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22.2 Comets and Kuiper Belt Objects Roxanne Ryan.

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Presentation on theme: "22.2 Comets and Kuiper Belt Objects Roxanne Ryan."— Presentation transcript:

1 22.2 Comets and Kuiper Belt Objects Roxanne Ryan

2 Overview Comets – Dynamics of tail – Composition Oort Cloud Kuiper Belt

3 Model of a Comet 1950 -Fred Whipple proposed a model which explained most physical characteristics.  Nucleus  Tails  Coma  Halo

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5 Dynamics of Comet Tails Two distinct tails – Dust tail- created by radiation pressure on freed dust grains – Ion tail – interaction of ions in the comet with solar wind and suns magnetic field. Tails are always directed away from the sun.

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8 Composition of Comets Dust tails are white or yellowish due to light scattering off the particles.

9 Composition of Comets The ion tail is blue because it is rich in CO + ions which absorb and reradiate photons at wavelengths near 420 nm

10 Robotic Exploration of Comets In March 1986 Whipple’s “dirty-snowball” model was confirmed. July 4, 2004 Deep Impact sent a impactor into Comet Temple 1, allowing scientist to study interior. Comets density is roughly that of powder snow ~600 kg/m 3.

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13 Where do Comets come From? Two types of comets: – Short period: periods of less than 200 year and are found near the ecliptic – Long period: periods greater than 200 years and seemingly random orbits

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15 Kuiper Belt Located 30 – 50 AU from the sun First proposed around 1950 The first KBO was discovered in 1992 By 2006 over 900 had been discovered

16 Classes of Kuiper Belt Object’s Classical KBO’s – 30 – 50 AU from the sun – Orbital inclination of less than 30˚ – Semi-major axis 42-48 AU

17 Classes of Kuiper Belt Object’s Scattered KBO’s – Much higher eccentricity – Greater orbital inclination – Perihelion ~ 35 AU – Source of short period comets

18 Classes of Kuiper Belt Object’s Resonant KBO’s – KBO’s that are in orbital resonance with Neptune – Resonant Kbo’s with the same 3:2 resonance as Pluto and Charon are called Plutinos

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20 Oort Cloud In 1950 Jan Oort proposed that long period comets originate in a distant distribution of cometary nuclei. Has never been observed, but it’s existence is certain.

21 Oort Cloud 3,000-100,00 AU from the sun 10 12 -10 13 bodies Total mass ~ 100 solar masses

22 22.2 Comets and Kuiper Belt Objects Roxanne Ryan


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