State Vector Reference Body Transformations Throughout The Solar System

Similar documents
Earth's Pseudo-Moon 2016 HO 3

Importance of the study of extrasolar planets. Exoplanets Introduction. Importance of the study of extrasolar planets

EPM the high-precision planetary ephemerides of IAA RAS for scientific research, astronavigation on the Earth and space

Apollo 15 Trans-Earth Trajectory Reconstruction

Astronomy Test Review. 3 rd Grade

Celestial Objects. Background Questions. 1. What was invented in the 17 th century? How did this help the study of our universe? 2. What is a probe?

Which of the following planets are all made up of gas? When a planets orbit around the Sun looks like an oval, it s called a(n)

Yes, inner planets tend to be and outer planets tend to be.

Proper initial conditions for long-term integrations of the solar system

Flight and Orbital Mechanics

LEARNING ABOUT THE OUTER PLANETS. NASA's Cassini spacecraft. Io Above Jupiter s Clouds on New Year's Day, Credit: NASA/JPL/University of Arizona

Earth Departure Trajectory Reconstruction of Apollo Program Components Undergoing Disposal in Interplanetary Space

Solar System. The Solar System. Nebular animation. Planets drawn to scale. Mercury. Mariner 10. Chapter 22 Pages

The escape speed for an object leaving the surface of any celestial body of mass M and radius d is

Comparative Planetology I: Our Solar System. Chapter Seven

The Solar System. Name Test Date Hour

Name Date Class. Earth in Space

Recent Developments in Planetary Ephemeris Observations. W. M. Folkner

The Solar System LEARNING TARGETS. Scientific Language. Name Test Date Hour

Astrodynamics (AERO0024)

Lecture Outlines. Chapter 6. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.

Celestial Mechanics I. Introduction Kepler s Laws

Astro 1: Introductory Astronomy

ASEN 5050 SPACEFLIGHT DYNAMICS Interplanetary

Assignment 1. Due Jan. 31, 2017

A Survey of the Planets Earth Mercury Moon Venus

Lecture 13. Gravity in the Solar System

Observational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws

What is it like? When did it form? How did it form. The Solar System. Fall, 2005 Astronomy 110 1

After you read this section, you should be able to answer these questions:

Chapter 29. The Solar System. The Solar System. Section 29.1 Models of the Solar System notes Models of the Solar System

CONTENTS. vii. in this web service Cambridge University Press. Preface Acknowledgements. xiii xvi

It Might Be a Planet If...

9J Gravity and Space ILU

ASTRONOMY. Chapter 7 OTHER WORLDS: AN INTRODUCTION TO THE SOLAR SYSTEM PowerPoint Image Slideshow

GRAIL Takes A Roundabout Route To Lunar Orbit

TEKS Cluster: Space. identify and compare the physical characteristics of the Sun, Earth, and Moon

Astrodynamics (AERO0024)

Part 4: Exploration 1

Rigorous Global Optimization of Impulsive Space Trajectories

Prentice Hall EARTH SCIENCE

Unit 12 Lesson 1 What Objects Are Part of the Solar System?

Planets: Name Distance from Sun Satellites Year Day Mercury 0.4AU yr 60 days Venus yr 243 days* Earth 1 1 yr 1 day Mars 1.

23.1 The Solar System. Orbits of the Planets. Planetary Data The Solar System. Scale of the Planets The Solar System

CHAPTER 6. The Solar System

Solar System Scales. PTYS/ASTR 206 The Golden Age of Planetary Exploration Shane Byrne

Chapter 4 The Solar System

Asteroids, Comets and NEOs. (Answers) Solar System Impacts. Author: Sarah Roberts

VLBA Astrometry of Planetary Orbiters

In so many and such important. ways, then, do the planets bear witness to the earth's mobility. Nicholas Copernicus

Physics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits. Planetary Motion

Question number Answer Notes Marks 1 correctly; (ii) Sun X should be left of the imaginary 5-7 line, reject X placed outside the orbit

Our Solar System. Lesson 5. Distances Between the Sun and the Planets

Patterns in the Solar System (Chapter 18)

Edmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006

astronomy A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.

6 The Orbit of Mercury

AST111, Lecture 1b. Measurements of bodies in the solar system (overview continued) Orbital elements

October 19, NOTES Solar System Data Table.notebook. Which page in the ESRT???? million km million. average.

Name Class Date. For each pair of terms, explain how the meanings of the terms differ.

Solar System. Sun, 8 planets, hundred moons, thousand.dwarf.planets million asteroids, billion comets etc.

1 The Solar System. 1.1 a journey into our galaxy

Early Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle

PHYS 160 Astronomy Test #1 Fall 2017 Version B

Welcome to the Solar System

Name: Pd Parent Signature of completion:

is a revolution relative to a fixed celestial position. is the instant of transit of mean equinox relative to a fixed meridian position.

AST Section 2: Test 1

Fundamentals of Satellite technology

SOLAR SYSTEM SCALE LAB

Interplanetary Mission Opportunities

Numerical analysis of the compliance of interplanetary CubeSats with planetary protection requirements

Comparative Planetology I: Our Solar System. Chapter Seven

Falcon Heavy's Maiden Launch Opens An Interplanetary Superhighway

Located Between The Orbits Of

Name Class Date. Chapter 29. The Solar System. Review Choose the best response. Write the letter of that choice in the space provided.

FUNDAMENTAL CONSTANTS FOR EPHEMERIS ASTRONOMY AND THE ORIENTATION OF PLANET EPHEMERIDES TO ICRF. Pitjeva E. V. Institute of Applied astronomy RAS

Our Solar System and Its Place in the Universe

Synodic and Relative Flower Constellations with Applications to Planetary Explorations

1 Solar System Debris and Formation

A Peek At Cassini After 7 Years In Saturn Orbit

Chapter 16 Astronomy Study Guide. VOCABULARY WORDS TO KNOW geocentric system meteorite meteoroid

Class Notes: Astronomy

The Jovian Planets. Why do we expect planets like this in the outer reaches of the solar system?(lc)

Contents of the Solar System

James L. Green Director, Planetary Science NASA

Assessment Vocabulary Instructional Strategies

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley

INPOP10a. A. Fienga, UTINAM/IMCCE

Interplanetary Mission Analysis

Topic 1: Celestial Objects, phenomena, and interactions are important to people in many different ways.

Gravity: Motivation An initial theory describing the nature of the gravitational force by Newton is a product of the resolution of the

INPOP06: the new European Planetary, Moon and Earth rotation Ephemeris

CVtpf 2-1. Section 1 Review. 3. Describe How did the process of outgassing help shape Earth's atmosphere?

The Formation of the Solar System

Mission Design Options for Solar-C Plan-A

Transneptunian objects. Minor bodies in the outer Solar System. Transneptunian objects

Phys 214. Planets and Life

Planetary Orbits: Kepler s Laws 1/18/07

Prentice Hall EARTH SCIENCE

Transcription:

Introduction One of the more mind-boggling programming challenges encountered during interplanetary trajectory design software development is how to transform a specified inertial position and velocity state vector for Body B with respect to Body A, denoted V A B, such that it is instead centered on Body C to become V C B. Note the transformation, expressed as V A B V C B, only changes the origin of the inertial coordinate system in which both state vectors are expressed. No rotations of this coordinate system are performed. Consequently, this transformation is equivalent to the Equation 1 state vector addition. V A B V C B = V A B + V C A (1) Transformations considered by this paper will be called Galilean because only the inertial coordinate system's origin is changed and Special/General Relativity is ignored. In many Galilean transformation definitions, a further condition is constant velocity between the two origins over time. This condition is not generally satisfied between bodies in the Solar System because they undergo differing inertial accelerations. To avoid this violation, any transformation considered herein is conducted with respect to a single specified epoch. Galilean transformations are of great utility to interplanetary trajectory design. For example, consider a spacecraft (S/C) departing Earth for interplanetary cruise. At some point with the S / spacecraft about a million km from Earth, a V C S / Earth V C Sun transformation would be performed. Perturbing Earth gravity accelerations on the spacecraft's subsequent heliocentric trajectory would then act in the direction of position components given by the transformation S / V C S / Sun V C Earth. In the context of V A B notation, and to underscore the vector nature of a state, this paper's narrative will refer to a subscripted body as the "tail" body and to a superscripted body as the "head" body. When using state vectors from the Horizons ephemeris server 1 or the Spacecraft Planet Instrument C-matrix Events (SPICE) information system 2, note that a head body is equivalent to the "target" body and a tail body is equivalent to the "observer" body. Galilean transformations in this paper comply with a trajectory design ephemeris operations concept developed by the author from experience working with Horizons ephemerides and SPICE software since the late 1990s. This concept imports text-based, short-term, typically single-use ephemerides from Horizons in which state vectors for spacecraft, asteroids, moons, comets, and other bodies of special interest are stored. Along with these imports, concurrent 1 This facility may be invoked using links and documentation available at https://ssd.jpl.nasa.gov/?horizons (accessed 16 August 2018). 2 Software and documentation for SPICE may be downloaded at https://naif.jpl.nasa.gov/naif/ (accessed 16 August 2018). Daniel R. Adamo 1

ephemerides for the Sun, Moon, planets, or Pluto can be created using SPICE software to access a Spacecraft and Planet Kernel (SPK) binary file spanning a relatively protracted time interval. 3 Method Under SPICE conventions 4, any body in the Solar System can be assigned an integer ID code. These conventions are summarized in Table 1. Note multiple Table 1 conventions are becoming saturated as the bodies they govern proliferate. Substantial revisions can be expected. Table 1. Integer ID code assignments for Solar System bodies according to SPICE conventions. SPICE ID Body 0 Solar System Barycenter (SSB) 1 through 9 Planetary system barycenters from Mercury through Neptune 5 10 Sun 199, 299,, 999 Planetary centers from Mercury through Neptune 6 n01, n02,, n98 Moons for systems n = 1 through 9-100,000 < ID < 0 Interplanetary spacecraft 7 ID < -100,000 Earth-orbiting spacecraft 8 1,000,000 < ID < 2,000,000 Comets 2,000,000 < ID < 50,000,000 Asteroids 9 50,000,000 < ID < 50,000,024 Comet Shoemaker-Levy 9 fragments When accessed by SPICE utility application BRIEF, the SPK file pertinent to this paper's Galilean transformations generates output reproduced in Table 2. In the Bodies section of this output, a head body SPICE ID (headid) is followed by "w.r.t." and the corresponding tail body SPICE ID (tailid) for a set of state vector interpolation data. With SPICE software, each dataset generates valid state vectors for the corresponding headid/tailid from epoch 1950.0 to epoch 2100.0 in barycentric dynamical time (TDB). 3 These text-based Horizons imports could be replaced with dedicated SPK binary files optionally concatenated into other such files. But some small bodies are transient in nature. Furthermore, a newly discovered small body is associated with rapidly evolving uncertainty in predicted position as additional observations are accumulated. Consequently, text-based ephemeris imports are the adopted alternative due to their straightforward reconfiguration and traceability. 4 Reference the SPICE Toolkit download's doc/naif_ids.req text file. The toolkit may be downloaded at https://naif.jpl.nasa.gov/naif/toolkit.html (accessed 24 August 2018). 5 The SPICE ID 9 is assigned to the Pluto system's barycenter. 6 The SPICE ID 999 is assigned to the center of Pluto. 7 An interplanetary spacecraft's SPICE ID is typically the negative of its assigned Deep Space Network ID. 8 An Earth-orbiting spacecraft's SPICE ID is -100,000 minus its assigned NORAD ID. International Space Station has SPICE ID -125,544. 9 An asteroid's SPICE ID is 2,000,000 plus its JPL catalog number. The asteroid (1) Ceres has SPICE ID 2,000,001. Daniel R. Adamo 2

Table 2. Contents of the SPK file supporting this paper's ephemeris operations concept are summarized by output from the SPICE utility application BRIEF. BRIEF -- Version 4.0.0, September 8, 2010 -- Toolkit Version N0066 Summary for: DE431_PLNCNT_1950-2100.bsp Bodies: MERCURY BARYCENTER (1) w.r.t. SOLAR SYSTEM BARYCENTER (0) VENUS BARYCENTER (2) w.r.t. SOLAR SYSTEM BARYCENTER (0) EARTH BARYCENTER (3) w.r.t. SOLAR SYSTEM BARYCENTER (0) MARS BARYCENTER (4) w.r.t. SOLAR SYSTEM BARYCENTER (0) JUPITER BARYCENTER (5) w.r.t. SOLAR SYSTEM BARYCENTER (0) SATURN BARYCENTER (6) w.r.t. SOLAR SYSTEM BARYCENTER (0) URANUS BARYCENTER (7) w.r.t. SOLAR SYSTEM BARYCENTER (0) NEPTUNE BARYCENTER (8) w.r.t. SOLAR SYSTEM BARYCENTER (0) PLUTO BARYCENTER (9) w.r.t. SOLAR SYSTEM BARYCENTER (0) SUN (10) w.r.t. SOLAR SYSTEM BARYCENTER (0) MERCURY (199) w.r.t. MERCURY BARYCENTER (1) VENUS (299) w.r.t. VENUS BARYCENTER (2) MOON (301) w.r.t. EARTH BARYCENTER (3) EARTH (399) w.r.t. EARTH BARYCENTER (3) MARS (499) w.r.t. MARS BARYCENTER (4) JUPITER (599) w.r.t. JUPITER BARYCENTER (5) SATURN (699) w.r.t. SATURN BARYCENTER (6) URANUS (799) w.r.t. URANUS BARYCENTER (7) NEPTUNE (899) w.r.t. NEPTUNE BARYCENTER (8) PLUTO (999) w.r.t. PLUTO BARYCENTER (9) Start of Interval (ET) End of Interval (ET) ----------------------------- ----------------------------- 1950 JAN 01 00:00:00.000 2100 JAN 01 00:00:00.000 The Table 2 SPK data serve as the "trunk" and main "branches" in a tree-like topology encompassing core Galilean transformations throughout the Solar System. Branches supplementing the SPK file's tree can be added by importing a Horizons ephemeris such that the imported tailid is zero (the SSB) or one of the file's headid values. Additional imports can further extend the tree, provided each has a tailid matching a headid somewhere in the tree. Cumulative applications of Equation 1 are used to reconstruct state vector branches in the tree, ultimately computing SSB-centered state vectors with tailid = 0. A portion of the SPK-resident tree described in Table 2 is illustrated in Figure 1 with each green arrow representing a state vector. The orange arrow denotes a state vector stored in an imported Moon-centered Lunar Reconnaissance Orbiter (LRO) ephemeris "grafted" onto the tree. Daniel R. Adamo 3

LRO Spacecraft ID = -85 Moon ID = 301 "85 V 301 Jupiter ID = 599 Earth Barycenter ID = 3 V 3 301 Sun ID = 10 V 5 599 Jupiter Barycenter ID = 5 V 0 3 V 0 10 V 0 5 Solar System Barycenter ID = 0 Figure 1. A tree-like topology, relating the Solar System's components through Galilean transformations of state vectors (green arrows), is illustrated for some SPICE IDs in Table 2. The LRO spacecraft has been grafted onto this tree (orange dot) by importing its Mooncentered ephemeris from Horizons. 10 Note this diagram is completely relational in nature and not to scale. When tasked to produce a state vector V B A, the standard strategy is to iteratively apply Equation 1 to the initial Body A state vector until its tailid = 0. While thus reconstructing the branch for Body A's headid in the transformation tree, a tailid corresponding to Body B may be encountered serendipitously. If so, the task is complete. In other less fortuitous cases, Body B in a V B A state vector computation lies on a different "secondary" transformation tree branch from the "primary" branch occupied by Body A. In those instances, reconstruction first produces a primary state vector P 0 A for Body A with respect to the SSB. An independent branch reconstruction then produces a secondary SSB-centered state vector S 0 B for Body B whose headid is the desired tailid for Body A's state vector. The specified state vector is then computed with Equation 2. V B A = P 0 A - S 0 B (2) For instance, consider a task to compute solar illumination on the outer martian moon Deimos (SPICE ID = 402). Completion of this task requires an illumination vector equivalent to the position components of V 10 402. The only imported ephemeris required to produce V 10 402 is one for 10 This diagram is patterned after a similar example of bodies pertinent to the Galileo spacecraft's mission in the SPICE Toolkit download's doc/spk.req text file. The toolkit may be downloaded at https://naif.jpl.nasa.gov/naif/toolkit.html (accessed 24 August 2018). Daniel R. Adamo 4

Deimos centered on Mars covering the TDB epoch of interest. Applying Equation 1 to the primary transformation branch occupied by Deimos produces the sequence P 402 499 P 402 402 4 P 0 (per Table 2, tailids 499 = Mars and 4 = Mars barycenter). The secondary branch immediately contributes S 10 0 without any transformations. Equation 2 then produces the desired state with V 402 10 = P 402 0 - S 10 0. Essential to Galilean transformations between ephemerides is an accurate interpolator using TDB epoch as its argument. A 6-point Lagrange interpolator, as documented by Meeus 11, is employed to produce results documented in the following section. Numeric Example As illustrated by Figure 1, an object deeply embedded in the Solar System's Galilean transformation tree is the LRO spacecraft with SPICE ID = -85. As of this writing, stable asflown trajectory data for LRO are available on Horizons from shortly after its launch on 18 June 2009 through its lunar orbit insertion 4 days later until 15 March 2018. This example first obtains a Jupiter-centered LRO state vector V 85 599 on 28 February 2018 at 12:00:00 TDB in the Earth mean equator and equinox of epoch J2000.0 coordinate system (J2K). The result, which requires no Lagrange interpolation, is compared with a similar computation by Horizons. A second J2K V 85 599 state vector is produced 0.0083 d later than the first on 28 February 2018 at 12:11:57.120 TDB such that Lagrange interpolation is required. When compared with synchronized Horizons data, this later state vector demonstrates the degree of precision degradation arising from 6-point Lagrange interpolation. Note both V 85 599 state vectors are geometric in that they do not incorporate the effects of planetary aberration or stellar aberration. 12 This task requires an LRO ephemeris be imported from Horizons. Circa late February 2018, Horizons indicates LRO's Moon-centered trajectory has a low eccentricity near 0.002 and a period near 117 min. The 6-point Lagrange interpolator is reasonably accurate when operating with 15 state vectors in a single nearly circular orbit's period, suggesting the imported ephemeris have 8 min between consecutive epochs. Starting the imported ephemeris at 11:36 TDB and ending it at 12:48 TDB provides adequate access to P 85 301 states initiating primary branch reconstructions. To achieve maximum interpolation accuracy, it is essential the 12:11:57.120 TDB epoch lie between epochs 3 and 4 in the 6-state Lagrange interpolation table. Imported ephemeris sequencing is summarized in Table 3. 11 Reference J. Meeus, Astronomical Algorithms, Willmann-Bell, Inc., 1991, pp. 32-33. 12 Planetary aberration shifts the geometric state vector of the head body as seen from the tail body according to the finite speed of light. Stellar aberration contributes another shift to this state vector according to the tail body's SSBcentered velocity. These shifts produce the apparent state vector of the head body as seen from the tail body. Both aberration shifts can be computed using Galilean transformations as documented herein. Reference the SPICE Toolkit download's doc/abcorr.req text file. The toolkit may be downloaded at https://naif.jpl.nasa.gov/naif/toolkit.html (accessed 24 August 2018). Daniel R. Adamo 5

Table 3. A chronology of Moon-centered state vectors appearing in the imported LRO ephemeris follows. These are supplemented with a state vector inferred from 6 of them using a Lagrange interpolator. 28 Feb 2018 Ephemeris Lagrange Table TDB Epoch State Index State Index Comment 11:36:00 1 11:44:00 2 11:52:00 3 1 12:00:00 4 2 85 No-Lagrange P 301 12:08:00 5 3 12:11:57.120 85 Lagrange-interpolated P 301 12:16:00 6 4 12:24:00 7 5 12:32:00 8 6 12:40:00 9 12:48:00 10 Deviations between this paper's methodology and Horizons arising in corresponding J2K V 85 599 position and velocity vectors are quantified by three parameters. The first of these is ΔRSS, the deviation's vector difference magnitude. Angular deviation between the two vectors is quantified by the Δθ parameter. Finally, Δr is the deviation's signed radial component in the sense "this paper minus Horizons". Results appear in Table 4. Table 4. Deviations between Jupiter-centered LRO state vectors as computed by this paper's methodology and by Horizons are summarized with three parameters defined in the foregoing narrative. 28 Feb 2018 Vector ΔRSS TDB Epoch Components (m or m/s) Δθ (deg) Δr (m or m/s) 12:00:00 Position 0.065 0.000000854-0.006437302 Velocity 0.000058 0-0.000030287 12:11:57.120 Position 802.432 0.000001479 +476.613 Velocity 0.089765 0.000159596 +0.040021172 Conclusion An ephemeris operations concept, together with Galilean transformations and associated logic, have been documented with which to relate the position and velocity of any object in the Solar System to any other object therein. Although to some degree limited by ephemeris interpolation accuracy, this capability has been shown to be in close agreement with JPL's Horizons ephemeris server. Daniel R. Adamo 6