3D representation of the Non-Rotating Origin Olivier de Viron and Veronique Dehant Royal Observatory of Belgium Scientific adviser: Nicole Capitaine.

Slides:



Advertisements
Similar presentations
Astronomy Class Notes Jim Mims.
Advertisements

The 3D representation of the new transformation from the terrestrial to the celestial system. Véronique Dehant, Olivier de Viron Royal Observatory of Belgium.
MAE 5410 – Astrodynamics Lecture 5 Orbit in Space Coordinate Frames and Time.
A comparison of R1 and R4 IVS networks S.B. Lambert, Royal Observatory of Belgium, formerly at NVI, Inc./US Naval Observatory A.-M. Gontier, Paris Observatory.
Processing of VLBI observation in St. Petersburg University Kudryashova Maria Astronomical Institute of Saint Petersburg University.
Chapter 1: Introduction to Earth
Axial tilt is an astronomical term regarding the inclination angle of Earth’s rotational axis in relation to a perpendicular to its orbital plane Solar.
The old geocentric view of the universe held that the Earth was surrounded by a celestial sphere that held the stars: 1) never moved. 2) rotated from east.
Solar vs. Sidereal Day.
Astronomy and Cosmology week 2 - Tuesday Star Date Short lecture on Ch.1-2 Questions? Your Web-X posts Thursday assignments Solar motion workshop: predictions.
Constellations. Celestial Sphere Our Point of View.
Roger A. Freedman • William J. Kaufmann III
AST 208 Topics Time and celestial coordinates. Telescopes.
Run 1 Ball at rest relative to inertial frame On a flat rotating disk.
Lecture Notes on Astrometry Rotation (Euclidean) Distance-Invariant Finite Rotation: Matrix representation Orthogonality.
1 O Path Reference Frame (x,y) coord r  (r,  ) coord x yr Path Reference Frame x yr (n,t) coord velocity meter Summary: Three Coordinates (Tool) Velocity.
Read pp Do 6, 11, 12, 28. Pendula (or Pendulums, in the vernacular)
Grab your text book Chapter 1 Astronomy Today 7th Edition
Modern Navigation Thomas Herring MW 11:00-12:30 Room
Theory of Machines Lecture 4 Position Analysis.
Lab Intro & Lab 1: Celestial Sphere & Planispheres Tiffany Pewett 25 Park Place, 625E.
Coordinate systems on the Moon and the physical libration Natalia Petrova Kazan state university, Russia 20 September, 2007, Mitaka.
AAS 2004 Denver, 2004 May 31 SOFA software support for IAU 2000 Patrick Wallace Rutherford Appleton Laboratory, UK
Astronomical Coordinates Summary
University of Colorado Boulder ASEN 5070: Statistical Orbit Determination I Fall 2014 Professor Brandon A. Jones Lecture 3: Basics of Orbit Propagation.
Athanasios Dermanis and Dimitrios Tsoulis Numerical evidence for the inconsistent separation of the ITRF-ICRF transformation into precession-nutation,
Compatibility of the IERS earth rotation representation and its relation to the NRO conditions Athanasios Dermanis Department of Geodesy and Surveying.
Astronomy Picture of the Day
The ICRF, ITRF and VLBA Chopo Ma NASA’s Goddard Spaceflight Center.
Announcements Clear sky patrol has not yet started We will start using PRS units this week, make sure that you have one.
Introduction to Positional Astronomy The Night Sky  Nick Devereux 2006.
Constellations. I. Constellations A. A constellation is typically thought of as a collection of ____________ named after _______________, ______________.
University of Colorado Boulder ASEN 5070: Statistical Orbit Determination I Fall 2015 Professor Brandon A. Jones Lecture 3: Time and Coordinate Systems.
1 Lines in the Sky In order to use the sky to measure time you need to measure the location of objects in the sky. We will look at two methods of measuring.
22.2 The Earth-Moon-Sun System Pages I. Motions of Earth A. Rotation (Spinning) 1. Causes: Day and Night 1. Causes: Day and Night hours-
Another Look at Non-Rotating Origins George Kaplan Astronomical Applications Department U.S. Naval Observatory
Earth in Space Mr. Woodham’s 6 th Grade Earth Science Class.
What causes the Seasons?. The Earth’s orbit Seasons do NOT arise from the distance the Earth is from the Sun but rather as a result of the Earth’s annual.
Coordinate Transformations TM, A. Tamburro Based on Slalib docs/sun67.htx/sun67.html Tested against MACRO algorithms and.
RELATIVE MOTION An important concept of formalize.
Catherine LeCocq SLAC USPAS, Cornell University Large Scale Metrology of Accelerators June 27 - July 1, 2005 Coordinate Systems 1 Coordinate Systems Purpose:
Seasonal Motion.
Earth and the Universe Eric Angat Teacher PMHS.
Geodesy with Mars lander Network V. Dehant, J.-P. Barriot, and T. Van Hoolst Royal Observatory of Belgium Observatoire Midi-Pyrénées.
How do we get our seasons?. The AXIS is important! The axis is the imaginary line through Earth from the North Pole to the South Pole. The earth spins.
Seasonal Motion. Daily and yearly motion intertwined Solar vs Siderial Day –Earth rotates in 23 h 56 m –also rotates around sun  needs 4 min. to “catch.
Chapter 0: Charting the Heavens. Units of Chapter 0 The “Obvious” View Earth’s Orbital Motion The Motion of the Moon The Measurement of Distance Science.
Importance of SLR in the Determination of the ITRF Zuheir Altamimi IGN, France Geoscience Australia, Canberra, August 29, 2005 SLR Strength: its contribution.
Introduction to On-Orbit Thermal Environments
Lecture Notes on Astrometry Space Newtonian Viewpoint Spatial Coord. System = Reference Frame Inertial Reference Frame Spatial Coord. Transformation.
Celestial Mechanics III
Phases of the Moon Lab The Celestial Sphere Model One way the celestial sphere model is used explains positions in the sky as seen from YOUR position.
The Celestial Sphere (The sphere should really be rotating, not Earth)
Mission Analysis with STK
The Night Sky…last time, The Horizon System
The Appearance of the Night Sky
11.4 Rotations 1/12/17.
ASEN 5050 SPACEFLIGHT DYNAMICS Intro to STK, More 2-Body
What do the pictures represent?
4.3 Rotations Goals: Perform Rotations
Write a polar equation in r and {image} of a hyperbola with the focus at the origin, with the eccentricity 5 and directrix {image} . {image}
Orbit in Space Coordinate Frames and Time
Chapter 2 Motion in 1 Dimension.
Tilt of the Earth’s Rotational Axis
The Four Seasons.
The Sky (Celestial Sphere)
Hour 30 Euler’s Equations
Numerical evidence for the inconsistent separation
Physics 319 Classical Mechanics
Physics 319 Classical Mechanics
Presentation transcript:

3D representation of the Non-Rotating Origin Olivier de Viron and Veronique Dehant Royal Observatory of Belgium Scientific adviser: Nicole Capitaine

The Terrestrial Reference Frame

The Celestial Reference Frame

2 systems in an ideal world

The less ideal world

TRF CRF Intermediate RS 1. polar motion in Earth 2. Earth rotation 3. Celestial motion of CIP Only the intermediate system is different when using the new or the old formalism. The definition of the TRF and CRF are not affected.

The old-version transformation

1. From TRF to CIP

2. To the True equinox of the date

How to go from one equinox another? Equator 1 Ecliptic 1  Ecliptic 2  Equator 2 x Z y

How to go from one equinox another? Equator 1 Ecliptic 1  Ecliptic 2 ii Z rotation 1 (z) x y x y

How to go from one equinox another? Equator 1 Ecliptic 2 ii x Z y y Z Rotation 2 (x)

How to go from one equinox to another? Equator 1 Ecliptic 2 ii Z  y x Rotation 4 (z) x Equator 2

How to go from one equinox to another? Ecliptic 2 Z  x Equator 2 Z Rotation 5 (x)

How to go from one equinox another? Ecliptic 2  x Equator 2 It took 5 successive steps…

True equator of the date Mean equator of the date Equator at J2000 Mean ecliptic of the date True ecliptic of the date Ecliptic at J2000 vv 0

The new transformation

1. From TRF to CIP

2. From the terrestrial NRO

3. Earth Rotation Angle

4. To the X CRF projection: s

5. To CRF: celestial motion of the CIP

What is the NRO 2. Not a point in particular, any point of the CIP equator can work. 1. Characterized by its motion: no velocity around the CIP equator associated with polar motion or nutation. 3. Allows to get rid of the equinox in the change of reference frame.

So, we can take any points we want? 2. But, we want the new system to be consistent with the old one. 1. Yes, it is not the point it-self that matter, but its motion. 3. Thus, the point is chosen to insure continuity.

Conclusions The NRO is defined by its position at the base epoch (continuity) its motion (no motion in the CIP equator associated with polar motion). Only the Intermediate system is involved, no change of the CRF or TRF