Analysis of Orbit Stability in the Geosynchronous Region for End-Of-Life Disposal
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NTI Day 9 Astronomy Michael Feeback Go To: Teachastronomy
NTI Day 9 Astronomy Michael Feeback Go to: teachastronomy.com textbook (chapter layout) Chapter 3 The Copernican Revolution Orbits Read the article and answer the following questions. Orbits You can use Newton's laws to calculate the speed that an object must reach to go into a circular orbit around a planet. The answer depends only on the mass of the planet and the distance from the planet to the desired orbit. The more massive the planet, the faster the speed. The higher above the surface, the lower the speed. For Earth, at a height just above the atmosphere, the answer is 7.8 kilometers per second, or 17,500 mph, which is why it takes a big rocket to launch a satellite! This speed is the minimum needed to keep an object in space near Earth, and is called the circular velocity. An object with a lower velocity will fall back to the surface under Earth's gravity. The same idea applies to any object in orbit around a larger object. The circular velocity of the Moon around the Earth is 1 kilometer per second. The Earth orbits the Sun at an average circular velocity of 30 kilometers per second (the Earth's orbit is an ellipse, not a circle, but it's close enough to circular that this is a good approximation). At further distances from the Sun, planets have lower orbital velocities. Pluto only has an average circular velocity of about 5 kilometers per second. To launch a satellite, all you have to do is raise it above the Earth's atmosphere with a rocket and then accelerate it until it reaches a speed of 7.8 kilometers per second. -
Up, Up, and Away by James J
www.astrosociety.org/uitc No. 34 - Spring 1996 © 1996, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. Up, Up, and Away by James J. Secosky, Bloomfield Central School and George Musser, Astronomical Society of the Pacific Want to take a tour of space? Then just flip around the channels on cable TV. Weather Channel forecasts, CNN newscasts, ESPN sportscasts: They all depend on satellites in Earth orbit. Or call your friends on Mauritius, Madagascar, or Maui: A satellite will relay your voice. Worried about the ozone hole over Antarctica or mass graves in Bosnia? Orbital outposts are keeping watch. The challenge these days is finding something that doesn't involve satellites in one way or other. And satellites are just one perk of the Space Age. Farther afield, robotic space probes have examined all the planets except Pluto, leading to a revolution in the Earth sciences -- from studies of plate tectonics to models of global warming -- now that scientists can compare our world to its planetary siblings. Over 300 people from 26 countries have gone into space, including the 24 astronauts who went on or near the Moon. Who knows how many will go in the next hundred years? In short, space travel has become a part of our lives. But what goes on behind the scenes? It turns out that satellites and spaceships depend on some of the most basic concepts of physics. So space travel isn't just fun to think about; it is a firm grounding in many of the principles that govern our world and our universe. -
Multisatellite Determination of the Relativistic Electron Phase Space Density at Geosynchronous Orbit: Methodology and Results During Geomagnetically Quiet Times Y
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 110, A10210, doi:10.1029/2004JA010895, 2005 Multisatellite determination of the relativistic electron phase space density at geosynchronous orbit: Methodology and results during geomagnetically quiet times Y. Chen, R. H. W. Friedel, and G. D. Reeves Los Alamos National Laboratory, Los Alamos, New Mexico, USA T. G. Onsager NOAA, Boulder, Colorado, USA M. F. Thomsen Los Alamos National Laboratory, Los Alamos, New Mexico, USA Received 10 November 2004; revised 20 May 2005; accepted 8 July 2005; published 20 October 2005. [1] We develop and test a methodology to determine the relativistic electron phase space density distribution in the vicinity of geostationary orbit by making use of the pitch-angle resolved energetic electron data from three Los Alamos National Laboratory geosynchronous Synchronous Orbit Particle Analyzer instruments and magnetic field measurements from two GOES satellites. Owing to the Earth’s dipole tilt and drift shell splitting for different pitch angles, each satellite samples a different range of Roederer L* throughout its orbit. We use existing empirical magnetic field models and the measured pitch-angle resolved electron spectra to determine the phase space density as a function of the three adiabatic invariants at each spacecraft. Comparing all satellite measurements provides a determination of the global phase space density gradient over the range L* 6–7. We investigate the sensitivity of this method to the choice of the magnetic field model and the fidelity of the instrument intercalibration in order to both understand and mitigate possible error sources. Results for magnetically quiet periods show that the radial slopes of the density distribution at low energy are positive, while at high energy the slopes are negative, which confirms the results from some earlier studies of this type. -
Geosynchronous Orbit Determination Using Space Surveillance Network Observations and Improved Radiative Force Modeling
Geosynchronous Orbit Determination Using Space Surveillance Network Observations and Improved Radiative Force Modeling by Richard Harry Lyon B.S., Astronautical Engineering United States Air Force Academy, 2002 SUBMITTED TO THE DEPARTMENT OF AERONAUTICS AND ASTRONAUTICS IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN AERONAUTICS AND ASTRONAUTICS AT THE MASSACHUSETTS INSTITUTE OF TECHNOLOGY JUNE 2004 0 2004 Massachusetts Institute of Technology. All rights reserved. Signature of Author: Department of Aeronautics and Astronautics May 14, 2004 Certified by: Dr. Pa1 J. Cefola Technical Staff, the MIT Lincoln Laboratory Lecturer, Department of Aeronautics and Astronautics Thesis Supervisor Accepted by: Edward M. Greitzer H.N. Slater Professor of Aeronautics and Astronautics MASSACHUSETTS INS E OF TECHNOLOGY Chair, Committee on Graduate Students JUL 0 1 2004 AERO LBRARIES [This page intentionally left blank.] 2 Geosynchronous Orbit Determination Using Space Surveillance Network Observations and Improved Radiative Force Modeling by Richard Harry Lyon Submitted to the Department of Aeronautics and Astronautics on May 14, 2004 in Partial Fulfillment of the Requirements for the Degree of Master of Science in Aeronautics and Astronautics ABSTRACT Correct modeling of the space environment, including radiative forces, is an important aspect of space situational awareness for geostationary (GEO) spacecraft. Solar radiation pressure has traditionally been modeled using a rotationally-invariant sphere with uniform optical properties. This study is intended to improve orbit determination accuracy for 3-axis stabilized GEO spacecraft via an improved radiative force model. The macro-model approach, developed earlier at NASA GSFC for the Tracking and Data Relay Satellites (TDRSS), models the spacecraft area and reflectivity properties using an assembly of flat plates to represent the spacecraft components. -
Itu Recommendation Itu-R S.1003.2
SPACE DEBRIS MITIGATION STANDARDS ITU RECOMMENDATION ITU‐R S.1003.2 International mechanism: International Telecommunications Union (ITU) Recommendation ITU‐R S.1003.2 (12/2010) Environmental protection of the geostationary‐satellite orbit Description: ITU‐R S.1003.2 provides guidance about disposal orbits for satellites in the geostationary‐ satellite orbit (GSO). In this orbit, there is an increase in debris due to fragments resulting from increased numbers of satellites and their associated launches. Given the current limitations (primarily specific impulse) of space propulsion systems, it is impractical to retrieve objects from GSO altitudes or to return them to Earth at the end of their operational life. A protected region must therefore be established above, below and around the GSO which defines the nominal orbital regime within which operational satellites will reside and manoeuvre. To avoid an accumulation of non‐functional objects in this region, and the associated increase in population density and potential collision risk that this would lead to, satellites should be manoeuvred out of this region at the end of their operational life. In order to ensure that these objects do not present a collision hazard to satellites being injected into GSO, they should be manoeuvred to altitudes higher than the GSO region, rather than lower. The recommendations embodied in ITU‐R S.1003.2 are: – Recommendation 1: As little debris as possible should be released into the GSO region during the placement of a satellite in orbit. – Recommendation 2: Every reasonable effort should be made to shorten the lifetime of debris in elliptical transfer orbits with the apogees at or near GSO altitude. -
Recommendation Itu-R S.1003-2*
Recommendation ITU-R S.1003-2 (12/2010) Environmental protection of the geostationary-satellite orbit S Series Fixed-satellite service ii Rec. ITU-R S.1003-2 Foreword The role of the Radiocommunication Sector is to ensure the rational, equitable, efficient and economical use of the radio-frequency spectrum by all radiocommunication services, including satellite services, and carry out studies without limit of frequency range on the basis of which Recommendations are adopted. The regulatory and policy functions of the Radiocommunication Sector are performed by World and Regional Radiocommunication Conferences and Radiocommunication Assemblies supported by Study Groups. Policy on Intellectual Property Right (IPR) ITU-R policy on IPR is described in the Common Patent Policy for ITU-T/ITU-R/ISO/IEC referenced in Annex 1 of Resolution ITU-R 1. Forms to be used for the submission of patent statements and licensing declarations by patent holders are available from http://www.itu.int/ITU-R/go/patents/en where the Guidelines for Implementation of the Common Patent Policy for ITU-T/ITU-R/ISO/IEC and the ITU-R patent information database can also be found. Series of ITU-R Recommendations (Also available online at http://www.itu.int/publ/R-REC/en) Series Title BO Satellite delivery BR Recording for production, archival and play-out; film for television BS Broadcasting service (sound) BT Broadcasting service (television) F Fixed service M Mobile, radiodetermination, amateur and related satellite services P Radiowave propagation RA Radio astronomy RS Remote sensing systems S Fixed-satellite service SA Space applications and meteorology SF Frequency sharing and coordination between fixed-satellite and fixed service systems SM Spectrum management SNG Satellite news gathering TF Time signals and frequency standards emissions V Vocabulary and related subjects Note: This ITU-R Recommendation was approved in English under the procedure detailed in Resolution ITU-R 1. -
Analysis of Space Elevator Technology
Analysis of Space Elevator Technology SPRING 2014, ASEN 5053 FINAL PROJECT TYSON SPARKS Contents Figures .......................................................................................................................................................................... 1 Tables ............................................................................................................................................................................ 1 Analysis of Space Elevator Technology ........................................................................................................................ 2 Nomenclature ................................................................................................................................................................ 2 I. Introduction and Theory ....................................................................................................................................... 2 A. Modern Elevator Concept ................................................................................................................................. 2 B. Climber Concept ............................................................................................................................................... 3 C. Base Station Concept ........................................................................................................................................ 4 D. Space Elevator Astrodynamics ........................................................................................................................ -
Gateway Globe Lesson Plan: Understanding Orbits
Gateway Globe Lesson Plan: Understanding Orbits Location of Gateway Globe Gateway to Space Overview of Gateway Globe The Gateway Globe is a 36-inch wide spherical projection system which shows two different movies on it. One movie shows examples of parabolic flight paths of future space planes, and one shows examples of existing satellite orbits around the Earth. This lesson will allow students to learn how to describe the different kinds of satellite orbits. Lesson Background Information This lesson plan/unit could be used independently or to prepare for (or to extend the learning after) a visit to Spaceport America. It can be used by teachers or parents wishing to make the Spaceport visit a richer learning experience (for everyone!). An object that orbits the Earth is essentially falling around the Earth, but because of its horizontal velocity it never hits the ground. To understand this concept, you have to first understand a few of the basic laws of physics. You can do some simple experiments outdoors with your students that will help them grasp these basics. For both experiments, you will need two identical baseballs. Ask two students to throw the baseballs (forward) into the air while your other students watch. Then ask your class what they notice about the path of the balls. (The paths are curved.) This is because the force of the throw is causing the balls to go forward, but the force of gravity is also pulling the balls “down” toward the center of the Earth. This makes the paths curved. The faster they throw the ball, the farther it seems to go. -
Geosynchronous Satellite GF-4 Observations of Chlorophyll-A Distribution Details in the Bohai Sea, China
sensors Article Geosynchronous Satellite GF-4 Observations of Chlorophyll-a Distribution Details in the Bohai Sea, China Lina Cai 1, Juan Bu 1, Danling Tang 2,*, Minrui Zhou 1, Ru Yao 1 and Shuyi Huang 1 1 Marine Science and Technology College, Zhejiang Ocean University, Zhoushan 316004, China; [email protected] (L.C.); [email protected] (J.B.); [email protected] (M.Z.); [email protected] (R.Y.); [email protected] (S.H.) 2 Southern Marine Science and Engineering Guangdong Laboratory Guangdong Key Laboratory of Ocean Remote Sensing (LORS), South China Sea Institute of Oceanology, Chinese Academy of Sciences, Guangzhou 510301, China * Correspondence: [email protected] Received: 5 August 2020; Accepted: 21 September 2020; Published: 24 September 2020 Abstract: We analyzed the distribution of chlorophyll-a (Chla) in the Bohai Sea area based on data from the geosynchronous orbit optical satellite Gaofen-4 (GF-4), which was launched in 2015, carrying a panchromatic multispectral sensor (PMS). This is the first time the geosynchronous orbit optical satellite GF-4 remote-sensing data has been used in China to detect the Chla change details in the Bohai Sea. A new GF-4 retrieved model was established based on the relationship between in situ Chla value and the reflectance combination of 2 and 4 bands, with the R2 of 0.9685 and the total average relative error of 37.42%. Twenty PMS images obtained from 2017 to 2019 were applied to analyze Chla in Bohai sea. The results show that: (1) the new built Chla inversion model PMS-1 for the GF-4 PMS sensor can extract Chla distribution details in the Bohai Sea well. -
Rendezvous and Proximity Operations: Friend Or Foe?
Promoting Cooperative Solutions for Space Sustainability Rendezvous and Proximity Operations: Friend or Foe? Victoria Samson, Washington Office Director Secure World Foundation “Supporting Diplomacy: Clearing the Path for Dialogue” UNIDIR Geneva, Switzerland May 28-29, 2019 ©2019 Secure World Foundation. Used with Permission www.swfound.org UNIDIR May 29 ,2019 @SWFoundation Development of OOS and RPO Capabilities Promoting Cooperative Solutions for Space Sustainability • On-orbit servicing (OOS) and rendezvous and proximity operations (RPO) are key to enabling future of on-orbit activities • Benefits and challenges – Greatly increase the viability of and benefits from space activities – Raises a number of diplomatic, legal, safety, operational, and policy challenges that need to be tackled • OOS and RPO are not new, and are already international – 50+ years of experience in doing it with human spaceflight, but increasingly shifting to robotic/autonomous – Multiple countries/companies developing and testing RPO capabilities • How to develop norms and standards to enable cooperative OOS/RPO and mitigate challenges? UNIDIR May 29, 2019 2 www.swfound.org @SWFoundation RPO Activities and Counterspace Objectives Promoting Cooperative Solutions for Space Sustainability • Global Counterspace Capabilities: An Open Source Assessment, April 2019 – www.swfound.org/counterspace – Compiles and assesses publicly available information on the counterspace capabilities being developed by multiple countries across five categories: direct-ascent, co-orbital, -
Challenges for a South Texas Spaceport
Space Traffic Management Conference 2014 Roadmap to the Stars Nov 5th, 2:00 PM Challenges For A South Texas Spaceport Edward Ellegood Florida SpacerePort, [email protected] Wayne Eleazer Follow this and additional works at: https://commons.erau.edu/stm Ellegood, Edward and Eleazer, Wayne, "Challenges For A South Texas Spaceport" (2014). Space Traffic Management Conference. 17. https://commons.erau.edu/stm/2014/wednesday/17 This Event is brought to you for free and open access by the Conferences at Scholarly Commons. It has been accepted for inclusion in Space Traffic Management Conference by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. Safety Challenges for a South Texas Spaceport By Wayne Eleazer and Edward Ellegood, ERAU Space Traffic Management Conference, November 2014 Introduction On September 22, 2014, Space Exploration Technologies (SpaceX) broke ground on a new spaceport facility at Boca Chica, a remote beach located east of Brownsville, Texas, less than three miles north of the U.S./Mexico border. The groundbreaking followed the successful completion of an Environmental Impact Statement (EIS) in coordination with the Federal Aviation Administration’s Office of Commercial Space Transportation (FAA-AST), and the commitment of millions of dollars in financial assistance from Texas state and local governments. In addition to purely environmental/ecological impacts, the EIS focused on some other public safety risks, all of which were found to be acceptable with mitigating actions proposed by SpaceX. The EIS was an important step toward gaining community and state/local government support for the Boca Chica spaceport. The successful EIS triggered pledges of about $30 million in financial incentives that SpaceX plans to leverage to develop and operate the spaceport, a project expected to cost in excess of $100 million over several years. -
Geosynchronous Patrol Orbit for Space Situational Awareness
Geosynchronous patrol orbit for space situational awareness Blair Thompson, Thomas Kelecy, Thomas Kubancik Applied Defense Solutions Tim Flora, Michael Chylla, Debra Rose Sierra Nevada Corporation ABSTRACT Applying eccentricity to a geosynchronous orbit produces both longitudinal and radial motion when viewed in Earth-fixed coordinates. An interesting family of orbits emerges, useful for “neighborhood patrol” space situational awareness and other missions. The basic result is a periodic (daily), quasi- elliptical, closed path around a fixed region of the geosynchronous (geo) orbit belt, keeping a sensor spacecraft in relatively close vicinity to designated geo objects. The motion is similar, in some regards, to the relative motion that may be encountered during spacecraft proximity operations, but on a much larger scale. The patrol orbit does not occupy a fixed slot in the geo belt, and the east-west motion can be combined with north-south motion caused by orbital inclination, leading to even greater versatility. Some practical uses of the geo patrol orbit include space surveillance (including catalog maintenance), and general space situational awareness. The patrol orbit offers improved, diverse observation geom- etry for angles-only sensors, resulting in faster, more accurate orbit determination compared to simple inclined geo orbits. In this paper, we analyze the requirements for putting a spacecraft in a patrol orbit, the unique station keeping requirements to compensate for perturbations, repositioning the patrol orbit to a different location along the geo belt, maneuvering into, around, and out of the volume for proximity operations with objects within the volume, and safe end-of-life disposal requirements. 1. INTRODUCTION The traditional geosynchronous (“geosynch” or “geo”) orbit is designed to keep a spacecraft in a nearly fixed position (longitude, latitude, and altitude) with respect to the rotating Earth.