12/2/04ESS 298 Fall 20041 The Two Faces of Iapetus The Brightness Contrast Explored Colleen Milbury The Brightness Contrast Explored Colleen Milbury.

Slides:



Advertisements
Similar presentations
Our Solar System A Write On Activity.
Advertisements

Asteroids On-line Lesson. What are they? Asteroids are solid pieces of rock that have been left around the Solar System from the time when the planets.
Water Ice on Titan’s Surface Spectra were obtained of the leading and trailing hemispheres of Titan with SpeX at 0.8–5.1 microns with the IRTF and at 4.6–5.2.
Planets: Wandering Worlds Chapter 4. Planets The planets are called wondering worlds… This is because they are in motion.
4.5 The Outer Planets What Do the Outer Planets Have in Common?
The Moons of Saturn: Tethys, Rhea, & Iapetus
Jupiter and Saturn’s Satellites of Fire and Ice Chapter Fifteen.
The Super Solar System The Super Solar System By: Laura Bart.
Solar System Fun Facts and Vocabulary ©2012HappyEdugator.
The Moons of Our Solar System. How many moons are in our solar system? 1? 9? 61? 159? 159 and counting!
Pan and Atlas Pan is very small. It is the closest moon to Saturn and orbits within the Enckle Division, a gap within Saturn's A ring. Pan is an irregular.
Jovian Moons. Moons of Solar System Moons can sometimes be as large as planets –Ganymede & Titan are larger than Mercury –All 7 of these moons are larger.
 Satellites – natural or artificial bodies that revolve around larger bodies such as planets.
Our Solar System BIRTH OF SOLAR SYSTEM ndGc ndGc A BRIEF GLANCE
Our Solar System Mrs. Lacks 6th Grade.
Presentation by: Heather DeRoy
Saturn By: Zack and Kacey.
Unit 2 Lesson 1 What Objects Are Part of the Solar System?
1. Helium rain lower temperatures of Saturn's interior allow helium to come out of solution with hydrogen and form droplets, these droplets fall toward.
The Outer Planets Jupiter, Saturn, Uranus, Neptune Click here to move to the next slide!
Our Solar System. The Sun Our Sun is a medium-sized yellow star in the middle of its life cycle. Its the center of our Solar System and holds objects.
Judith Trillo Alyssa Waugh Chaz Isaacks Saturn improved and changed a lot when the advent of space light that we really began to gain a greater understanding.
SATURN By Alex Clarke 7.4. Introduction For my science project I have chosen to do Saturn, a large planet in our solar system. This presentation will.
Our Solar System Intro Video Intro Video. Your Parents’ Solar System.
Our solar system Chapter 2 By Mrs. Shaw.
Other Objects in the Solar System (13.15). Planetary Moons Large natural objects that revolve around planets are called satellites or moons. Moons range.
PHYSICAL CHARACTERIZATION OF ASTEROIDS NEON Group 5: Koraljka Mužić Nikola Vitas Grzegorz Nowak Mario Mars Simone Marchi (tutor) 5 th NEON SCHOOL, OHP,
Our Solar System. Your Parents’ Solar System 21 st Century Solar System.
Our Solar System A Write On Activity. Our Solar System Our solar system is made up of: Sun Nine planets Their moons Asteroids Comets.
Crash Landing Activity First, get into teams of three to five (I will assign) and create a list of items you would need to bring to survive an extended.
Big Bang theory Parts of our solar system Planet characteristics Galaxies Constellations Nebulas.
Other Solar System Bodies Moons Asteroids Comets Meteors and Meteorites.
A Journey to Our Planetary Neighbors
Our Solar System A Write On Activity EARTH AND SPACE SCIENCE Tennessee Standard: Content Standard: 7.0 Earth and Its Place in the Universe The student.
Our Solar System.
5B Satellites of the outer solar system The almost-planets.
Comets, Asteroids, and Meteoroids
Our Solar System By Shaikh Muhammad Mustafa 8b5 and his slaves Omar, Vishan and Hamdan.
The Outer Planets The outer planets are: Jupiter Saturn Uranus Neptune.
NOTES: Saturn 9.5 D earth Same atmosphere as Jupiter, but cloud obscures belts and zones. Tilt 26.7 degrees, Day = 10.5 hours, very oblate 1/20th magnetic.
 4 planets: Mercury, Venus, Earth, & Mars.  Solid surfaces  Similar in size  All quite close to the sun and closer to each other compared to the Outer.
Saturn’s Moon System Most extensive, complex moon system in the solar system. Over 40 known moons.
Earth and Space Our Solar System Our solar system is made up of: Sun Eight planets Their moons Asteroids Comets Meteoroids.
1 Amazing Saturn Saturn from the ground. 2 Saturn Information Overload The Cassini Mission started orbiting Saturn in 2004.
The Planet Saturn.
Uranus’ Moons - 5 larger moons 10 smaller moons The smaller moons were discovered by Voyager 2.
Taking the Temperature of Phoebe and Iapetus with Cassini’s Composite Infrared Spectrometer (CIRS) John Spencer Southwest Research Institute Boulder, CO.
Jupitar. Jupitar is the solar systems largest planet. It’s mainly hydrogen and helium atmosphere resembles that of our Sun. Some scientists ever refer.
Don’t flush it all away. Get your missing, late or work you want redone turned in. Only 15 days remaining. Due 12/20/13.
Moons of Jupiter and Saturn
The Outer Planets - Jupiter Jupiter, the largest of the planets, is 2.5 times more massive than all the other planets combined It is covered by clouds.
The Outer Planets Section Standard e. Students know the appearance, general composition, relative position and size, an motion of objects.
© Sierra College Astronomy Department The Jovian Moons and Rings.
Astronomy 1010 Planetary Astronomy Fall_2015 Day-37.
Our Solar System Solar System Day 2. Objectives TODAY I WILL BE ABLE TO: – Compare and contrast _____________ planets to __________________ planets.
Our Solar System Our solar system is made up of: Sun Eight planets Their moons Asteroids Comets.
Gas Giants Jupiter, Saturn, Uranus, Neptune. The Asteroid Belt lies between Mars and Jupiter, separating the inner and outer planets.
Earth Science An overview of the Solar System. The Sun The sun is the biggest, brightest, and hottest object in the solar system. The sun is the biggest,
P LANETS AND MINOR MEMBERS OF THE S OLAR S YSTEM.
Unit 5 Lesson 2. Vocabulary  Solar System: A star and all the planets and other objects that revolve around it.  Planet: A body that revolves around.
The Moons of Other Planets Chapter 16-4 Part 2 Part 2 The moons of other planets range in size from very small to as large as terrestrial planets. Venus.
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.
The Solar System. What’s in Our Solar System? Our Solar System consists of a central star (the Sun), the eight planets orbiting the sun, moons, asteroids,
Our Solar System A Write On Activity.
Saturn’s Moon System Most extensive, complex moon system in the solar system. Over 60 known moons.
Uranus’ Moons - 5 larger moons 10 smaller moons The smaller moons were discovered by Voyager 2.
Super Saturn Super Saturn By Arabella Roshan Mr Speedie
The Moons Of Saturn.
Jupiter Astronomy 311 Professor Lee Carkner Lecture 17.
Presentation transcript:

12/2/04ESS 298 Fall The Two Faces of Iapetus The Brightness Contrast Explored Colleen Milbury The Brightness Contrast Explored Colleen Milbury

12/2/04ESS 298 Fall Overview Discovery of Iapetus Pictures Observations Endogenic Models Exogenic Models Summary/Conclusions

12/2/04ESS 298 Fall Discovery of Iapetus In Greek mythology Iapetus was a Titan, the son of Uranus, the father of Prometheus and Atlas and an ancestor of the human race. Discovered by Giovanni Cassini in 1671 He said the following about Iapetus in 1673: “One part of [Iapetus’] surface is not so capable of reflecting the light to us the light of the Sun which maketh it visible, as the other part is…” Cassini was able to observe Iapetus during western elongation, he could not detect it during eastern elongation.

12/2/04ESS 298 Fall Pictures of Iapetus

12/2/04ESS 298 Fall 20045

12/2/04ESS 298 Fall Table of Parameters

12/2/04ESS 298 Fall Nice Diagram of Saturn System

12/2/04ESS 298 Fall Observations Order of magnitude contrast Geometric albedo is Centered about apex of motion Low albedo inconsistent with silicates

12/2/04ESS 298 Fall More Observations Low albedo (dark) material is Red (albedo increases at longer ’s) -Does not match C-type (carbonaceous) asteroid [similar to Phoebe], only redder D-type asteroids Dark floored craters imply dark material is younger Absence of bright craters imply: -deposit is thick (>10 km), or -bright material darkened/buried with 100 million year period

12/2/04ESS 298 Fall Endogenic Model-Smith et al Site symmetry, Phoebe exogenic example Favor endogenic model Dark floored craters as strong endogenic evidence Site examples of other hemispheric alignments in solar system (Mars, Moon, and Io)

12/2/04ESS 298 Fall Exogenic Model-Owen et al Use mixing models of pure substances Satisfied 1,3, and 4 with amphorus carbon and water-ice Turned to organic compounds to satisfy 2 and stay consistent with 4 Conclude that component comes from Titan’s nitrogen rich atmosphere Titan impact that could have sprayed particles onto Hyperion and Iapetus and even produced Hyperion

12/2/04ESS 298 Fall Exogenic Model-Buratti et al Three nights of measurement from Hale telescope on Palomar Mountain Three D-type asteroids and icy Saturn satellites Range is µm

12/2/04ESS 298 Fall Exogenic Model-Buratti et al Don’t combine spectra of pure substance Use spectra of typical icy bodies, D-type asteroids F-normalized Fluxes Icy=Icy Bodies Iap=Iapetus D=D-type asteroids A-coefficient (percent of material)

12/2/04ESS 298 Fall p = geometric albedo Exogenic Model-Buratti et al Apply to albedo Conclude that dark side Iapetus created by collision of proto- Hyperion and D- type asteroid

12/2/04ESS 298 Fall Exogenic Model-Buratti et al Hyperion - irregular shape and chaotic rotation imply it is remnant of larger body Also note discovery of 5 new satellites that appear to be created from this impact Most particles are accreted by Titan

12/2/04ESS 298 Fall Summary and Conclusions Iapetus is somewhat of a rarity in the solar system Probably not of endogenic origin Probably not from Phoebe material Strong evidence of some type of exogenic origin Buratti et al. most likely

12/2/04ESS 298 Fall References Buratti et al. (2001). High Resolution µm Spectra of Iapetus, Hyperion, Rhea, Dione, and D-Type Asteroids. Icarus, 155, Morrison et al. (1974). The Two Faces of Iapetus. Icarus, 24, Owen et al. (2000). Decoding the Domino. Icarus, 149, Smith et al. (1982). A New Look at the Saturn System. Science, Vol. 215, No. 4532, Satellites. Edited by Joseph A. Burns, Mildred Shapley Matthews Tucson : University of Arizona Press, c1986. Saturn. Edited by Tom Gehrels, Mildred Shapley Matthews. Tucson, Ariz. : University of Arizona Press, c1984 Soter, S Brightness of Iapetus. Paper presented at IAU Colloq. 28, Cornell University, August Squyres et al. (1984). Voyager Photometry of Iapetus. Icarus, 59,

12/2/04ESS 298 Fall The End!

12/2/04ESS 298 Fall The Facts Phoebe exogenic models (Soter 1974) - fact 4 Endogenic models - fact 3 Superficial layer of ice covering underlying dark surface - fact 5 Saturn book p. 853 Inconsistencies