in future) – by shape (rounded by gravity - includes many moons) – relative (dominates mass in orbital domain)

8 Taxa of Sun-Orbiting Bodies, Part 2 ● Minor Planets (Planetoids) - smaller than planets ● Composition Categories – asteroids (rocks, no volatiles; 10m - 1000km) – comets (“primitive” composition; <~ a few km) ● long-P (>200yr) and intermed (20-200yr) from Oort Cloud ● Jupiter-family (<20yr) from Kuiper Belt ● Location Categories – Near-Earth (NEOs) - Atens, Apollos, Amors – Trojans (Mars, Jupiter, and Neptune to date) – Trans-Jovian - Centaurs (KB?), Damocloids (OC?) – Trans-Neptunian (TNOs)

9 Taxa of Sun-Orbiting Bodies, Part 3 ● Trans-Neptunian Objects – Kuiper Belt (KBOs) (30-50 AU) - nebular remnant? ● “Classical” KBOs, a.k.a. “Cubewanos” (after 1992 QB1) ● Resonance KBOs – “Plutinos” (“little Plutos” in 3:2 resonance with Neptune) – “Twotinos” (2:1) and others (1:1, 2:5, 4:5, 4:7, 3:5, 3:4) ● Scattered Disk Objects ● “Detatched” KBOs (Jewitt includes Sedna here) – Oort Cloud (OCOs) (50 AU - 50,000 AU) - scattered? ● “Classical” (Outer?) OCOs - aphelia ~ a few x 10,000 AU ● “Inner” OCOs may exist (Brown includes Sedna here)

10 TNO Motions over 100 Years (MPC) Comets High-e Objects Centaurs Plutinos Classical KBOs Scattered Disk Objects

11 TNO Orbits (from Jewett) Planets: Jupiter Neptune TNOs: Classical Plutinos Scattered

12 Sedna Orbit (from Brown)

13 Sedna Observations (the paper!) ● 48” Palomar Schmidt w/ 172 Mpix CCD array, drift-scanning 9.5 deg^2 area to 21 mag in R ● Detected Sedna 2003 Nov 14 w/ 1.5”/hr => r ~ 100 AU (apparent drift mostly Earth motion) ● Found prior detections 2003 Aug + 2002, 2001 data from NEAT survey; 1991 PDSS match poor ● From these data, refined orbital parameters derived: r=90.32+/-0.02 AU, a=480+/-40 AU, etc. ● This orbit is unprecedented. What is it?

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15 Sedna Data ● RA+DEC for March 30: ~ 3h14m32s +5d49.0m ● Current Distance from Sun: 90 AU (12.5 light hr) ● Perihelion / Aphelion: 76 / 850 AU (a ~ 480 AU) ● Inclination: 11.927 deg (Pluto = 17; Mercury = 7) ● Sednan year: 10,500 Earth years ● Sednan day: ~ 40 Earth days (due to moon?) ● Diameter: 1180-1800 km (51%-78% of Pluto) (upper limit from Spitzer & IRAM nondetection) ● Albedo, Color: > ~ 0.2?, very red (like Mars)

16 How Did It Get There? ● Orbit resembles Scattered KBO, but perihelion too big for Neptune to get it out there. ● Scattering by unseen planet near 70 AU – no detections of such an object to date ● Galactic tidal perturbation too soft ● Stellar encounter – very unlikely at short enough range, but who knows? ● Formation in a stellar cluster – denser than present stellar neighborhood; statistics more favorable; requires large new inner Oort pop ● All mechanisms more likely w/ richer population

17 Biggest Known TNOs ● Pluto - 2320 km (Charon - 1270 km) ● Sedna - 1200-1800 km (detatched KBO / Oort?) ● 2004 DW - 1600 km (plutino) ● Quaoar - 1200 km (cubewano) ● Varuna - 1060 km (cubewano) ● Ixion - 1055 km (plutino) ● (Ceres - 960; Triton - 2706; Ganymede - 5268)

18 Texas

19 What Else is Out There? ● Other Sednas (“Sedninos”?) - time will tell ● Oort Cloud Objects with much larger aphelia? ● “Planet X”? (Lowell's term) – no Neptunes unless d > 160 AU; Tombaugh looked (and Voyager 2 showed no gravitational evidence) ● Nemesis?? (Whitmore & Matese 1985) – hard to disprove object w/ d=20,000-90,000 AU and period ~ 32 Myr, but no real evidence, even in geological record; not useful for Sedna orbit either

20 (R mag ~ 20.5)


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