RS platforms. Fabio Dell Acqua - Gruppo di Telerilevamento
|
|
|
- Shauna James
- 10 years ago
- Views:
Transcription
1 RS platforms
2 Platform vs. instrument Sensor Platform Instrument The remote sensor can be ideally represented as an instrument carried by a platform
3 Platforms Remote Sensing: Ground-based air-borne space-borne Different characteristics and cost structures
4 Ground based RS Platform is bound to the Earth surface Ex.: radar, weather radar, GPR, GB-SAR, hand-held spectrometers
5 airborne RS Flying platform: airplane, UAV, helicopter, kite, balloon... elevation: 100 m 30/40 km e.g. airborne radar
6 Airplane Usually modified to fit the RS instruments cruise speed between 140 and 600 km/h, often connected with the specific acquisition height from hundreds to thousand of m, connected with the specific acquisition wind bias, limited pilot correction GPS + IMU (=Inertial Measurement Units) for a-posteriori correction high costs (both maintenance and missions), ad-hoc acquisitions mission cost: tens of k s
7 Spaceborne RS mostly artificial satellites but also spacecrafts (e.g. Space Shuttle, for SRTM mission) km elevation periodic acquisition high design, production and launch costs low per-datum cost
8 spaceborne RS: two segments Space segment acquisition storage (temporary) downlink Ground segment mission control data reception correction processing
9 What is a satellite? a celestial body revolving around another body artificial satellites Earth Observation satellites
10 Structure of an EO satellite Complex, depending on addressed application Two main sections: - payload and - bus
11 Details
12 Communication systems up- and down-link. Command and control, downlink of RS data
13 Sensors Earth Observation sensors and related devices (e.g. temporary storage)
14 Navigation systems Exact determination of satellite location and attitude Some (limited) capabilities for adjustments
15 Power Normally supplied by sunrays through solar panels Excess energy stored in batteries (about ½ orbit)
16 Structure and envelope Mechanically keeps the entire device together, ensuring also thermal and radiation protection. Controlled dispersion of heat
17 Orbit Repetitive path of a satellite around the Earth, due to the equilibrium between weight and centrifugal force (due to its motion) Gravity force is inversely proportional to the squared distance from Earth, while the centrifugal force is proportional to tangential velocity orbits at higher elevation slower revolution
18 Circular orbit In a simplifying hypothesis of circular orbit and mass negligible wrt Earth, radius r and period T comply with: T 2 GM = 4π 2 r 3 where M=mass of the Earth, G= gravity constant The period can thus be computed as: T = 2π r 3 GM
19 Features of an orbit Height: distance between the satellite and the average Earth surface km or km (GEO) Inclination: angle between the equator and the orbit plane Period: time required to complete an orbit (tens of minutes, at the usual speeds of 7-8 km/s) Revisit time: time between two passages above the same point on the order of days or tens of days
20 RS orbits heliosyncronous orbits Low Earth Quasi-polar Orbits (LEO) orbits Geostationary Earth Orbit (GEO)
21 RS orbits Quasi-polar: next to the polar axis. Most common km LEO: km. Used for high resolution and short revisit times Sun-synchronous: to minimize sun bias and to ensure proper operation of solar panels GEO: km. Revolution=Earth rotation. The satellite appears idling on the equatorial plane. Weather satellites.
22 Nadir Nadir direction: towards the Earth centre Nadir point: intersection between the Earth surface and the line joining the sensor and the Earth centre
23 Swath the Earth surface strip as sensed by an EO satellite, and the width of the strip itself
24 Downlink RS satellites have limited onboard storage capabilities data is usually directed downlinked to the ground station in some cases a second satellite can provide support to link with non-visible stations
2. Orbits. FER-Zagreb, Satellite communication systems 2011/12
2. Orbits Topics Orbit types Kepler and Newton laws Coverage area Influence of Earth 1 Orbit types According to inclination angle Equatorial Polar Inclinational orbit According to shape Circular orbit
Hyperspectral Satellite Imaging Planning a Mission
Hyperspectral Satellite Imaging Planning a Mission Victor Gardner University of Maryland 2007 AIAA Region 1 Mid-Atlantic Student Conference National Institute of Aerospace, Langley, VA Outline Objective
Mobile Communications: Satellite Systems
Mobile Communications: Satellite Systems Mobile Communication: Satellite Systems - Jochen Schiller http://www.jochenschiller.de 1 History of satellite communication 1945 Arthur C. Clarke publishes an essay
Orbital Mechanics and Space Geometry
Orbital Mechanics and Space Geometry AERO4701 Space Engineering 3 Week 2 Overview First Hour Co-ordinate Systems and Frames of Reference (Review) Kepler s equations, Orbital Elements Second Hour Orbit
Section 4: The Basics of Satellite Orbits
Section 4: The Basics of Satellite Orbits MOTION IN SPACE VS. MOTION IN THE ATMOSPHERE The motion of objects in the atmosphere differs in three important ways from the motion of objects in space. First,
Examination Space Missions and Applications I (AE2103) Faculty of Aerospace Engineering Delft University of Technology SAMPLE EXAM
Examination Space Missions and Applications I AE2103 Faculty of Aerospace Engineering Delft University of Technology SAMPLE EXAM Please read these instructions first: This are a series of multiple-choice
Satellite technology
Satellite technology Overview What is a satellite? The key elements of orbital position Satellite manufacturers and design The components of a satellite: payload and bus Digital versus analogue How do
Penn State University Physics 211 ORBITAL MECHANICS 1
ORBITAL MECHANICS 1 PURPOSE The purpose of this laboratory project is to calculate, verify and then simulate various satellite orbit scenarios for an artificial satellite orbiting the earth. First, there
Newton s Law of Gravity
Gravitational Potential Energy On Earth, depends on: object s mass (m) strength of gravity (g) distance object could potentially fall Gravitational Potential Energy In space, an object or gas cloud has
5. Satellite Systems. History of Satellite Communications
5. Satellite Systems History and Orbits Routing, Localization, and Hand-over Systems 2005 Burkhard Stiller and Jochen Schiller FU Berlin M5 1 History of Satellite Communications 1945 Arthur C. Clarke about
KINEMATICS OF PARTICLES RELATIVE MOTION WITH RESPECT TO TRANSLATING AXES
KINEMTICS OF PRTICLES RELTIVE MOTION WITH RESPECT TO TRNSLTING XES In the previous articles, we have described particle motion using coordinates with respect to fixed reference axes. The displacements,
Chapter 2. Mission Analysis. 2.1 Mission Geometry
Chapter 2 Mission Analysis As noted in Chapter 1, orbital and attitude dynamics must be considered as coupled. That is to say, the orbital motion of a spacecraft affects the attitude motion, and the attitude
Orbital Mechanics. Angular Momentum
Orbital Mechanics The objects that orbit earth have only a few forces acting on them, the largest being the gravitational pull from the earth. The trajectories that satellites or rockets follow are largely
Automated Spacecraft Scheduling The ASTER Example
Automated Spacecraft Scheduling The ASTER Example Ron Cohen [email protected] Ground System Architectures Workshop 2002 Jet Propulsion Laboratory The Concept Scheduling by software instead of
Mobile Communications Chapter 5: Satellite Systems
Mobile Communications Chapter 5: Satellite Systems History Basics Localization Handover Routing Systems History of satellite communication 1945 Arthur C. Clarke publishes an essay about Extra Terrestrial
Supplemental Questions
Supplemental Questions The fastest of all fishes is the sailfish. If a sailfish accelerates at a rate of 14 (km/hr)/sec [fwd] for 4.7 s from its initial velocity of 42 km/h [fwd], what is its final velocity?
Artificial Satellites Earth & Sky
Artificial Satellites Earth & Sky Name: Introduction In this lab, you will have the opportunity to find out when satellites may be visible from the RPI campus, and if any are visible during the activity,
Günter Seeber. Satellite Geodesy 2nd completely revised and extended edition
Günter Seeber Satellite Geodesy 2nd completely revised and extended edition Walter de Gruyter Berlin New York 2003 Contents Preface Abbreviations vii xvii 1 Introduction 1 1.1 Subject of Satellite Geodesy...
Mobile Computing. Chapter 5: Satellite Systems
Mobile Computing Chapter 5: Satellite Systems Prof. Sang-Jo Yoo History of satellite communication 1945 Arthur C. Clarke publishes an essay about Extra Terrestrial Relays 1957 First satellite SPUTNIK by
Section 2. Satellite Orbits
Section 2. Satellite Orbits References Kidder and Vonder Haar: chapter 2 Stephens: chapter 1, pp. 25-30 Rees: chapter 9, pp. 174-192 In order to understand satellites and the remote sounding data obtained
Satellite Communications
Satellite Communications Department of Electrical Engineering Faculty of Engineering Chiangmai University Origin of Satellite Communications Arthur C. Clark (1945) British Science fiction writer propose
Satellites and Space Stations
Satellites and Space Stations A satellite is an object or a body that revolves around another object, which is usually much larger in mass. Natural satellites include the planets, which revolve around
Physics 2A, Sec B00: Mechanics -- Winter 2011 Instructor: B. Grinstein Final Exam
Physics 2A, Sec B00: Mechanics -- Winter 2011 Instructor: B. Grinstein Final Exam INSTRUCTIONS: Use a pencil #2 to fill your scantron. Write your code number and bubble it in under "EXAM NUMBER;" an entry
Bi-Directional DGPS for Range Safety Applications
Bi-Directional DGPS for Range Safety Applications Ranjeet Shetty 234-A, Avionics Engineering Center, Russ College of Engineering and Technology, Ohio University Advisor: Dr. Chris Bartone Outline Background
Niraj Sir GRAVITATION CONCEPTS. Kepler's law of planetry motion
GRAVITATION CONCEPTS Kepler's law of planetry motion (a) Kepler's first law (law of orbit): Every planet revolves around the sun in an elliptical orbit with the sun is situated at one focus of the ellipse.
The RapidEye optical satellite family for high resolution imagery
'Photogrammetric Week 01' D. Fritsch & R. Spiller, Eds. Wichmann Verlag, Heidelberg 2001. Scherer, Krischke 139 The RapidEye optical satellite family for high resolution imagery STEFAN SCHERER and MANFRED
How To Monitor Sea Level With Satellite Radar
Satellite Altimetry Wolfgang Bosch Deutsches Geodätisches Forschungsinstitut (DGFI), München email: [email protected] Objectives You shall recognize satellite altimetry as an operational remote sensing
DIRECT ORBITAL DYNAMICS: USING INDEPENDENT ORBITAL TERMS TO TREAT BODIES AS ORBITING EACH OTHER DIRECTLY WHILE IN MOTION
1 DIRECT ORBITAL DYNAMICS: USING INDEPENDENT ORBITAL TERMS TO TREAT BODIES AS ORBITING EACH OTHER DIRECTLY WHILE IN MOTION Daniel S. Orton email: [email protected] Abstract: There are many longstanding
Flight and Orbital Mechanics
Flight and Orbital Mechanics Lecture slides Challenge the future 1 Material for exam: this presentation (i.e., no material from text book). Sun-synchronous orbit: used for a variety of earth-observing
Solar System. 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X?
Solar System 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X? A) Earth B) Sun C) Moon D) Polaris 2. Which object orbits Earth in both the Earth-centered
Dynamics of Iain M. Banks Orbitals. Richard Kennaway. 12 October 2005
Dynamics of Iain M. Banks Orbitals Richard Kennaway 12 October 2005 Note This is a draft in progress, and as such may contain errors. Please do not cite this without permission. 1 The problem An Orbital
Use the following information to deduce that the gravitational field strength at the surface of the Earth is approximately 10 N kg 1.
IB PHYSICS: Gravitational Forces Review 1. This question is about gravitation and ocean tides. (b) State Newton s law of universal gravitation. Use the following information to deduce that the gravitational
Earth in the Solar System
Copyright 2011 Study Island - All rights reserved. Directions: Challenge yourself! Print out the quiz or get a pen/pencil and paper and record your answers to the questions below. Check your answers with
Angular Velocity vs. Linear Velocity
MATH 7 Angular Velocity vs. Linear Velocity Dr. Neal, WKU Given an object with a fixed speed that is moving in a circle with a fixed ius, we can define the angular velocity of the object. That is, we can
Can Hubble be Moved to the International Space Station? 1
Can Hubble be Moved to the International Space Station? 1 On January 16, NASA Administrator Sean O Keefe informed scientists and engineers at the Goddard Space Flight Center (GSFC) that plans to service
Chapter 5 Using Newton s Laws: Friction, Circular Motion, Drag Forces. Copyright 2009 Pearson Education, Inc.
Chapter 5 Using Newton s Laws: Friction, Circular Motion, Drag Forces Units of Chapter 5 Applications of Newton s Laws Involving Friction Uniform Circular Motion Kinematics Dynamics of Uniform Circular
Lecture L17 - Orbit Transfers and Interplanetary Trajectories
S. Widnall, J. Peraire 16.07 Dynamics Fall 008 Version.0 Lecture L17 - Orbit Transfers and Interplanetary Trajectories In this lecture, we will consider how to transfer from one orbit, to another or to
Lecture 13. Gravity in the Solar System
Lecture 13 Gravity in the Solar System Guiding Questions 1. How was the heliocentric model established? What are monumental steps in the history of the heliocentric model? 2. How do Kepler s three laws
PHY121 #8 Midterm I 3.06.2013
PHY11 #8 Midterm I 3.06.013 AP Physics- Newton s Laws AP Exam Multiple Choice Questions #1 #4 1. When the frictionless system shown above is accelerated by an applied force of magnitude F, the tension
16 th IOCCG Committee annual meeting. Plymouth, UK 15 17 February 2011. mission: Present status and near future
16 th IOCCG Committee annual meeting Plymouth, UK 15 17 February 2011 The Meteor 3M Mt satellite mission: Present status and near future plans MISSION AIMS Satellites of the series METEOR M M are purposed
Satellite Communication Systems. mgr inż. Krzysztof Włostowski Instytut Telekomunikacji PW [email protected]
Satellite Communication Systems mgr inż. Krzysztof Włostowski Instytut Telekomunikacji PW [email protected] Satellite Communication Satellite Communication combines the missile and microwave technologies
Mobile Communications Chapter 5: Satellite Systems
History of satellite communication Mobile Communications Chapter 5: Satellite Systems History Basics Orbits LEO, MEO, GEO Examples Handover, Routing 1945 Arthur C. Clarke publishes an essay about Extra
Understanding Orbital Mechanics Through a Step-by-Step Examination of the Space-Based Infrared System (SBIRS)
Understanding Orbital Mechanics Through a Step-by-Step Examination of the Space-Based Infrared System (SBIRS) Denny Sissom Elmco, Inc. May 2003 Pg 1 of 27 SSMD-1102-366 [1] The Ground-Based Midcourse Defense
C-S TEAM. Page 1 of 5
Title: Medium/large vehicle tracking system Primary POC: Jacoba Auret Organization: C-S Team (Cape Peninsula University of Technology-Stellenbosch University) POC email: [email protected] Need We exist
Halliday, Resnick & Walker Chapter 13. Gravitation. Physics 1A PHYS1121 Professor Michael Burton
Halliday, Resnick & Walker Chapter 13 Gravitation Physics 1A PHYS1121 Professor Michael Burton II_A2: Planetary Orbits in the Solar System + Galaxy Interactions (You Tube) 21 seconds 13-1 Newton's Law
Solar System Fundamentals. What is a Planet? Planetary orbits Planetary temperatures Planetary Atmospheres Origin of the Solar System
Solar System Fundamentals What is a Planet? Planetary orbits Planetary temperatures Planetary Atmospheres Origin of the Solar System Properties of Planets What is a planet? Defined finally in August 2006!
circular motion & gravitation physics 111N
circular motion & gravitation physics 111N uniform circular motion an object moving around a circle at a constant rate must have an acceleration always perpendicular to the velocity (else the speed would
Name Class Period. F = G m 1 m 2 d 2. G =6.67 x 10-11 Nm 2 /kg 2
Gravitational Forces 13.1 Newton s Law of Universal Gravity Newton discovered that gravity is universal. Everything pulls on everything else in the universe in a way that involves only mass and distance.
Remote Sensing Satellite Information Sheets Geophysical Institute University of Alaska Fairbanks
Remote Sensing Satellite Information Sheets Geophysical Institute University of Alaska Fairbanks ASTER Advanced Spaceborne Thermal Emission and Reflection Radiometer AVHRR Advanced Very High Resolution
Astrodynamics (AERO0024)
Astrodynamics (AERO0024) 6. Interplanetary Trajectories Gaëtan Kerschen Space Structures & Systems Lab (S3L) Course Outline THEMATIC UNIT 1: ORBITAL DYNAMICS Lecture 02: The Two-Body Problem Lecture 03:
DSL Mission Concept at Lunar Orbit
DSL Mission Concept at Lunar Orbit Jingye Yan Na9onal Space Science Center (NSSC) Chinese Academy of Sciences (CAS) 2015-02- 02, ASTRON, The Netherland 1 Payload onboard single nano- sat Element antenna
The National Strategy, Current Activities for Space Technology Development and Application
14-18 November 2011, Putrajaya, Malaysia The National Strategy, Current Activities for Space Technology Development and Application Lai Anh Khoi Space Technology Institute, VAST, Vietnam Bief History Space
Elements of Physics Motion, Force, and Gravity Teacher s Guide
Teacher s Guide Grade Level: 9 12 Curriculum Focus: Physical Science Lesson Duration: Three class periods Program Description Examine Isaac Newton's laws of motion, the four fundamental forces of the universe,
Basic Principles of Inertial Navigation. Seminar on inertial navigation systems Tampere University of Technology
Basic Principles of Inertial Navigation Seminar on inertial navigation systems Tampere University of Technology 1 The five basic forms of navigation Pilotage, which essentially relies on recognizing landmarks
1-2. What is the name given to the path of the Sun as seen from Earth? a.) Equinox b.) Celestial equator c.) Solstice d.
Chapter 1 1-1. How long does it take the Earth to orbit the Sun? a.) one sidereal day b.) one month c.) one year X d.) one hour 1-2. What is the name given to the path of the Sun as seen from Earth? a.)
F N A) 330 N 0.31 B) 310 N 0.33 C) 250 N 0.27 D) 290 N 0.30 E) 370 N 0.26
Physics 23 Exam 2 Spring 2010 Dr. Alward Page 1 1. A 250-N force is directed horizontally as shown to push a 29-kg box up an inclined plane at a constant speed. Determine the magnitude of the normal force,
Mobile Communications Exercise: Satellite Systems and Wireless LANs. Georg von Zengen, IBR, TU Braunschweig, www.ibr.cs.tu-bs.de
Mobile Communications Exercise: Satellite Systems and Wireless LANs N 1 Please define the terms inclination and elevation using the following two figures. How do these parameters influence the usefulness
Aerospace Information Technology Topics for Internships and Bachelor s and Master s Theses
Aerospace Information Technology s for Internships and Bachelor s and Master s Theses Version Nov. 2014 The Chair of Aerospace Information Technology addresses several research topics in the area of: Avionic
Educator Guide to S LAR SYSTEM. 1875 El Prado, San Diego CA 92101 (619) 238-1233 www.rhfleet.org
Educator Guide to S LAR SYSTEM 1875 El Prado, San Diego CA 92101 (619) 238-1233 www.rhfleet.org Pre-Visit Activity: Orbital Paths Materials: Plastic Plate Marble Scissors To Do: 1. Put the plate on a flat
Introduction to satellite constellations orbital types, uses and related facts
Introduction to satellite constellations orbital types, uses and related facts Dr Lloyd Wood space team, Cisco Systems http://www.cisco.com/go/space Guest lecture, ISU summer session July 2006 created
Sentinel-1 Mission Overview
Sentinel-1 Mission Overview Pierre Potin Sentinel-1 Mission Manager, ESA Advanced Course on Radar Polarimetry ESRIN, Frascati, 19 January 2011 Global Monitoring for Environment and Security GMES is established
CONSTRUCTING A CONSTELLATION OF 6U SOLAR POWER CUBE SATELLITES
CONSTRUCTING A CONSTELLATION OF 6U SOLAR POWER CUBE SATELLITES Authors: Corey Bergsrud 1, Jeremy Straub 2, Matthew Clausing 3, Johnathan McClure 1, and Sima Noghanian 1. 1 Department of Electrical Engineering,
DIN Department of Industrial Engineering School of Engineering and Architecture
DIN Department of Industrial Engineering School of Engineering and Architecture Elective Courses of the Master s Degree in Aerospace Engineering (MAE) Forlì, 08 Nov 2013 Master in Aerospace Engineering
DEOS. Deutsche Orbitale Servicing Mission. The In-flight Technology Demonstration of Germany s Robotics Approach to Service Satellites
DEOS Deutsche Orbitale Servicing Mission The In-flight Technology Demonstration of Germany s Robotics Approach to Service Satellites B. Sommer, K. Landzettel, T. Wolf, D. Reintsema, German Aerospace Center
Quasi-Synchronous Orbits
Quasi-Synchronous Orbits and Preliminary Mission Analysis for Phobos Observation and Access Orbits Paulo J. S. Gil Instituto Superior Técnico Simpósio Espaço 50 anos do 1º Voo Espacial Tripulado 12 de
Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti
Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti INSTRUCTIONS: Please, use the `bubble sheet and a pencil # 2 to answer the exam questions, by marking
TOPO Trajectory Operations Officer
ISS Live! was developed at NASA s Johnson Space Center (JSC) under NASA Contracts NNJ14RA02C and NNJ11HA14C wherein the U.S. Government retains certain rights. Console Handbook TOPO Trajectory Operations
A. 81 2 = 6561 times greater. B. 81 times greater. C. equally strong. D. 1/81 as great. E. (1/81) 2 = 1/6561 as great.
Q12.1 The mass of the Moon is 1/81 of the mass of the Earth. Compared to the gravitational force that the Earth exerts on the Moon, the gravitational force that the Moon exerts on the Earth is A. 81 2
Earth Coverage by Satellites in Circular Orbit
arth Coverage by Satellites in Circular Orbit Alan R. Washburn Department of Operations Research Naval Postgraduate School The purpose of many satellites is to observe or communicate with points on arth
Magnetism. d. gives the direction of the force on a charge moving in a magnetic field. b. results in negative charges moving. clockwise.
Magnetism 1. An electron which moves with a speed of 3.0 10 4 m/s parallel to a uniform magnetic field of 0.40 T experiences a force of what magnitude? (e = 1.6 10 19 C) a. 4.8 10 14 N c. 2.2 10 24 N b.
Nanosat 4 Competition
Nanosat 4 Competition NMSUSat2 Team New Mexico State University College of Engineering Presented by Jeremy Bruggemann Topics Competition Overview Mission Overview Design Concept Tests and Analyses Hardware
Chapter 11 Satellite Systems
Chapter 11 Satellite Systems 1 Outline Introduction Types of Satellite Characteristic of Satellite Systems Satellite System Infrastructures Call Setup GPS Limitations of GPS Beneficiaries of GPS Applications
USE OF SCILAB FOR SPACE MISSION ANALYSIS AND FLIGHT DYNAMICS ACTIVITIES
USE OF SCILAB FOR SPACE MISSION ANALYSIS AND FLIGHT DYNAMICS ACTIVITIES Thierry Martin CNES Scilabtec 09 Use of Scilab for space mission analysis Page 1 Use of Scilab in CNES Scilab is now widely used
C B A T 3 T 2 T 1. 1. What is the magnitude of the force T 1? A) 37.5 N B) 75.0 N C) 113 N D) 157 N E) 192 N
Three boxes are connected by massless strings and are resting on a frictionless table. Each box has a mass of 15 kg, and the tension T 1 in the right string is accelerating the boxes to the right at a
GPS Precise Point Positioning as a Method to Evaluate Global TanDEM-X Digital Elevation Model
GPS Precise Point Positioning as a Method to Evaluate Global TanDEM-X Digital Elevation Model 7 th FIG Regional Conference TS 1C Advances in GNSS Positioning and Applications I Volker Schwieger 1, Jürgen
Two primary advantages of radars: all-weather and day /night imaging
Lecture 0 Principles of active remote sensing: Radars. Objectives: 1. Radar basics. Main types of radars.. Basic antenna parameters. Required reading: G: 8.1, p.401-40 dditional/advanced reading: Online
Newton s Law of Universal Gravitation
Newton s Law of Universal Gravitation The greatest moments in science are when two phenomena that were considered completely separate suddenly are seen as just two different versions of the same thing.
Notes: Most of the material in this chapter is taken from Young and Freedman, Chap. 13.
Chapter 5. Gravitation Notes: Most of the material in this chapter is taken from Young and Freedman, Chap. 13. 5.1 Newton s Law of Gravitation We have already studied the effects of gravity through the
Presentation of problem T1 (9 points): The Maribo Meteorite
Presentation of problem T1 (9 points): The Maribo Meteorite Definitions Meteoroid. A small particle (typically smaller than 1 m) from a comet or an asteroid. Meteorite: A meteoroid that impacts the ground
Halliday, Resnick & Walker Chapter 13. Gravitation. Physics 1A PHYS1121 Professor Michael Burton
Halliday, Resnick & Walker Chapter 13 Gravitation Physics 1A PHYS1121 Professor Michael Burton II_A2: Planetary Orbits in the Solar System + Galaxy Interactions (You Tube) 21 seconds 13-1 Newton's Law
Moon Phases & Eclipses Notes
Moon Phases & Eclipses Notes Melka 2014-2015 The Moon The Moon is Earth s one natural satellite. Due to its smaller size and slower speed of rotation, the Moon s gravity is 1/6 of the Earth s gravitational
Presentation by: Dimov Stojce Ilcev DUT. CNS Systems. August 2011
Satellite Asset Tracking (SAT) of Ships, Containers, Vehicles, Wagons and Aircraft Presentation by: Dimov Stojce Ilcev DUT CNS Systems August 2011 SATELLITE OPERATORS Current Satellite Constellations Suitable
astronomy 2008 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.
1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. 5. If the distance between the Earth and the Sun were increased,
Analysis on the Long-term Orbital Evolution and Maintenance of KOMPSAT-2
Analysis on the Long-term Orbital Evolution and Maintenance of KOMPSAT-2 Ok-Chul Jung 1 Korea Aerospace Research Institute (KARI), 45 Eoeun-dong, Daejeon, South Korea, 305-333 Jung-Hoon Shin 2 Korea Advanced
VIETNAM ACADEMY OF SCIENCE AND TECHNOLOGY VIETNAM NATIONAL SATELLITE CENTER CUBESAT PICO DRAGON. Presenter Name: Do Xuan Phong
VIETNAM ACADEMY OF SCIENCE AND TECHNOLOGY VIETNAM NATIONAL SATELLITE CENTER CUBESAT PICO DRAGON Presenter Name: Do Xuan Phong Co-authors: Vu Viet Phuong, Truong Xuan Hung, Le Xuan Huy, Bui Nam Duong, Do
EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1
Instructor: L. M. Khandro EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1 1. An arc second is a measure of a. time interval between oscillations of a standard clock b. time
Nighthawk IV UAS. Versatility. User Friendly Design. Capability. Aerial Surveillance Simplified. [email protected] 800.639.6315 www.ara.
Aerial Surveillance Simplified The Nighthawk IV small unmanned aerial vehicle brings military hardened technology to civil agencies and commercial user groups. Supremely easy to operate and recently certified
The orbit of Halley s Comet
The orbit of Halley s Comet Given this information Orbital period = 76 yrs Aphelion distance = 35.3 AU Observed comet in 1682 and predicted return 1758 Questions: How close does HC approach the Sun? What
CHAPTER 2 ORBITAL DYNAMICS
14 CHAPTER 2 ORBITAL DYNAMICS 2.1 INTRODUCTION This chapter presents definitions of coordinate systems that are used in the satellite, brief description about satellite equations of motion and relative
UAV Road Surface Monitoring and Traffic Information
UAV Road Surface Monitoring and Traffic Information Czech Road and Motorway Network New capabilities for Unmanned Aerial Systems Current usage (military operation service) Possible civil usage (possible
How To Run A Space Station From A Polar Relay Station
SSC space expertise on high latitudes FMV Sensor Symposium Stockholm, September 2014 Björn Ohlson 1 50 years in space 1961 The first sounding rocket launch from Sweden 1962 Building of Esrange starts 1966
The Sun. Solar radiation (Sun Earth-Relationships) The Sun. The Sun. Our Sun
The Sun Solar Factoids (I) The sun, a medium-size star in the milky way galaxy, consisting of about 300 billion stars. (Sun Earth-Relationships) A gaseous sphere of radius about 695 500 km (about 109 times
Laser Ranging to Nano-Satellites
13-0222 Laser Ranging to Nano-Satellites G. Kirchner (1), Ludwig Grunwaldt (2), Reinhard Neubert (2), Franz Koidl (1), Merlin Barschke (3), Zizung Yoon (3), Hauke Fiedler (4), Christine Hollenstein (5)
Interaction of Energy and Matter Gravity Measurement: Using Doppler Shifts to Measure Mass Concentration TEACHER GUIDE
Interaction of Energy and Matter Gravity Measurement: Using Doppler Shifts to Measure Mass Concentration TEACHER GUIDE EMR and the Dawn Mission Electromagnetic radiation (EMR) will play a major role in
Phases of the Moon. The next phase, at about day 10, we can see roughly three quarters of the moon. This is called the waxing gibbous phase.
Phases of the Moon Though we can see the moon s size change throughout the month, it is really always the same size. Yet we see these different sizes or moon phases at regular intervals every month. How
Sun Earth Relationships
1 ESCI-61 Introduction to Photovoltaic Technology Sun Earth Relationships Ridha Hamidi, Ph.D. Spring (sun aims directly at equator) Winter (northern hemisphere tilts away from sun) 23.5 2 Solar radiation
Earth-Sun Relationships. The Reasons for the Seasons
Earth-Sun Relationships The Reasons for the Seasons Solar Radiation The earth intercepts less than one two-billionth of the energy given off by the sun. However, the radiation is sufficient to provide
Space Export Controls Update
Space Export Controls Update Since Delivering the 1248 Report to Congress - April 2012 Congress added language into the FY13 National Defense Authorization Act that gave the President the authority to
