Evidence for Liquid Water on Comets Rob Sheldon, Richard Hoover SPIE SanDiego July 31, 2005.

Slides:



Advertisements
Similar presentations
15 Comets Fire and Ice. 15 Goals What are comets? How are they different from asteroids? What are meteor showers? How are they different from typical.
Advertisements

Comets The last type of minor solar system object is the one which has been most noticed since deep antiquity… Comet Hale-Bopp in spring of 1997.
Goal: To understand what comets are and to explore the Oort cloud.
Unt4: asteroid part 2. Comets Comet Ikeya-Seki in the dawn sky in 1965.
Solar System.
The Edge of the Solar System The Oort Cloud. What is the Oort Cloud? Spherical area between 5,000 and 100,000 AU from the sun (Kuiper belt ends at 55.
Clicker Questions Chapter 6 The Terrestrial Planets Copyright © 2010 Pearson Education, Inc.
Structure & Formation of the Solar System
COMETS, ASTEROIDS, AND METEORS
Comets May 7, 2004 Icy bodies left over from formation of Solar System Possibly brought water & organic material to early Earth.
Implications of cometary water: deep impact, stardust, and Hyabusa Rob Sheldon, Richard Hoover SPIE SanDiego August 15, 2006.
The Universe. The Milky Way Galaxy, one of billions of other galaxies in the universe, contains about 400 billion stars and countless other objects. Why.
Jupiter Astronomy 311 Professor Lee Carkner Lecture 17.
Comets Astronomy 311 Professor Lee Carkner Lecture 22.
Comets Astronomy 311 Professor Lee Carkner Lecture 22.
Comet cartoon from 1857: Will a comet impact destroy Earth?
The Solar System 1 star 9 8 planets 63 (major) moons
How our Solar System (and Moon) came to be…. Learning Objectives Be able to explain – How our solar system and moon came to be.
Our Solar System Chapter 28.
Copyright © 2010 Pearson Education, Inc. Our Solar System.
STRAND #1 – EARLY ASTRONOMY 1. Name the scientist that said the sun was the center of the solar system (and not the Earth) AND name the scientist that.
We continue to Learn a lot about the Solar System by using Space Exploration CHAPTER 11.
9.2 Comets Our Goals for Learning How do comets get their tails? Where do comets come from?
Comparative Planetology I: Our Solar System Chapter Seven.
Earth and Other Planets Chapter 16 Great Idea: Earth, one of the planets that orbit the Sun, formed 4.5 billion years ago from a great cloud of dust.
Solar System. MILKY WAY 200 billion stars Diameter LY Height at center LY Solar System is LY from center.
The Solar System. Overview of the Solar System Basics Source: Nine Planets - A Multimedia Tour of the Solar System * By Bill Arnett.
The Moon Chapter 6. Characteristics of the Moon The ___________ neighbor in space The ___________ neighbor in space No atmosphere No atmosphere Marked.
Big Bang theory Parts of our solar system Planet characteristics Galaxies Constellations Nebulas.
Our Solar system YouTube - The Known Universe by AMNH.
Space Asteroids Raynaldo 6B.
We continue to Learn a lot about the Solar System by using Space Exploration CHAPTER 11.
Comparative Planetology I: Our Solar System. Guiding Questions 1.Are all the other planets similar to Earth, or are they very different? 2.Do other planets.
Comets, Asteroids, Meteoroid and Meteorites Chapter 21 Section 5 Pages
1. Amor asteroid -an asteroid whose orbit crosses the orbit of Mars.
03 Oct 2000ASTR103, GMU, Dr. Correll1 Ch 8--Asteroids, Meteors, Comets.
Small Bodies in the Solar System
The Earth and Other Planets
A Family of Planets Chapter 9
The Sun & The Solar System. Structure of the Sun The Sun has layers which can be compared to the Earth’s core, mantle, crust, and atmosphere All of these.
Study Guide Answers. 1. What is the difference between geocentric and heliocentric? Geocentric: Earth is the center of the universe Heliocentric: Sun.
Small Bodies in the Solar System ESS ( ). Small Planetary Bodies  In addition to planets & moons, the solar system contains many other types of.
The Solar System. Solar System the sun and all things orbiting around it, including the eight major planets, their satellites, and all the smaller pieces.
The Moon Chapter 6. Characteristics of the Moon The ___________ neighbor in space The ___________ neighbor in space No atmosphere No atmosphere Marked.
EARTH IN SPACE. DAY AND NIGHT The Earth completes one rotation on its axis every 24 hours. The rotation of the Earth on its axis is responsible for day.
Meteor seen Over Des Moines, Iowa. The Loenid Meteor Shower.
The Solar System Inner and Outer Planets
Chapter 4 The Solar System. Comet Tempel Chapter overview Solar system inhabitants Solar system formation Extrasolar planets.
Chapter 7: Comets composition, origin, fate tail formation; the physics of sublimation.
Dokumentname > Dokumentname > B Recent Results of Comet Activity Modeling as input for RPC Plasma Simulations Recent Results of Comet.
Comets. The Kuiper Belt Many Plutoids and smaller icy planetismals or “cometary bodies” orbit close to the same plane as the planets forming a “belt”
Meteoroids, Meteors, Meteorites, Asteroids & Comets What ’ s The Difference? ? ? ? ? ? ? ?
Green House Effect and Global Warming. Do you believe that the planet is warming? 1.Yes 2.No.
Know about Pluto Know about the Asteroids Know about Comets Comprehend the Oort Cloud and Kuiper Belt Asteroids and Kuiper Belt Objects.
What they are Where the are They and Us.  Comet – A body that produces a coma of gas and dust; a small, icy body that orbits the Sun  Made of ice and.
Know about Pluto Know about the Asteroids Know about Comets Comprehend the Oort Cloud and Kuiper Belt Asteroids and Kuiper Belt Objects.
Ch. 20 and 21.  Our solar system has been here for awhile  5 billion years!  It formed from a solar nebula  Clouds of dust in space that combined.
The Solar System By Gina Wike. Solar System Early Greeks thought that everything centered around the Earth. Copernicus thought differently. He said the.
1 Earth and Other Planets 3 November 2015 Chapter 16 Great Idea: Earth, one of the planets that orbit the Sun, formed 4.5 billion years ago from a great.
Study of the universe (Earth as a planet and beyond)
Unit 5: The Solar System Mr. Ross Brown Brooklyn School for Law and Technology.
Can Comets Contain Water? A “Wet” Comet Theory Rob Sheldon NSSTC October 29, 2004.
On the Larger Picture in Cometary Science
© 2017 Pearson Education, Inc.
Small Bodies in the Solar System
Rosetta mission discovers the wet-comet model Rob Sheldon Aug 11, 2015
The Inner Planets.
The Study of the Universe
Ch. 28 – minor bodies of the solar system
Our Solar System.
Presentation transcript:

Evidence for Liquid Water on Comets Rob Sheldon, Richard Hoover SPIE SanDiego July 31, 2005

Harold’s Bane 1066 AD Her forðferde Eaduuard king. Harold eorl feng to ðam rice heold hit.xl. wucena. ænne dæg. her com Willelm gewann ængla land. her on ðison geare barn Cristes cyrice. [her atiwede cometa.xiii. kalendæ MAI. ]

Fred Whipple’s 1950 “Dirty Snowball” Model But equilibrium temperature of bodies in the inner solar system is > 273 K ! To keep the comet from melting, we apply some refrigeration principles: - white color (high albedo) - sublimation cooling - low spin rate - dust insulation (porous) But this condition is unstable!

Temperature Regulation If heat transport overwhelms refrigeration the pressure goes up, or should“black goo” / melt liquid plug reduce the permeability, then the lid goes on the pressure cooker. At high enough pressure, meltwater forms. This clogs more crust, permitting higher pressures, less sublimation cooling, higher heat transport in (waterlogged attic insulation)= more melting. E.g., Positive feedback (Yelle 2004) And the Rayleigh-Taylor instability can trigger a large increase in heat transport.

Rayleigh-Taylor Instability Contours Slow Rotator,T=10.4hrFast Rotator, T=5h T=5hr w/cosine insolation (4/3  DG –  2 )  = gravity at equator (x-axis) Sun at left 3min Therefore mean temperature has a phase transition at critical T c. This initiates a positive feedback sequence. Below T c heat is pumped out on night side, above T c heat pumped in. Stretched 10X y-axis scale below line 3min  =1hr stable

Spin contribution to feedback Melted dirty snow will segregate, dust drops “down” to to the equatorial surface. This thickens the crust, reduces the gas flow, and permits higher pressure and hence more liquid. Another feedback. Dust has higher density than water/ice, so migration to equator will slow the rotation rate of the comet. When it drops below 1/T c, it immediately refreezes. Thus RT drives a comet to T c. Liquid acts as a nutation damper, eliminating precession, giving higher spin in 1-axis, which promotes RT. A positive feedback. Differentiation lowers the density of the interior, which enhances RT (lowers T c.)

Concrete Crust Dust at the surface reduces the albedo, both by color and roughness. This increases the temperature and heat flow into the comet. Crust “dries out” in original shape. Meter thick rigid crust develops which can support observed vertical landscape. Crust at equator may be cooler (due to R-T) than crust at the poles (no RT). This makes the RT “spread out” across the surface. As water “leaks out” vapor pockets form in equatorial belt (geysers). Collapse/explosion of vapor pockets lead to cratering, and eventually to prolate erosion of comet.

Activity & Fragmentation Release of vapor and/or liquid from vapor pockets = geyser. See Yelle (Icarus04) Partial pressures can support liquid water. When sufficient equatorial erosion has made comet prolate, liquid water facilitates a swap of rotation axes. Old polar regions had been under compression, now find themselves under tension = likely breakup scenario. Weakest prolate crust is at the poles, where Borrelly had a stable geyser. Accident? Or global melting? Breakup separation speed depends on aspect ratio and/or vapor pressure, both functions of light intensity.

A Comet’s Life Ice Liquid Vapor Spin Axis Spin Flip a) b) c) d) e) f) g) Cement

Issues before s/c era 1.Birth: 1.Density of comets 2.Albedo-Area 3.Kuiper Belt vs Oort 4.Aphelion vs Perihelion 2.Life: 1.Spin rate 2.Shape aspect ratio 3.Brightness vs radial distance 4.Active area, jets 5.New vs. Old comets 6.Outbursts 7.Tail Shedding 3.Death: 1.Earth crossing asteroids 2.Fireballs vs chondrites 3.Tidal Force Breakup

Issues after s/c visits to P/Halley (& P/Borrelly & P/Wild-2) 1.Albedo: darker than soot! 2.Shape: very prolate! 3.Dust distribution across limb, size. 4.Small active area Jets: dayside, geyser-like 5.Temperature: K 6.Pinnacles, cliffs, craters, patterned ground 7.Deep Impact raised only dust

1.1 Comet Density Brownlee particles collected in the stratosphere thought to be from comets. Comets are thought to have a density 1/10 that of water?

1.2 Albedo Before the spacecraft era, astronomers only knew the product of albedo & area. Comets were thought to have albedo in the.3-.7 range, like most asteroids. This made comets seem much smaller than was actually correct. They turned out to be blacker than soot! So much bigger too. And hotter.

1.4 Aphelion vs Perihelion Why is there a gap both for q 3? And nothing near hyberbolic? Comets, 1981

1.4 Apogees in Theory & Life Comets, 1981 Theory Weighted Observations

2.1 Spin by jets Why do comets spin slower than asteroids? Why do comets all spin much slower than breakup? than RT? Comets, 1981

2.2 Spin from Stellar obs. CCD camera observations at large distance “stellar” lightcurves for prolate objects ApJ 1988

2.3 Activity The dust follows a 1/r 4 law, but gas doesn’t? Post<>Pre-perihelion? Comets, 1981

2.4 Active area & jets Why is post-perihelion different from pre (both in absolute and r dependence)? Why was Kohoutek so disappointing? (Methane ice, or CO ice, etc. Some phase transition occurred, but no one is sure what. Skylab, H-corona, 1973

2.5 New vs Old Comets New are dustier, but old are supposed to lose their volatiles! If gas/dust ratios are fixed, why aren’t they the same? Hale-Bopp, 1997

2.6 Outbursts? What would cause 8 order of magnitude changes in brightness P/Schwassmann-Wachmann? Collisions? But then how does the comet survive? Halley had a 300-fold increase in brightness in 1991, while at 14.3AU. Collisions don’t seem to explain it, nor were there any convenient solar flares. Tempel-1 had 2 outbursts during the week before collision.

2.7 Tail Shedding Shouldn’t they occur at every sector crossing? Why so infrequent then? Comets, 1981

3.2 Tensile Strength Do fireballs determine the tensile strength of comets? Comets, 1981

3.3 Tidal Breakup? Comets, 1981

4.1 Black Prolate P/Halley Blacker than the coma behind it! Jets! Prolate Not outgassing 400K Little dust Courtesy Giotto

4.2 Prolate Shape (P/Borrelly) Courtesy Deep Space 1

Prolate P/Wild-2 Courtesy Stardust Stereo pairs showing top panel with large projection out of the frame; middle panel with deep canyon; bottom panel with high pinnacles in the “crater” at the bottom. Courtesy Stardust

4.4 Geysers Giotto DS-1 Stardust Deep Impact

4.6 Pinnacles Stardust

41 hours Outbursts 4.7 Deep Impact

50ms frames What, No Water?

Spin Axis Estimate 1.7 deg motion of crater 3.0 deg motion of “rim” +

Insolation vs Axis Putative pole Impact site Pole remains in sunlight, as does impact site + x

Evacuation of 9P/Tempel-1 From the wet comet=critical period calculation, T=41hr, D=20kg/m 3. That’s really fluffy snow! And completely inconsistent with cratering data. But that assumes uniform density. If the comet has vapor pockets, then RT instability still operates. g If pristine comet has D=200 kg/m 3, we estimate 90% of the interior is vapor, 10% pristine.

Conclusions Comets are in an unstable thermal equilibrium as they enter the inner solar system. We believe many factors contribute to their spontaneous phase change from sublimation cooled to “wet” comets. Wet comet theory explains many unsolved puzzles of cometary dynamics. Deep Impact results seem to show no water, and we argue why this result is still consistent with the wet comet theory. Therefore the major objection to life on comets, the absence of water, appears less defensible.

Planetary Protection “Planetary Protection Matters” J. Rummel, NASA HQ, and L. Billings, SETI (Cospar 8/04) Planetary protection is the term given to the policies and practices that protect other solar system bodies…from terrestrial life, and that protect the Earth from life that may be brought back…. The cost of meeting stringent Category V requirements on a Mars surface sample return mission is estimated at about 5-10% of the entire mission budget. Genesis category I? Stardust category II? SpaceNews 9/20/04 “Genesis Mishap Renews Debate About Mars Sample Return”. “Genesis did not have a planetary protection requirement for containment.” Rummel. “Everyone agrees that we must be as careful as possible with the Mars sample,..The question is whether we want to spend billions are tens of billions of dollars to make the risk even more infinitesimal.” Mendell

References: Comets, ed. L. Wilkening, 1981 Physics and Chemistry of Comets, ed. W.Huebner ApJ 1988 Jewett and Meech Icarus issue on Borelly R. Hoover et al. SPIE proceedings 5555

Birth Oort cloud. Volatile rich. Coalescence from primordial nebula. Carbon rich. (Why?!) Loose, weakly bound gravitational objects 1-100km in size. Possible 26 Al heating may have caused partial melting. Cosmic ray transformed outer cm-thick crust. Black goo / burnt toast. Tensile strength of interior estimated 1-10 kPa. (Tidal stress breakup, fireballs) In comparison plaster of paris has a tensile strength 0.6 MPa, ice around 1.6 MPa. Comets are 200x weaker than solid ice!

Life Orbit is deflected from circular to elliptical As comet approaches the “snow line” at 5AU it begins to vaporize and form a tail. Several tons/s loss of mass. The tail grows as it nears the sun, produces dust & plasma tails, and dynamic effects due to jets and outbursts. May break up at any point in orbit. On receding from the sun, the tails shrink and the comet becomes “stellar” beyond 5AU. May get trapped or deflected by Jupiter.

Death Volatiles are lost and comet looks asteroidal Crust of non-volatile material gets too thick mimicking the loss of volatiles. Comet fragments (tidal forces, spin rate?). Comet interacts with Jupiter and is either ejected, or trapped. Comet collides with another body, fireballs (spectacular Shoemaker-Levy-9 collision) Comet leaves on a hyperbolic orbit

Summary Water explains why fireballs break up early-I.e. Columbia. Crustal differentiation with water explains albedo. W. explains rapid diffusion of aphelion W. explains slow spinrate, prolate shape, and lightcurves. W. explains asymmetry around perihelion, gas production with wrong radial dependence, and existence of jets. W. explains why new comets (dry, subliming) are brighter than old (wet, crusty). W. explains non-tidal fragmentation. W. may explain rapid brightening by collision (splashing=large surface area). W. may explain reduced tail-shedding. And the $64,000 question: What about Life?