Cassini Encounters Enceladus: Background and the Discovery of a South Polar Hot Spot
|
|
- Austin Tyler
- 6 years ago
- Views:
Transcription
1 Cassini Encounters Enceladus: Background and the Discovery of a South Polar Hot Spot Spencer et al., 10 March 2006, Science, 311, 1401 Presented by Shannon Guiles Astronomy 671 April 10, 2006 Image Credit: NASA/JPL/GSFC
2 Tiger! Tiger! burning bright, In the forests of the night, What immortal hand or eye Could frame thy fearful symmetry?
3 Cassini Cassini entered orbit around Saturn on 1 July 2004, and it will orbit there for four years. Credit: NASA Cassini has 12 instruments while the Hyugens probe (which descended to Titan's surface in January 2005) had 6. CIRS Credit: NASA Cassini had three close flybys of Enceladus between Feb & July One more scheduled for Spring 2008.
4 Cassini Composite Infrared Spectrometer Reference: Flazar et al. (2004)
5 In what distant deeps or skies Burnt the fire of thine eyes? On what wings dare he aspire? What the hand dare seize the fire?
6 Enceladus Credit: NASA/JPL/Space Science Institute. Composite of UV (338 nm), green (568 nm), and IR (752 nm). discovered in 1789 by William Hershel 6th largest moon of Saturn orbits close to Saturn at r= 3.94 r_saturn eccentricity = , in 2:1 orbital resonance with Dione Voyager found (1981) r_enceladus = 252 km high visual geom. albedo implying fresh snow or ice vastly different surfaces resides in the middle of Saturn's E ring, and probably its source surface dominated by water ice with organics and CO2 coincident with tiger stripes
7 Why do we care? Scientists like a good puzzle. Before Cassini observations of Enceladus' South Pole, it was expected that Enceladus would be cold. Surprise! Enceladus is one of only 3 outer solar system bodies (along with Jupiter's Io & Neptune's Triton) where active geological eruptions have now been seen. What is the origin of Enceladus' internal heating? Possibility of life?
8 The Puzzle Only previous measurement of Enceladus' thermal radiation made by Voyager 2 in 1981 inferred temperatures of 75 +/ 3 K. Left: Predicted temperatures on Enceladus based on solar heating. Right: Temperature image from measurements of Enceladus' heat radiation from 9 to 16.5 microns. Image Credit: NASA/JPL/GSFC
9 And what shoulder and what art Could twist the sinews of thy heart? And, when thy heart began to beat, What dread hand and what dread feet?
10 Cassini CIRS Observations of Enceladus Far IR brightness temperature images of the thermal emission from the anti Saturn hemisphere of Enceladus Figure 1(A) of Spencer et al. (2006).
11 Thermal Model Fits to Determine Physical Properties Temperatures near 76 K consistent with Voyager estimates Note the large spatial variations in the thermal inertia (TI). TI is 100 x < TI of solid water ice, implying a very lose surface. The high albedo is consistent with Voyager determination of / Figure 1 (B) of Spencer et al. (2006). Temperatures measured during orbits 3 and 4. Thermal Inertia (T.I.) in MKS units of J m 2 s 1/2 K 1
12 What the hammer? what the chain? In what furnace was thy brain? What the anvil? what dread grasp Dare its deadly terrors clasp?
13 Mid-IR Data on Enceladus' South Pole (12.5 to 16 µm) Figure 2 of Spencer et al. (2006).
14 Mid-IR Data on Enceladus' South Pole The FIR detector has low spatial resolution, but MIR detector made a map with resolution of 25 km from 12.5 to 16 µm (Fig. 2 A and B). Equatorial regions had 650 cm 1 brightness temperatures ~77 K, in agreement with models of passive solar heating based on thermal inertias and albedos determined from FIR observations (Fig. 1). Surprise: near the south pole brightness temperatures reach 85 K (thermal models predicted a temperature of ~68 K, assuming zero thermal inertia, at the pole because of the oblique angle of Sun's rays there).
15 Mid-IR Data on Enceladus' South Pole A greybody fit to the south polar spectrum implies temperatures of 133 +/ 12 K from ~ % of the area (Fig. 2 C). They used Monte Carlo simulations to determine the uncertainties in the temperature and area found from the spectral fit (Fig. 2 D E). Temperatures below 110 K are very unlikely. The spectral fit was used to estimate the total radiated power from the southern hot spot of 5.8 +/ 1.9 GW (Fig. 2F).
16 What Causes the Hot Is it seasonal effects? No. The season is midway between the southern summer solstice & fall equinox, and a nonzero thermal inertia would cause the temperature to be even lower. How about a solid state greenhouse effect? Spot at the South Pole? Probably not. This is where solar radiation gets trapped beneath the surface, & might make warm gases that could escape along fractures and cause plumes. Proposed for Neptune's Triton. Good in theory, difficult in practice. A heat source from within? Quite possibly. The hot spot is located in a recently resurfaced region that has four big troughs (tiger stripes ~130 km long, ~500 m deep, ~2 km wide from ISS imaging).
17 Thermal Emission Associated with Individual Tiger Stripes Precise locations of hot sources A and B. MIR FOV is 17.5 km for source A and 6.0 km for source B. Figure 3 of Spencer et al. (2006).
18 Of Hot Spots and Tiger Stripes During the last 2.5 hours of the approach to Enceladus' South Pole, CIRS pointed where the optical cameras pointed. These high spatial resolution observations confirm that the hot spots are associated with individual tiger stripe troughs (Fig. 3). Properties of individual hot spots: Table 2 of Spencer et al. (2006).
19 When the stars threw down their spears, And watered heaven with their tears, Did He smile His work to see? Did He who made the Lamb, make thee?
20 Plume, Hot SpotS and Tiger Stripes Likely that warm tiger stripes are the source of the dust and vapor plume seen by other Cassini instruments Assuming the plume originates from thermal sublimation of warm water ice this warm ice is visible to CIRS Then using Cassini ISS image of Fountains of Enceladus. Credit: NASA/JPL/Space Science Institute escape rate = (5 10)x1027 molecules/second mean south polar radiance at 900 cm 1 of ~ 5x10 10 W cm 2str 1(cm 1) 1 Get plume source temperature > 180 K
21 Plume, Hot SpotS, & Tiger Stripes In order to produce the escape rate in the plume, a 180 K plume source must have an area of ~ 28 km2 consistent with a 50 m width along each of the four tiger stripes The 345 km2 area of the south polar hot spots is in agreement with all the hot material being concentrated along the tiger stripes derive a width of ~660 m (4 stripes x 139 km length x km width = 343 km2 ), consistent with that derived from high resolution spectra.
22 In what funace was thy brain? - Possible Heat Sources Radioactive decay. The max power from this, assuming a meteor (chondritic = silicate blob) composition for non ice material in Enceladus is ~ 0.1 GW << the 6 GW inferred from observations. Tidal heating may generate 1 10 GW Enceladus is in a 2:1 mean motion orbital resonance with Dione. Enceladus may have been in a 1:4 spin orbit resonance in the past (based on the analysis of Enceladus' shape, Porco et al, 2006). This would have caused strong tidal heating, from which Enceladus may still be cooling down.
23 Tiger! Tiger! burning bright, In the forests of the night, What immortal hand or eye Dare frame thy fearful symmetry?
24 Summary Cassini CIRS found Enceladus is generating ~ 6 GW from within at temperatures around 150 K Comparison with Cassini visual images most if not all of the heat is concentrated along the tiger stripe troughs Warm troughs probably source of vapor and dust plumes seen by other Cassini instruments
25 References Cassini Encounters Enceladus: Background and the Discovery of a South Polar Hot Spot, Spencer et al. (2006) Science, 311, 1401 Exploring the Saturn System in the Thermal Infrared: the Composite Infrared Spectrometer, Flazar et al. (2004) Space Science Reviews, 115, 169 Cassini Observes the Active South Pole of Enceladus, Porco et al. (2006) Science, 311, 1393 wikipedia article on Enceladus at: Cassini home page at:
26 The Tiger Tiger! Tiger! burning bright, In the forests of the night, What immortal hand or eye Could frame thy fearful symmetry? What the hammer? what the chain? In what furnace was thy brain? What the anvil? what dread grasp Dare its deadly terrors clasp? In what distant deeps or skies Burnt the fire of thine eyes? On what wings dare he aspire? What the hand dare seize the fire? When the stars threw down their spears, And watered heaven with their tears, Did He smile His work to see? Did He who made the Lamb, make thee? And what shoulder and what art Could twist the sinews of thy heart? And, when thy heart began to beat, What dread hand and what dread feet? Tiger! Tiger! burning bright, In the forests of the night, What immortal hand or eye Dare frame thy fearful symmetry? William Blake ( )
27 Artist's Conception of Enceladus Image Credit: NASA
AST 248, Lecture 21. James Lattimer. Department of Physics & Astronomy 449 ESS Bldg. Stony Brook University. November 15, 2018
vi AST 248, Lecture 21 James Lattimer Department of Physics & Astronomy 449 ESS Bldg. Stony Brook University November 15, 2018 The Search for Intelligent Life in the Universe james.lattimer@stonybrook.edu
More informationChapter 4: William Blake
Romanticism Chapter 4: William Blake The Tyger, The Sick Rose, The Fly, London 2011 Fall Sehjae Chun Largely unrecognized during his lifetime, William Blake is now considered a seminal figure in the history
More informationJovian planets, their moons & rings
Jovian planets, their moons & rings The Moons of the Jovian Planets The terrestrial planets have a total of 3 moons. The jovian planets have a total of 166 moons. Each collection of moons orbiting the
More informationASTR-1010: Astronomy I Course Notes Section X
ASTR-1010: Astronomy I Course Notes Section X Dr. Donald G. Luttermoser Department of Physics and Astronomy East Tennessee State University Edition 2.0 Abstract These class notes are designed for use of
More informationJovian Planet Systems
Jovian Planet Systems Reading: Chapter 14.1-14.5 Jovian Planet Systems Voyager 1 and 2 explored the outer planets in the 1970s and 1980s. The Galileo spacecraft circled Jupiter dozens of times in the late
More informationLEARNING ABOUT THE OUTER PLANETS. NASA's Cassini spacecraft. Io Above Jupiter s Clouds on New Year's Day, Credit: NASA/JPL/University of Arizona
LEARNING ABOUT THE OUTER PLANETS Can see basic features through Earth-based telescopes. Hubble Space Telescope especially useful because of sharp imaging. Distances from Kepler s 3 rd law, diameters from
More informationMimas, moon of Saturn and Death Star impersonator responsible for several gaps in Saturn s ring system
Last time: Gravitational signs of large outer moons in the rings Ring shepherding/gap maintenance Longer lived structures due to mean motion resonances with large satellites Example: 2:1 resonance with
More informationPhys 214. Planets and Life
Phys 214. Planets and Life Dr. Cristina Buzea Department of Physics Room 259 E-mail: cristi@physics.queensu.ca (Please use PHYS214 in e-mail subject) Lecture 29. Search for life on jovian moons. Habitability.
More informationHigh heat flow from Enceladus south polar region measured using cm 1 Cassini/CIRS data
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116,, doi:10.1029/2010je003718, 2011 High heat flow from Enceladus south polar region measured using 10 600 cm 1 Cassini/CIRS data C. J. A. Howett, 1 J. R. Spencer,
More informationThe Fathers of the Gods: Jupiter and Saturn
The Fathers of the Gods: Jupiter and Saturn Learning Objectives! Order all the planets by size and distance from the Sun! How are clouds on Jupiter (and Saturn) different to the Earth? What 2 factors drive
More informationSOLAR SYSTEM B Division
SOLAR SYSTEM B Division Team Name: Team #: Student Names: IMAGE SHEET A E B C D F G H Spectrum I Spectrum II SS2014 Spectrum III Spectrum IV Spectrum V Spectrum VI 1. A. What satellite is pictured in Image
More informationAmazing Saturn. Saturn from the ground
1 Amazing Saturn Saturn from the ground 2 Saturn Information Overload The Cassini Mission started orbiting Saturn in 2004. 3 Getting There Planetary pinball with passes by Venus, Venus, Earth, and Jupiter
More informationImage: solarsystem.nasa.gov. Orbital trajectory of Cassini spacecraft ( ).
1 Enceladus This image, acquired by the Cassini spacecraft, captures Saturn, its rings (edge on), and the moon Enceladus. It was discovered that this moon emits jets of ice from possible underground seas.
More informationChapter 11 Jovian Planet Systems. Comparing the Jovian Planets. Jovian Planet Composition 4/10/16. Spacecraft Missions
Chapter 11 Jovian Planet Systems Jovian Planet Interiors and Atmospheres How are jovian planets alike? What are jovian planets like on the inside? What is the weather like on jovian planets? Do jovian
More informationWeather in the Solar System
Weather in the Solar System Sanjay S. Limaye Space Science and Engineering Center University of Wisconsin-Madison 8 February 2002 What is Weather? Webster s New Collegiate Dictionary: state of the atmosphere
More informationAstronomy November, 2016 Introduction to Astronomy: The Solar System. Mid-term Exam 3. Practice Version. Name (written legibly):
Astronomy 101 16 November, 2016 Introduction to Astronomy: The Solar System Mid-term Exam 3 Practice Version Name (written legibly): Honor Pledge: On my honor, I have neither given nor received unauthorized
More informationLast Class. Today s Class 11/28/2017
Today s Class: The Jovian Planets & Their Water Worlds 1. Exam #3 on Thursday, Nov. 30 th! a) Covers all the reading Nov. 2-28. b) Covers Homework #6 and #7. c) Review Space in the News articles/discussions.
More informationEnceladus. Michelle Wenz
Enceladus Michelle Wenz Enceladus General Information Diameter 314 miles (505 km) Fit in Arizona (Pozio 1995) 1/7 th of Earth s moon diameter Herschel discovered in 1789 During the equinox of Saturn (reduced
More informationDirected Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past?
Skills Worksheet Directed Reading Section: Viewing the Universe 1. How did observations of the sky help farmers in the past? 2. How did observations of the sky help sailors in the past? 3. What is the
More informationUranus & Neptune, The Ice Giants
Uranus & Neptune, The Ice Giants What We Will Learn Today How & When were Uranus & Neptune discovered? How are the interiors and weather on these planets? Why is Neptune as warm as Uranus? What are their
More information1. The Sun is a huge ball of very hot gas in space, which radiates heat and light in one direction.
PLEASE ANSWER YOUR QUESTIONS ON THIS PROVIDED QUESTION PAPER. EACH QUESTION IS FOLLOWED BY ANSWERS MARKED A AND B, OR A, B, C AND D. ONLY ONE ANSWER IS CORRECT. CHOOSE THE MOST CORRECT ANSWER AND CIRCLE
More informationScientists are gushing over a discovery by the Cassini spacecraft evidence of water on one of Saturn s many moons!
Cold Faithful Geysers Spout From Icy Saturn Moon Scientists are gushing over a discovery by the Cassini spacecraft evidence of water on one of Saturn s many moons! Cassini snapped shots of Enceladus (en-sell-ahdus)
More informationASTR 380 Possibilities for Life in the Outer Solar System
ASTR 380 Possibilities for Life in the Outer Solar System Possibility of Life in the Inner Solar System The Moon, Mercury, and the Moons of Mars Deimos NO LIFE NOW or EVER This is a 98% conclusion! Phobos
More informationASTR 2020, Spring 2018
ASTR 2020, Spring 2018 Last Name First Name Professor Jack Burns Exam #3 April 27, 2018 Student ID Number A INSTRUCTIONS: Closed books, one page (2 sides) of notes allowed, calculators may be used, strictly
More informationAstronomy. Uranus Neptune & Remote Worlds
Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Uranus Neptune & Remote Worlds Uranus and Neptune Orbits and Atmospheres Internal Structure Magnetic Fields Rings Uranus's
More informationLife in the outer Solar System. AST 309 part 2: Extraterrestrial Life
Life in the outer Solar System AST 309 part 2: Extraterrestrial Life Prospects for life on: Overview: 1. Europa (Jupiter moon) 2. Titan (Saturn s moon) 3. Enceladus (Saturn s moon) Life on Europa? NASA
More informationLecture 11 The Structure and Atmospheres of the Outer Planets October 9, 2017
Lecture 11 The Structure and Atmospheres of the Outer Planets October 9, 2017 1 2 Jovian Planets 3 Jovian Planets -- Basic Information Jupiter Saturn Uranus Neptune Distance 5.2 AU 9.5 AU 19 AU 30 AU Spin
More informationPhys 214. Planets and Life
Phys 214. Planets and Life Dr. Cristina Buzea Department of Physics Room 259 E-mail: cristi@physics.queensu.ca (Please use PHYS214 in e-mail subject) Lecture 28. Search for life on jovian moons. March
More informationIcy Moons of Jupiter, Saturn, and Beyond Rosaly Lopes, JPL
Icy Moons of Jupiter, Saturn, and Beyond Rosaly Lopes, JPL Galilean satellites: Io, Europa, Ganymede, and Callisto Io: hot volcanoes, colorful surface, lots of sulfur, no impact craters Europa: icy crust,
More informationChapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres
Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds What is an atmosphere? Planetary Atmospheres Pressure Composition Greenhouse effect Atmospheric structure Color of the sky 1 Atmospheres
More informationChapter 17 Solar System
Chapter 17 Solar System Rotation Earth spinning on its axis (like a top) "TOP" imaginary rod running through the center of the Earth from North pole to South pole The Earth is tilted on its axis at an
More informationChapter 26 Section 1 pages Directed Reading Section: Viewing the Universe
Name: Period: Chapter 26 Section 1 pages 659-666 Directed Reading Section: Viewing the Universe 1. How did observations of the sky help sailors in the past? 2. What is the main reason people study the
More information9/1/14. Chapter 2: Heating Earth s Surface and Atmosphere. The Atmosphere: An Introduction to Meteorology, 12 th. Lutgens Tarbuck
Chapter 2: Heating Earth s Surface and Atmosphere The Atmosphere: An Introduction to Meteorology, 12 th Lutgens Tarbuck Lectures by: Heather Gallacher, Cleveland State University! Earth s two principal
More information1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely
CHAPTER 3 SOLAR AND TERRESTRIAL RADIATION MULTIPLE CHOICE QUESTIONS 1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely 2. is the distance between successive
More informationASTR 1050: Survey of Astronomy Fall 2012 PRACTICE Exam #2 Instructor: Michael Brotherton Covers Solar System and Exoplanet Topics
ASTR 1050: Survey of Astronomy Fall 2012 PRACTICE Exam #2 Instructor: Michael Brotherton Covers Solar System and Exoplanet Topics Instructions This exam is closed book and closed notes, although you may
More information1781: Uranus Discovered. The Outer Worlds. 1846: Neptune Discovered. Distance Comparison. Uranus Rotates Sideways. Exaggerated Seasons On Uranus
The Outer Worlds 1781: Discovered (accidentally!) by William Herschel using a 6 inch telescope [he thought it was a comet!] 2 Draft 12/03/2006 Updated May 05, 2011 1846: Discovered Le Verrier: proposed
More informationChapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization
Objectives Describe characteristics of the universe in terms of time, distance, and organization Identify the visible and nonvisible parts of the electromagnetic spectrum Compare refracting telescopes
More informationMULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version E of the exam. Please fill in (E). A) This
More information4. THE SOLAR SYSTEM 1.1. THE SUN. Exercises
4. THE SOLAR SYSTEM 1.1. THE SUN The sun is the star located in the center of the solar system. The sun is a yellow star, since its superficial temperature is about 5.500 C (although, the temperature can
More informationThe Solar System. Tour of the Solar System
The Solar System Tour of the Solar System The Sun more later 8 planets Mercury Venus Earth more later Mars Jupiter Saturn Uranus Neptune Various other objects Asteroids Comets Pluto The Terrestrial Planets
More information12. Jovian Planet Systems Pearson Education Inc., publishing as Addison Wesley
12. Jovian Planet Systems Jovian Planet Properties Compared to the terrestrial planets, the Jovians: are much larger & more massive 2. are composed mostly of Hydrogen, Helium, & Hydrogen compounds 3. have
More informationMULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version B of the exam. Please fill in (B). A) This
More information12a. Jupiter. Jupiter Data (Table 12-1) Jupiter Data: Numbers
12a. Jupiter Jupiter & Saturn data Jupiter & Saturn seen from the Earth Jupiter & Saturn rotation & structure Jupiter & Saturn clouds Jupiter & Saturn atmospheric motions Jupiter & Saturn rocky cores Jupiter
More informationThe Jovian Planets and Their Moons
The Jovian Planets and Their Moons Jupiter 1 Physical Properties of Earth and Jupiter Jupiter Earth Equatorial lradius 11.2 R Earth 6378 km Mass 318 M Earth 5.976 10 24 kg Average Density 1.34 g/cm 3 5.497
More information2/22/ Atmospheric Characteristics
17.1 Atmospheric Characteristics Atmosphere: the gaseous layer that surrounds the Earth I. In the past, gases came from volcanic eruptions A. Water vapor was a major component of outgassing B. Other gases
More informationThe moons of Saturn 7 August 2015, by Matt Williams
The moons of Saturn 7 August 2015, by Matt Williams the irregular moons in the outermost regions have orbital radii of millions of kilometers, orbital periods lasting several years, and move in retrograde
More informationChapter 2. Heating Earth's Surface & Atmosphere
Chapter 2 Heating Earth's Surface & Atmosphere Topics Earth-Sun Relationships Energy, Heat and Temperature Mechanisms of Heat Transfer What happens to Incoming Solar Radiation? Radiation Emitted by the
More informationThe Icy Moons. and the. Extended Habitable Zone
The Icy Moons and the Extended Habitable Zone Europa Interior Models Other Types of Habitable Zones Water requires heat and pressure to remain stable as a liquid Extended Habitable Zones You do not need
More informationPhysics 3/3/2013. Kepler s Three Laws of Planetary Motion. Distance, Velocity from the Sun at any given time: q=angle from perihelion
Physics Kepler s Three Laws of Planetary Motion a=semi-major axis b=semi-minor axis e=eccentricity Focus, Foci Distance, Velocity from the Sun at any given time: a(1 e ) r 1 ecosq v 1 GM ro a q=angle from
More informationChapter 11 Lecture. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc.
Chapter 11 Lecture The Cosmic Perspective Seventh Edition Jovian Planet Systems Jovian Planet Systems 11.1 A Different Kind of Planet Our goals for learning: Are jovian planets all alike? What are jovian
More informationInvestigating Planets Name: Block: E1:R6
FYI: Planetary Temperatures and Atmospheres Read FYI: A Planet s Temperature, The Importance of an Atmosphere, and The Greenhouse Effect As you read answer the following questions about the readings: Word/Term
More informationMoon, Planet, Star, Solar System, Galaxy, Universe
Dr. V s Study Guide : Astronomy Unit 1) Place the following in order of increasing size: The Galaxy, the Solar System, a Star, the Universe,a Moon and a Planet. Moon, Planet, Star, Solar System, Galaxy,
More informationSimilarities & Differences to Inner Planets
Similarities & Differences to Inner Planets Jupiter Jupiter: Basic Characteristics Mass = 1.898 10 27 kg (318 x Earth) Radius = 71,492 km (11x Earth) Albedo (reflectivity) = 0.34 (Earth = 0.39) Average
More information[19] Jovian Planet Moons and Rings (11/2/17)
1 [19] Jovian Planet Moons and Rings (11/2/17) Upcoming Items Which of these is Europa? 1. Read Ch. 8.3 and 12.1 12.3 by next Thursday and do the self-study quizzes 2. Midterm #2 on Tuesday! 2 LEARNING
More informationThe Jovian Planets. Why do we expect planets like this in the outer reaches of the solar system?(lc)
The Jovian Planets Beyond Mars and the Asteroid belt are the Jovian or Gas Giant Planets that are totally different than the terrestrial planets: They are composed almost entirely of gas They do not have
More informationJupiter & Saturn. Moons of the Planets. Jupiter s Galilean satellites are easily seen with Earth-based telescopes. The Moons
The Moons Jupiter & Saturn Earth 1 Mars 2 Jupiter 63 Saturn 47 Uranus 27 Neptune 13 Pluto 3 Moons of the Planets Galileo (1610) found the first four moons of Jupiter. Total 156 (as of Nov. 8, 2005) Shortened
More informationMoonrise. Bonnie Meinke, PhD. the surprisingly diverse array of moons in our solar system. Hubble Science Briefing May 1, 2014
Moonrise the surprisingly diverse array of moons in our solar system Hubble Science Briefing May 1, 2014 Bonnie Meinke, PhD Inner Solar System Mercury Venus Earth Mars 0 moons 0 moons 1 moon 2 moons 2
More informationGiant Planets Or Why the Solar System Is the Way It Is. Dr. Josh Colwell University of Central Florida
Giant Planets Or Why the Solar System Is the Way It Is Dr. Josh Colwell University of Central Florida Almost everything you see in this image is a galaxy containing tens of billions of stars each. Figure
More informationChapter 15 & 16 Science Review (PATTERNS IN THE SKY, OUR SOLAR SYSTEM)
Chapter 15 & 16 Science Review (PATTERNS IN THE SKY, OUR SOLAR SYSTEM) The Milky Way the galaxy that contains our solar system Our solar system is a speck in the Milky Way galaxy Pluto is now considered
More informationCassini ISS. The Imaging Science Subsystem. (The Cameras)
Cassini ISS The Imaging Science Subsystem (The Cameras) "We are the eyes of Cassini, our cameras capture all the dramatic sights and vistas there are to see around Saturn. And through their imagery, they
More informationSATELLITES: ACTIVE WORLDS AND EXTREME ENVIRONMENTS. Jessica Bolda Chris Gonzalez Crystal Painter Natalie Innocenzi Tyler Vasquez.
SATELLITES: ACTIVE WORLDS AND EXTREME ENVIRONMENTS Jessica Bolda Chris Gonzalez Crystal Painter Natalie Innocenzi Tyler Vasquez. Areas of interest! How did the Satellites of the outer solar system form
More informationObject Type Moons Rings Planet Terrestrial none none. Max Distance from Sun. Min Distance from Sun. Avg. Distance from Sun 57,910,000 km 0.
Mercury Mercury is the closest planet to the sun. It is extremely hot on the side of the planet facing the sun and very cold on the other. There is no water on the surface. There is practically no atmosphere.
More informationUNIT 3: Chapter 8: The Solar System (pages )
CORNELL NOTES Directions: You must create a minimum of 5 questions in this column per page (average). Use these to study your notes and prepare for tests and quizzes. Notes will be turned in to your teacher
More informationLecture #11: Plan. Terrestrial Planets (cont d) Jovian Planets
Lecture #11: Plan Terrestrial Planets (cont d) Jovian Planets Mercury (review) Density = 5.4 kg / liter.. ~ Earth s Rocky mantle + iron/nickel core Slow spin: 59 days (orbital period = 88 days) No satellites
More informationChapter 8 Jovian Planet Systems
Chapter 8 Jovian Planet Systems They are much larger than terrestrial planets They do not have solid surfaces The things they are made of are quite different Terrestrial planets are made principally of
More informationChapter 8 Jovian Planet Systems
Chapter 8 Jovian Planet Systems They are much larger than terrestrial planets They do not have solid surfaces The things they are made of are quite different Terrestrial planets are made principally of
More informationAstronomy 1 Winter Lecture 15; February
Astronomy 1 Winter 2011 Lecture 15; February 9 2011 Previously on Astro-1 Mercury, Venus, Mars (and Earth) Size and composition Crusts and cores Volcanism and internal activity Stargazing Events Santa
More informationDr. Linda Spilker Cassini Project Scientist, JPL/Caltech Outer Planets Assessment Group 8 February 2016
Dr. Linda Spilker Cassini Project Scientist, JPL/Caltech Outer Planets Assessment Group 8 February 2016 Solstice Mission Inclination Profile Saturn s Breathing Atmosphere Saturn s atmosphere has been found
More informationExploring The Planets: Jupiter
Exploring The Planets: Jupiter By Encyclopaedia Britannica, adapted by Newsela staff on 08.28.17 Word Count 691 Level 800L New Horizons spacecraft took this collection of images of Jupiter and Io in 2007.
More informationJupiter. Jupiter, its atmosphere, and its magnetic field 10/19/17 PROBLEM SET #5 DUE TUESDAY AT THE BEGINNING OF LECTURE
Jupiter PROBLEM SET #5 DUE TUESDAY AT THE BEGINNING OF LECTURE 19 October 2017 ASTRONOMY 111 FALL 2017 1 Jupiter and Io as seen from Cassini as it flew by (JPL/NASA) Jupiter, its atmosphere, and its magnetic
More informationChapter 8 Jovian Planet Systems
Chapter 8 Jovian Planet Systems How do jovian planets differ from terrestrials? They are much larger than terrestrial planets They do not have solid surfaces The things they are made of are quite different
More informationTidal Heating of Moons
http://nssdc.gsfc.nasa.gov/image/planetary/comet/sl9pre_hst.jpg Tidal Heating of Moons http://photojournal.jpl.nasa.gov/catalog/pia11688 outreach@astronomy.nmsu.edu http://astronomy.nmsu.edu http://www.nasa.gov/multimedia/imagegallery
More informationAstronomy Ch. 11 Jupiter. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
Name: Period: Date: Astronomy Ch. 11 Jupiter MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Jupiter is noticeably oblate because: A) it has a
More informationAstronomy 111 Review Problems Solutions
Astronomy 111 Review Problems Solutions Problem 1: Venus has an equatorial radius of 6052 km. Its semi-major axis is 0.72 AU. The Sun has a radius of cm. a) During a Venus transit (such as occurred June
More informationSOLAR SYSTEM 2019 SAMPLE EXAM
SOLAR SYSTEM 2019 SAMPLE EXAM Team Name: Team #: No calculators are allowed. All questions are of equal weight unless otherwise noted. Turn in all materials when you have completed the test! Make sure
More informationAstronomy 1140 Quiz 4 Review
Astronomy 1140 Quiz 4 Review Anil Pradhan November 16, 2017 I Jupiter 1. How do Jupiter s mass, size, day and year compare to Earth s? Mass: 318 Earth masses (or about 1/1000th the mass of the Sun). Radius:
More informationThe Gas Giants Astronomy Lesson 13
The Gas Giants Astronomy Lesson 13 The four outer planets: Jupiter, Saturn, Uranus, and Neptune, are much larger and more massive than Earth, and they do not have solid surfaces. Because these planets
More informationElectromagnetic Radiation and Scientific Instruments. PTYS April 1, 2008
Electromagnetic Radiation and Scientific Instruments PTYS 206-2 April 1, 2008 Announcements Deep Impact 6 PM Wednesday Night Pizza, no beer Watch at home if you can t watch here. It will be discussed in
More information10/6/16. Observing the Universe with Gravitational Waves
Lecture Outline Observing the Universe with Gravitational Waves Thursday, October 13 7:00 PM Bell Museum Auditorium This event is free and open to the public, and will be followed by telescope observing.
More information9.2 - Our Solar System
9.2 - Our Solar System Scientists describe our solar system as the Sun and all the planets and other celestial objects, such as moons, comets, and asteroids, that are held by the Sun s gravity and orbit
More informationTitan and Enceladus after 7 years of. discoveries by Cassini
Titan and Enceladus after 7 years of 1. Titan Organic cycle Geological features Deep ocean 2. Enceladus Jets of vapor on the southern hemisphere Origin of the jets 3. New questions and future missions
More informationThe greenhouse effect
16 Waves of amplitude of 1 m roll onto a beach at a rate of one every 12 s. If the wavelength of the waves is 120 m, calculate (a) the velocity of the waves (b) how much power there is per metre along
More informationChapter 11 Review Clickers. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc.
Review Clickers The Cosmic Perspective Seventh Edition Jovian Planet Systems If Jupiter was the size of a basketball, Earth would be the size of a(n) a) bacterium. b) grain of rice. c) marble. d) orange.
More informationAstronomy Unit Notes Name:
Astronomy Unit Notes Name: (DO NOT LOSE!) To help with the planets order 1 My = M 2 V = Venus 3 Eager = E 4 M = Mars 5 Just = J 6 Served = Saturn 7 Us = Uranus 8 N = N 1 Orbit: The path (usually elliptical)
More informationDirected Reading B. Section: The Outer Planets
Skills Worksheet Directed Reading B Section: The Outer Planets 1. What is one way that gas giants differ from the terrestrial planets? a. They are much smaller. b. They are rocky and icy. c. They are made
More informationIX. Dwarf Planets A. A planet is defined to be an object that is large enough to coalesce into a sphere and to have cleared its orbit of other
7/1 VII. VIII. Uranus A. Gas Giant 1. Rings but not visible 2. HUGE axial tilt 97! 3. Mostly hydrogen and helium 4. Medium rotation rate 5. Cold 55 K at the cloud tops B. Physical characteristics 1. Mass:
More informationChapter 8 Jovian Planet Systems
Chapter 8 Jovian Planet Systems How do jovian planets differ from terrestrials? They are much larger than terrestrial planets They do not have solid surfaces The things they are made of are quite different
More information11.2 A Wealth of Worlds: Satellites of Ice and Rock
11.2 A Wealth of Worlds: Satellites of Ice and Rock Our goals for learning: What kinds of moons orbit the jovian planets? Why are Jupiter's Galilean moons so geologically active? What is remarkable about
More informationChapter 8 Jovian Planet Systems
Chapter 8 Jovian Planet Systems How do jovian planets differ from terrestrials? They are much larger than terrestrial planets They do not have solid surfaces The things they are made of are quite different
More informationLab #8. The Moons of the Outer Planets
Lab #8 The Moons of the Outer Planets Introduction In this lab, we will explore the outer planets and their fascinating moons using the latest information on the Web. There are several processes at work
More information3. The name of a particularly large member of the asteroid belt is A) Halley B) Charon C) Eris D) Ceres E) Triton
Summer 2013 Astronomy - Test 2 Test form A Name Do not forget to write your name and fill in the bubbles with your student number, and fill in test form A on the answer sheet. Write your name above as
More informationEffective August 2007 All indicators in Standard / 14
8-4.1 Summarize the characteristics and movements of objects in the solar system (including planets, moons, asteroids, comets, and meteors). Taxonomy level: 2.4-B Understand Conceptual Knowledge Previous/Future
More informationTransneptunian objects. Minor bodies in the outer Solar System. Transneptunian objects
Transneptunian objects Minor bodies in the outer Solar System Planets and Astrobiology (2016-2017) G. Vladilo Around 1980 it was proposed that the hypothetical disk of small bodies beyond Neptune (called
More informationEdmonds Community College Astronomy 100 Winter Quarter 2007 Sample Exam # 2
Edmonds Community College Astronomy 100 Winter Quarter 2007 Sample Exam # 2 Instructor: L. M. Khandro 1. Relatively speaking, objects with high temperatures emit their peak radiation in short wavelengths
More informationUranus & Neptune: The Ice Giants. Discovery of Uranus. Bode s Law. Discovery of Neptune
Uranus & Neptune: The Ice Giants Discovery of Uranus Discovery of Uranus & Neptune Properties Density & Composition Internal Heat Source Magnetic fields Rings Uranus Rotational Axis by William Herschel
More informationFormation of the Universe The organization of Space
February 21, 2014 Formation of the Universe The organization of Space Theory: A theory is An example is cell Cell Theory Cell Theory states 1. All living organisms are composed of one or more cells 2.
More informationExam# 1 Review Gator 1 Keep the first page of the exam. Scores will be published using the exam number Chapter 0 Charting the Heavens
Exam# 1 Review Exam is Wednesday October 11 h at 10:40AM, room FLG 280 Bring Gator 1 ID card Bring pencil #2 (HB) with eraser. We provide the scantrons No use of calculator or any electronic device during
More informationEarth, Uranus, Neptune & Pluto. 14a. Uranus & Neptune. The Discovery of Uranus. Uranus Data: Numbers. Uranus Data (Table 14-1)
14a. Uranus & Neptune The discovery of Uranus & Neptune Uranus is oddly tilted & nearly featureless Neptune is cold & blue Uranus & Neptune are like yet dislike Jupiter The magnetic fields of Uranus &
More informationAstronomy 1140 Quiz 3 Review
Astronomy 1140 Quiz 3 Review Anil Pradhan October 26, 2016 I The Inner Planets 1. What are the terrestrial planets? What do they have in common? Terrestrial planets: Mercury, Venus, Earth, Mars. Theses
More informationEdmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006
Edmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006 Instructor: L. M. Khandro 10/19/06 Please Note: the following test derives from a course and text that covers the entire topic of
More information