Nick Cooper, Stefan Renner Carl Murray Encelade Meeting, UPMC, 22 January 2014 Recent Results on the Dynamics of Atlas.

Slides:



Advertisements
Similar presentations
Origins of Regular and Irregular Satellites ASTR5830 March 19, :30-1:45 pm.
Advertisements

Saturn’s Small Moons and Faint Rings : The View from Cassini Nick Cooper (with thanks to Carl Murray, Kevin Beurle, Mike Evans, Gareth Williams and the.
March , Birmingham GR tests and micro-arcsecond light bending parameters by global and differential Gaia mesurements Maria Teresa Crosta Astronomical.
ASTM001/MTH724U SOLAR SYSTEM Carl Murray / Nick Cooper Lecture 2: Structure of the Solar System.
MTH724U/ASTM001 SOLAR SYSTEM Nick Cooper/Carl Murray Lecture 9: Chaos and Long- Term Evolution.
GN/MAE155B1 Orbital Mechanics Overview 2 MAE 155B G. Nacouzi.
Dusty plasma near Enceladus South Pole M. Shafiq, M. W. Morooka and J.-E. Wahlund Swedish Institute of Space Physics, Uppsala, Sweden.
Asteroid Resonances [1]
Solving Equations = 4x – 5(6x – 10) -132 = 4x – 30x = -26x = -26x 7 = x.
GRACE GRAVITY FIELD SOLUTIONS USING THE DIFFERENTIAL GRAVIMETRY APPROACH M. Weigelt, W. Keller.
Geocentric Model. Epicycles & Deferents Galileo’s discoveries Moon has mountains.
11/15/99Norm Herr (sample file) SOLAR SYSTEM The Sun Nine Planets Sixty-one satellites of the planets Many Comets and asteroids.
NASA Finds Saturn's Moons May Be Creating New Rings October 11, 2006
Interaction Picture – Review Assume that we know solution.
Probing the Dynamics of Saturn’s Rings A.S. Bosh (Lowell Obs.), J.L. Elliot, C.B. Olkin, R.G. French, J. Rayner.
The most distant planet known to the ancients is NASA’s latest target for exploration.
Based on the definition given by Kasting et al. (1993). The Habitable Zone.
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.
Saturn By: Zack and Kacey.
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.
Saturn By Ola Smith This is a full colour view of Saturn and it’s rings taken from Voyager 2 on July
Phases of the Moon. Spin and orbital frequencies.
Mass Determination of Asteroids Kleinplanetentagung Heppenheim, 2005 Mike Kretlow.
Topic Three: Perturbations & Nonlinear Dynamics UW Spring 2008 Accelerator Physics J. J. Bisognano 1 Accelerator Physics Topic III Perturbations and Nonlinear.
Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington.
The Planet Saturn Mia and Kaylah. Saturn Facts Saturn is the sixth planet from the sun. It is the second largest in the solar system Saturn has an equatorial.
The Forces that Sculpt Saturn’s Rings…. Matt Hedman Cassini ISS team Cassini VIMS team CHARM telecon
Orbital Dynamics of Venus (and some of those other things out there) Billy Teets, PhD Candidate Dept. of Physics & Astronomy Vanderbilt University.
Orbits.
Rings Node Migration Plan Mark & Mitch PDSMC, UCLA November 28-29, 2012.
Dynamics. Solar System Explorers 05 How does the Sun affect objects in the Solar System?
David Nesvorny David Vokrouhlicky (SwRI) Alessandro Morbidelli (CNRS) David Nesvorny David Vokrouhlicky (SwRI) Alessandro Morbidelli (CNRS) Capture of.
Astronomy 340 Fall December 2005 Class #27.
An assessment of the NRLMSISE-00 density thermosphere description in presence of space weather events C. Lathuillère and M. Menvielle The data and the.
Title: SHAPE OPTIMIZATION OF AXISYMMETRIC CAVITATOR IN PARTIALY CAVITATING FLOW Department of Mechanical Engineering Ferdowsi University of Mashhad Presented.
Introduction4 Data acquisition and analysis8 Results17 Conclusion24 ASTEROID PHOTOMETRY GROUP, VSA
Jupiter (Galileo) Saturn (Cassini) Uranus (Hubble) Neptune (Voyager)
Proportionality between the velocity V and radius r
Saturn!!. FACTS!! Saturn has no life forms. Saturn has no life forms. Saturn is the sixth planet from the sun. Saturn is the sixth planet from the sun.
Integration for physically based animation CSE 3541 Matt Boggus.
1 Imaging the natural satellites J.E. Arlot IMCCE/CNRS/observatoire de Paris Astro/photo/phemu meeting October 14-18, 2015.
1 Phenomena in the Solar System: need of network of observation J.E. Arlot, M. Stavinschi IMCCE/CNRS/observatoire de Paris Institut astronomique de l’académie.
Development of Regular & Singular Perturbation Methods Anshu Narang-Siddarth.
The outer solar system: some points of physics A few points of physics I didn’t deal with earlier.
Moons of Jupiter and Saturn
GEOL 3045: Planetary Geology Lysa Chizmadia Saturn’s Satellites Lysa Chizmadia Saturn’s Satellites.
Boom and Bust Cycles in Saturn’s Rings? Larry W. Esposito LASP, University of Colorado 23 February 2010.
Some Peculiar Features In Saturn’s Rings Quentin Donnellan.
Saturn By: Maryellen.
SATURN’S RINGS Beatriz Frisón Máster en Astrofísica.
Observation vs. Inferences The Local Environment.
Natural satellites dynamics and internal structure 23 September 2004 Valéry Lainey, MAGE network.
26th October 2005 HST Calibration Workshop 1 The New GSC-II and it’s Use for HST Brian McLean Archive Sciences Branch.
ENA generation mechnism Krimigis et al, 2004 Some Questions about the Interaction between Trapped Particles and Neutrals l What is the source of trapped.
Celestial Mechanics I Introduction Kepler’s Laws.
Celestial Mechanics VI The N-body Problem: Equations of motion and general integrals The Virial Theorem Planetary motion: The perturbing function Numerical.
Boom and Bust Cycles in Saturn’s rings? Larry W. Esposito, Bonnie Meinke, Nicole Albers, Miodrag Sremcevic LASP/University of Colorado DPS Pasadena 5 October.
Capture of Irregular Satellites during Planetary Encounters
(2) Norut, Tromsø, Norway Improved measurement of sea surface velocity from synthetic aperture radar Morten Wergeland Hansen.
Analysis of Density Waves in UVIS Ring Stellar Occultations
Towards a kinematic model of the Local Group as-Astrometry with VLBI
Cassini UVIS Icy Satellites: Update and Progress on Analysis
Find 4 A + 2 B if {image} and {image} Select the correct answer.
ORBITAL Trajectories!!! Made by Karol Sanchez
Disk-integrated observations
UVIS results and ring evolution
题 目: 报告人: 摘 要: 时 间: 地 点: 欢迎大家积极参与!
What do we know? Fg = 78.6 N Fg = mg = (8)(9.8) = 78.4 N 1.
What do we know? Fg = 78.6 N Fg = mg = (8)(9.8) = 78.4 N 1.
Presentation transcript:

Nick Cooper, Stefan Renner Carl Murray Encelade Meeting, UPMC, 22 January 2014 Recent Results on the Dynamics of Atlas

Charnoz et al. (2010)

Astrometric Data 2580 Cassini ISS observations of Atlas, Prometheus, Pandora, Janus, Epimetheus QM SATELLORB and F Ring Images Data span Feb 2004 to Aug 2013 Atlas observations mostly centroided UCAC2 for pointing correction Phase correction SATELLORB astrometry by Mike Evans

Numerical Model Integration of full equations of motion in 3D Perturbations from 8 major satellites, Sun, Jupiter Saturn’s oblateness up to J6 Runge-Kutta-Nystrom 12 th order integrator Variational equations integrated simultaneously, iteratively fitting to observations Solving for states and masses of Atlas, Prometheus, Pandora, Janus and Epimetheus at epoch

Pre-fit (SAT353)Post-fit O-C Residuals

O-C Post-fit Residuals

Mean longitudes vs. time Resonant arguments vs. time ILR CER

Full Numerical Model Atlas, Prometheus, Saturn only Atlas Geometrical Elements

FLI vs time Full Numerical Model 3-body Numerical Model (Atlas, Prometheus, Saturn)

(Starting Conditions from Numerical Fit) Coralin Surfaces of Section ATLAS a_mean= km

Coralin Surfaces of Section (Starting Conditions from 3-body Model) ATLAS a_mean= km

Summary Fit to new astrometry: significant reduction in O-C residuals. Order of Magnitude improvement in mass estimates. Atlas dynamics dominated 54:53 resonance with Prometheus. Another example of coupled ILR/CER motion! Regular and chaotic episodes (FLI analysis). Chaos is due to Prometheus only. Atlas, Prometheus dynamics can be modelled as a 3-body system (CORALIN).