Orbital Satellite: 4) Non synchronous satellites have to be used when available,which may be little 15 minutes
|
|
- Christal Snow
- 5 years ago
- Views:
Transcription
1 Orbital Satellite: 1) Most of the satellites are orbital satellites and also called as Nonsynchronous Satellites. 2) Nonsynchronous Satellites are rotate around the earth in an elliptical or in circular pattern 3) In circular orbit the speed of rotation is constant for the satellites 4) For elliptical pattern the speed of the satellite is depend upon its height above the earth. 5) Speed of the satellite is greater when it is close to the earth than when it is farther away 1) If the satellite is orbiting in the same direction as Earth s rotation and at an angular velocity greater than that of Earth then the orbit is called prograde or posigrade 2) If the satellite is orbiting in the opposite direction as Earth s rotation or in the same direction at an angular velocity less than that of Earth, then the orbit is called retrograde 3) Non synchronous orbit always revolve around in prograde orbit.so it is continuously changing in respect to a fixed position on earth 4) Non synchronous satellites have to be used when available,which may be little 15 minutes 5) Advantage orbital satellites is propulsion rockets are not required to keep them in the orbit path 6) Expensive tracking equipment is needed to track the satellite is the main dis advantage
2 Satellite Elevation Categories: ORBITAL SATELLITES LOW EARTH ORBIT MEDIUM EARTH ORBIT GEOSYNCHRONOUS EARTH ORBIT LEO MEO GEO Frequency 1Ghz to 2.5 Ghz 1.2Ghz to 1.66Ghz Distance from Earth 480 Miles 6000 to Miles 2Ghz to 18Ghz to Miles Types of satellites Commercial Satellite for defense Commercial satellites and national use communication satellites Type of orbit Elliptical Elliptical Circular Advantages No path loss and less weight ) Geostationary satellites have an orbital time of approx. 24hrs.so it appears to be stationary and looks as fixed with respect to earth 2) Satellites between miles and miles said to be near synchronous orbit
3 3) If Satellite is slightly lower than miles from earth, the orbital time will be lower compared to the earth rotation period and move slowly around from west to east, so it is called as sub synchronous. 4) If Satellite is slightly higher than miles from earth the orbital will be longer compared to the earth rotation and it appear to have a reverse motion from east to west. Satellite Orbital Patterns: 1) The point in an orbit that is located farthest from earth is called Apogee. 2) The point in an orbit that is located closest from earth is called Perigee. 3) The line joining the Perigee and Apogee through center of earth is called Major axis. Sometimes called as line of apsides. 4) The line perpendicular to the major axis and halfway between the perigee and apogee is called minor axis. 5) Although we have numerous infinite numbers of orbits, only three of them is useful for communication purpose. 1) Inclined orbits 2) Polar orbits 3) Equatorial orbits 6) All satellite in an orbit forms a plane which passes through the center of gravity of earth called Geocenter. 7) The angle inclination is the angle between the earth equatorial s plane and the orbital plane of a satellite measured counterclockwise at the point in the orbit. 8) The point where a polar or inclined orbit crosses the equatorial plane travelling from south to north. This point is called ascending node.
4 9) The point where a polar or inclined orbit crosses the equatorial plane travelling from north to south. This point is called descending node. 10) The line joining the ascending and descending nodes through the center of earth is called line of nodes. 11) Inclined orbits are generally elliptical and vary between 0 and ) From Kepler s Law angular velocity of the satellite is slow at apogee. Therefore the satellite remains at longer period of time. 13) An equatorial orbit is when the satellite rotates in an orbit directly above the equator, usually in a circular path. Since the angle of inclination is 0 so there is no ascending order and descending order and hence no line of nodes. 14) All geosynchronous satellites are in equatorial orbits. 15) A polar orbit takes it over the north and south pole in an orbit perpendicular to the equatorial plane. 16) It follows a very low altitude path that is close to earth and passes over and very close to both the north and South Pole. 17) The angle of inclination of a polar orbit is nearly 90.A satellite also covers 100% of earth surface in a polar orbit 18) Satellite revolves around in a longitudinal orbit and earth rotate on its axis in latitudinal rotation. 19) Earth is not is a perfect sphere it bulges at the equator. The important reason is causing the elliptical orbit to rotate in a manner that causes the apogee and perigee to move around the earth. This phenomenon is called rotation of the line of apsides. 20) At a angle of inclination of 63.4 line of apsides is zero. 21) Another interesting type is molniya system of satellites, it is used in Russia for government communication purpose.
5 22) It is synchronous orbit, its perigee is 400km and apogee is 40,000km.the size of the ellipse was chosen to make its period exactly one-half a sidereal day. Geosynchronous satellites: 1) These satellite orbit having same angular velocity as earth, hence it is appeared to be fixed above one spot on earth s surface. 2) Since it seems to be fixed no special antenna tracking system is needed, it provide reliable communication to 40% of the earth surface. 3) Satellite is in orbit because of the balance between the centrifugal force and earth gravitational pull. If velocity of the satellite is high it will break out from the orbit, if velocity is low it suffering the earth gravitational pull. 4) Geosynchronous orbits are circular, so the speed of the rotation will be constant throughout the period. 5) There is only one geosynchronous orbit earth orbit; however it is occupied by so many satellites. 6) The excursion above and below the equator would build up at a rate of between 0.6 to 0.9 per year.in addition to that geosynchronous satellites in an elliptical orbit also rift in an east or west direction as viewed from earth. This process is called station keeping. 7) There are several requirements for satellites 1) It must have 0 angle of inclination 2) It should orbiting around same direction as earth s rotation with the same angular velocity. 8) The semi major axis is α=a (p) 2/3 = ( ) (0.9972) 2/3 = 42164km. 9) Earth equatorial radius is 6378km. so height (h) above mean sea level of a satellite is H= = 35768km.
6 10) Circumference (c) of a geosynchronous orbit is c = 2π(42164) = km 11) Therefore the velocity (v) of a geosynchronous satellite is v =(264790/24)=11033km/hr. 12) The round trip propagation delay between satellite and earth station located directly below it is t = ( d/c) =2(35768)/3*10 5 km/s = 238ms. Clarke Orbit: 1) Geosynchronous earth orbit is some time called as Clarke orbit or Clerk belt, 1) Be located directly above the equator 2) Travel in the same direction as earth s rotation at 6480mph. 3) Have an altitude of miles above earth 4) Complete one revolution in 24 hours. Advantages: 1) Expensive equipment is not required for geosynchronous satellite 2) They are available to all earth stations within their shadow 100% of the time. 3) There is no need for switch from one satellite to another satellite as they orbit overhead. 4) The effects of Doppler shift are negligible.
7 Disadvantages: 1) It needs sophisticated and heavy propulsion devices to keep them in a fixed orbit. 2) High altitude satellites introduce much longer delay. The delay between two earth stations is 500ms to 600ms 3) It requires high transmit power and more sensitive receivers because of longer distances and greater path losses. 4) High precision spaceman ship is required to put the satellite into the orbit and keep it there. Antenna look Angle: 1) To optimize the performance of the satellite, the direction of maximum gain of an earth station antenna must be pointed out directly at the satellite. 2) To determine that earth station antenna is aligned,two angles must be determined 1) Azimuth angle 2) Elevation angle 1) Geostationary satellite, the look angles of the earth station antenna need to be adjusted for once as the satellite will remain in a given position permanently, except for occasional minor variations. 2) The satellite location is specified with latitude and longitude similar to the way the location of a point on earth. 3) Since satellite is revolving around many miles above the earth, it has no latitude or longitude, therefore its location is identified by a point on the surface of earth directly below the satellite.it is called sub satellite point and for geo satellites it should fall on equator.so they all have 0 latitude. 4) Hence it will be given in degrees longitude east or west of the Greenwich meridian
8 Angle of Elevation: 1) It is the vertical angle formed between the direction of travel of an electromagnetic wave radiated from an earth station antenna pointing directly toward a satellite and the horizontal plane. 2) Smaller the elevation angle greater the distance a propagated wave must pass through earth s atmosphere. Due to absorption in atmosphere, and noise the signal wave may deteriorate and may not provide acceptable transmission quality. So 5 is considered as minimum acceptable angle of elevation. Azimuth Angle: 1) It is defined as the horizontal pointing angle of an earth station antenna.it is usually measured in clockwise direction in degrees from true north. 2) Angle of elevation and azimuth angle both depend on the latitude of the earth station and longitude of both earth station and satellite.
9 Satellite system link models: 1) A satellite system consist of three basic sections 1) An uplink 2) Transponder 3) Downlink Uplink model 1) The primary component within the uplink section of a satellite system is the earth station transmitter. 2) It consists of an IF modulator, an IF-to-RF microwave up converter, a high power amplifier and some means of band limiting the final output spectrum. Modulator BPF Mixer BPF HPA MW Generator 3) The above diagram is the transmitter in the earth station, the modulator converts the data signal to either FM or PSK or QAM signal in if frequency range. 4) Mixer converts the IF to RF frequencies; HPA provides adequate gain and output power to propagate the signal to the satellite transponder. HPA are normally klystron and travelling wave tube.
10 Transponder: 1) It consists of a BPF, low noise amplifier, frequency translator, allow level power amplifier and an output band pass filter. 2) The fig. bellow shows a simplified transponder diagram. 3) It is a RF to RF repeater, other configurations are IF and baseband repeaters similar to those used in microwave repeaters. 4) From the output of LNA the freq. translator which converts the high band uplink frequency to the low band down link frequency. 5) The low level power amplifier normally a travelling wave tube which will boost the power and send the data to earth station, each RF satellite channel requires a separate transponders. Downlink Model: 1) It consists of BPF, an LNA, and an RF-IF down converter; the figure below shows a typical earth station receiver. 2) The BPF limits the input noise power to the LNA. The LNA is a high sensitive, low noise device, such as a tunnel diode amplifier or a parametric amplifier.
11 3) The RF-IF down converter is a mixer/band pass filter combination that converts the received RF signal to an IF frequency BPF LNA Mixer BPF Demodula tor Cross Links: MW Generator 1) Occasionally, there is an application where it is necessary to communicate between satellites. This is done by satellite cross links are intersatellite links. 2) A disadvantage of using an ISL is that both the transmitter and the receiver are space bound 3) Here both the transmitter output power and input sensitivity are limited. Satellite system Link Equations: 1) The error performance of a digital satellite system is quite predictable. 2) When evaluating the performance of a satellite sytem,the uplink and downlink parameters are first considered separately, then the overall performance is determined in appropriate manner.
12 3) For a satellite radio the original or demodulated signal is digital in nature. And Rf portion of the radio is analog,that is FSK,PSK,QAM or some of the microwave carrier signal riding on a microwave carrier. Link Equations: 1) These equations separately analyze the uplink and down link sections 2) It considers only the ideal gains and losses, effects of the thermal noise associated with earth station transmitter, earth station receiver and the satellite transponder. Uplink Equation: (C/N 0 ) = (A t P in (L p L u )A r ) / (KT e ) = (A t P in (L p L u ))*G / KT e Where L p and L u are the additional uplink and downlink atmospheric losses, respectively. 3) The uplink and downlink signals must pass through earth s atmosphere, where they are partially absorbed by the moisture, oxygen, and particulates in the air. 4) Depending on the elevation angle Rf signal travels through the atmosphere varies from on earth station to another Advantages of Fiber Optic Communication: 1) Fiber cables are very thin, smaller and weigh lesser than coaxial/metallic cable 2) Fiber optic system use light frequencies as carrier.so it is having larger band width 3) It requires less space and easy to install without worrying about volatile liquids and gases. 4) It is immune to static interference and electrical noise sources like electrical motors. In fiber there is no magnetic induction between fiber cables and there is no possibility of cross talk
13 5) Metallic cables form capacitance between them and inductance along their conductors which act like low pass filter and limit the bandwidth of the system, but fiber optic is free from all. 6) It is virtually impossible to tap the information from a fiber cable. 7) It can operate at higher temperature and less affected by corrosive liquids and gases 8) It is cheaper comparing to other cables. 9) It is lost longer and are more reliable than metallic conductors because it is having higher tolerance to change in environmental conditions. Loses in optical fiber communication: 1) Power loss in an optical fiber cable is probably the most important characteristic of the cable. Power loss is often called attenuation and results in an reduction in the power of the light wave as it travels down the cable. 2) A db = 10log(p out / p in ) where A db is total reduction in power level,attenuation(unitless) p out is cable output power(watts) p in is cable input power 3) In general multi-mode fibers have more attenuation than single-mode cables because of increased scattering of light wave produced from the dopants in the glass. 4) A 13db cable loss reduces the output power to 50% of the input power. Attenuation of light is depending on the wavelength. 5) Three wavelengths 0.85microns- 20% loss per kilometer,1.3microns and 1.55microns- 5% loss per kilometer. 6) Attenuation of optical power is expressed in db. 7) P = p t * 10 -Al/10 where p= measured power level(watts) p t =transmitted power level (watts) A = cable power loss(db/km) l = cable length (km) 8) Likewise in db p(dbm) = p in (dbm) Al(dbm) where p = measured power level (dbm) p in = transmit power (dbm) Al = cable power loss, attenuation (db)
14 9) Transmission losses are one of the most important characteristics of fiber loss,the predominant losses in the optical fiber are 1) Absorption loss 2) Material or Rayleigh, scattering losses 3) Chromatic, or wavelength, dispersion 4) Radiation losses 5) Modal dispersion 6) Coupling losses
Advanced Electronic Communication Systems. Lecture 4. Satellite Orbits (2) Dr.Eng. Basem ElHalawany
Advanced Electronic Communication Systems Lecture 4 Satellite Orbits (2) Dr.Eng. Basem ElHalawany Orbital (nonsynchronous) Satellites (cont.) Posigrade orbit or Prograde: If the satellite is orbiting in
More informationCHAPTER 25 SATELLITE COMMUNICATIONS # DEFINITIONS TERMS. Satellite. 1) A celestial body that orbits around a planet.
CHAPTER 25 SATELLITE COMMUNICATIONS # DEFINITIONS TERMS 1) A celestial body that orbits around a planet. Satellite 2) Man-made satellites that orbit earth, providing a multitude of communication functions
More information(ii) We have already found out the velocity of the satellite in orbit in part (i) (using equation (2.5)) to be km/s
Chapter 2 Questions and Solutions Question 1. Explain what the terms centrifugal and centripetal mean with regard to a satellite in orbit around the earth. A satellite is in a circular orbit around the
More informationSatellite Communications
Satellite Communications Lecture (3) Chapter 2.1 1 Gravitational Force Newton s 2nd Law: r r F = m a Newton s Law Of Universal Gravitation (assuming point masses or spheres): Putting these together: r
More informationCreating Satellite Orbits
Exercises using Satellite ToolKit (STK) vivarad@ait.ac.th Creating Satellite Orbits 1. What You Will Do Create a low-earth orbit (LEO) satellite Create a medium-earth orbit (MEO) satellite Create a highly
More informationOrbit and Transmit Characteristics of the CloudSat Cloud Profiling Radar (CPR) JPL Document No. D-29695
Orbit and Transmit Characteristics of the CloudSat Cloud Profiling Radar (CPR) JPL Document No. D-29695 Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91109 26 July 2004 Revised
More informationMobile and Wireless Networks Course Instructor: Dr. Safdar Ali
Mobile and Wireless Networks Course Instructor: Dr. Safdar Ali Satellite Communication INTRODUCTION INTRODUCTION Communication satellite are off-course only one means of telecommunication transmission.
More informationRECOMMENDATION ITU-R S * Terms and definitions relating to space radiocommunications
Rec. ITU-R S.673-2 1 RECOMMENDATION ITU-R S.673-2 * Terms and definitions relating to space radiocommunications (Question ITU-R 209/4) (1990-2001-2002) The ITU Radiocommunication Assembly, considering
More informationFundamentals of Satellite technology
Fundamentals of Satellite technology Prepared by A.Kaviyarasu Assistant Professor Department of Aerospace Engineering Madras Institute Of Technology Chromepet, Chennai Orbital Plane All of the planets,
More informationComparative Study of LEO, MEO & GEO Satellites
Comparative Study of LEO, MEO & GEO Satellites Smridhi Malhotra, Vinesh Sangwan, Sarita Rani Department of ECE, Dronacharya College of engineering, Khentawas, Farrukhnagar, Gurgaon-123506, India Email:
More informationAS3010: Introduction to Space Technology
AS3010: Introduction to Space Technology L E C T U R E 6 Part B, Lecture 6 17 March, 2017 C O N T E N T S In this lecture, we will look at various existing satellite tracking techniques. Recall that we
More informationAS3010: Introduction to Space Technology
AS3010: Introduction to Space Technology L E C T U R E S 8-9 Part B, Lectures 8-9 23 March, 2017 C O N T E N T S In this lecture, we will look at factors that cause an orbit to change over time orbital
More informationSatellite Orbits.
atellite Orbits It was announced few days ago that a 6-ton NAA weather no-longer functioning satellite that was launched in 1991 would crash into arth some time between Thursday, 22 eptember 2011 and aturday,
More informationIntroduction to Satellite Orbits
Introduction to Satellite Orbits Dinesh Manandhar Center for Spatial Information Science The University of Tokyo Contact Information: dinesh@iis.u-tokyo.ac.jp Slide : 1 Basics of Satellite Orbits The speed
More informationSatellite meteorology
GPHS 422 Satellite meteorology GPHS 422 Satellite meteorology Lecture 1 6 July 2012 Course outline 2012 2 Course outline 2012 - continued 10:00 to 12:00 3 Course outline 2012 - continued 4 Some reading
More informationExperimental Analysis of Low Earth Orbit Satellites due to Atmospheric Perturbations
Experimental Analysis of Low Earth Orbit Satellites due to Atmospheric Perturbations Aman Saluja #1, Manish Bansal #2, M Raja #3, Mohd Maaz #4 #Aerospace Department, University of Petroleum and Energy
More informationMAHALAKSHMI ENGINEERING COLLEGE-TRICHY QUESTION BANK UNIT I PART A
MAHALAKSHMI ENGINEERING COLLEGE-TRICHY QUESTION BANK SATELLITE COMMUNICATION DEPT./SEM.:ECE/VIII UNIT I PART A 1.What are the different applications of satellite systems? *Largest International System(Intel
More informationSatellite communications and the environment of space. V 1.1 Swiss Space Summer Camp 2016 Images: NASA 1
Satellite communications and the environment of space Swiss Space Summer Camp 2016 Images: NASA 1 Can you name these satellites? Sputnik The first man made satellite Launched in 1957 by The USSR Mass 84kg,
More informationThe Mechanics of Low Orbiting Satellites Implications in Communication
Utah State University DigitalCommons@USU Undergraduate Honors Capstone Projects Honors Program 5-20-1985 The Mechanics of Low Orbiting Satellites Implications in Communication Lane Brostrom Utah State
More informationAssignment-I and Its Solution
Assignment-I and Its Solution Instructions i. Multiple choices of each questions are marked as A to D. One of the choices is unambiguously correct. Choose the most appropriate one amongst the given choices.
More informationMODULE 2 LECTURE NOTES 1 SATELLITES AND ORBITS
MODULE 2 LECTURE NOTES 1 SATELLITES AND ORBITS 1. Introduction When a satellite is launched into the space, it moves in a well defined path around the Earth, which is called the orbit of the satellite.
More informationChapter 2: Orbits and Launching Methods
9/20/ Chapter 2: Orbits and Launching Methods Prepared by Dr. Mohammed Taha El Astal EELE 6335 Telecom. System Part I: Satellite Communic ations Winter Content Kepler s First, Second, and Third Law Definitions
More informationANNEX 1. DEFINITION OF ORBITAL PARAMETERS AND IMPORTANT CONCEPTS OF CELESTIAL MECHANICS
ANNEX 1. DEFINITION OF ORBITAL PARAMETERS AND IMPORTANT CONCEPTS OF CELESTIAL MECHANICS A1.1. Kepler s laws Johannes Kepler (1571-1630) discovered the laws of orbital motion, now called Kepler's laws.
More informationTools of Astronomy Tools of Astronomy
Tools of Astronomy Tools of Astronomy The light that comes to Earth from distant objects is the best tool that astronomers can use to learn about the universe. In most cases, there is no other way to study
More informationName and Student ID Section Day/Time:
AY2 - Overview of the Universe - Midterm #1 - Instructor: Maria F. Duran Name and Student ID Section Day/Time: 1) Imagine we ve discovered a planet orbiting another star at 1 AU every 6 months. The planet
More informationPrinciples of Satellite Remote Sensing
Chapter 5 Principles of Satellite Remote Sensing Goal: Give a overview on the characteristics of satellite remote sensing. Satellites have several unique characteristics which make them particularly useful
More informationSatellite Orbital Maneuvers and Transfers. Dr Ugur GUVEN
Satellite Orbital Maneuvers and Transfers Dr Ugur GUVEN Orbit Maneuvers At some point during the lifetime of most space vehicles or satellites, we must change one or more of the orbital elements. For example,
More informationCelestial Mechanics and Satellite Orbits
Celestial Mechanics and Satellite Orbits Introduction to Space 2017 Slides: Jaan Praks, Hannu Koskinen, Zainab Saleem Lecture: Jaan Praks Assignment Draw Earth, and a satellite orbiting the Earth. Draw
More informationME 476 Solar Energy UNIT THREE SOLAR RADIATION
ME 476 Solar Energy UNIT THREE SOLAR RADIATION Unit Outline 2 What is the sun? Radiation from the sun Factors affecting solar radiation Atmospheric effects Solar radiation intensity Air mass Seasonal variations
More informationUNIT I SATELLITE ORBITS
UNIT I SATELLITE ORBITS 1.1 Introduction to satellite communication: Satellites are specifically made for telecommunication purpose. They are used for mobile applications such as communication to ships,
More informationAPPENDIX B SUMMARY OF ORBITAL MECHANICS RELEVANT TO REMOTE SENSING
APPENDIX B SUMMARY OF ORBITAL MECHANICS RELEVANT TO REMOTE SENSING Orbit selection and sensor characteristics are closely related to the strategy required to achieve the desired results. Different types
More informationChapter Seven. Solar Energy
Chapter Seven Solar Energy Why Studying Solar energy To know the heat gain or heat loss in a building In making energy studies In the design of solar passive homes. Thermal Radiation Solar spectrum is
More information1. (a) Describe the difference between over-expanded, under-expanded and ideallyexpanded
Code No: R05322106 Set No. 1 1. (a) Describe the difference between over-expanded, under-expanded and ideallyexpanded rocket nozzles. (b) While on its way into orbit a space shuttle with an initial mass
More informationLearning Lab Seeing the World through Satellites Eyes
Learning Lab Seeing the World through Satellites Eyes ESSENTIAL QUESTION What is a satellite? Lesson Overview: Engage students will share their prior knowledge about satellites and explore what satellites
More informationRECOMMENDATION ITU-R S Impact of interference from the Sun into a geostationary-satellite orbit fixed-satellite service link
Rec. ITU-R S.1525-1 1 RECOMMENDATION ITU-R S.1525-1 Impact of interference from the Sun into a geostationary-satellite orbit fixed-satellite service link (Question ITU-R 236/4) (21-22) The ITU Radiocommunication
More informationAP Physics Multiple Choice Practice Gravitation
AP Physics Multiple Choice Practice Gravitation 1. Each of five satellites makes a circular orbit about an object that is much more massive than any of the satellites. The mass and orbital radius of each
More informationKeplerian Elements Tutorial
Keplerian Elements Tutorial This tutorial is based on the documentation provided with InstantTrack, written by Franklin Antonio, N6NKF. Satellite Orbital Elements are numbers that tell us the orbit of
More informationSome Questions We ll Address Today
Some Questions We ll Address Today What makes a rocket go? How can a rocket work in outer space? How do things get into orbit? What s s special about geo-synchronous orbit? How does the force of gravity
More informationPhysics Mechanics. Lecture 29 Gravitation
1 Physics 170 - Mechanics Lecture 29 Gravitation Newton, following an idea suggested by Robert Hooke, hypothesized that the force of gravity acting on the planets is inversely proportional to their distances
More informationOrbit Definition. Reference Vector. Vernal (March) Equinox Vector. Sun Vector
Simulation: TMG Thermal Analysis User's Guide Orbit Definition TMG can model three types of orbits: Beta Angle, Geostationary and Classical. For Earth, three special classical orbits are already partially
More informationSAMPLE First Midterm Exam
Astronomy 1000 Dr C. Barnbaum SAMPLE First Midterm Exam Note: This is a sample exam. It is NOT the exam you will take. I give out sample exams so that you will have an understanding of the depth of knowledge
More informationPW-Sat two years on orbit.
13th of February 2014 is the second anniversary of launch of the first polish student-made satellite PW-Sat. Currently Students' Space Association on Warsaw University of Technology is working on another
More information4 Solar System and Time
4 olar ystem and Time 4.1 The Universe 4.1.1 Introduction The Universe consists of countless galaxies distributed throughout space. The bodies used in astro navigation belong to the Galaxy known as the
More informationMAE 180A: Spacecraft Guidance I, Summer 2009 Homework 2 Due Tuesday, July 14, in class.
MAE 180A: Spacecraft Guidance I, Summer 2009 Homework 2 Due Tuesday, July 14, in class. Guidelines: Please turn in a neat and clean homework that gives all the formulae that you have used as well as details
More informationDownloaded from
Chapter 8 (Gravitation) Multiple Choice Questions Single Correct Answer Type Q1. The earth is an approximate sphere. If the interior contained matter which is not of the same density everywhere, then on
More information17. According to the data below, what is the exact shape of the Earth?
1. The Earth is slightly flattened from a perfect spherical shape because of A) its rotation B) the pull of the sun and moon C) storms on the sun's surface D) its molten core 2. Which diagram most accurately
More information3.The wrecking crane shown is moving toward a brick wall that is to be torn down.
Test Name: Physics Practice Test Section 1 1.Which of the following best classifies a material that has extremely low conductivity? 1. A. semiconductor B. insulator C. metalloid D. conductor 2.Which of
More informationLecture 2c: Satellite Orbits
Lecture 2c: Satellite Orbits Outline 1. Newton s Laws of Mo3on 2. Newton s Law of Universal Gravita3on 3. Kepler s Laws 4. Pu>ng Newton and Kepler s Laws together and applying them to the Earth-satellite
More information(b) The period T and the angular frequency ω of uniform rotation are related to the cyclic frequency f as. , ω = 2πf =
PHY 302 K. Solutions for problem set #9. Non-textbook problem #1: (a) Rotation frequency of 1 Hz means one revolution per second, or 60 revolutions per minute (RPM). The pre-lp vinyl disks rotated at 78
More informationUnit 2: Celestial Mechanics
Unit 2: Celestial Mechanics The position of the Earth Ptolemy (90 168 AD) Made tables that allowed a user to locate the position of a planet at any past, present, or future date. In order to maintain circular
More informationAINOA GARCÍA MARTÍ LOW EARTH ORBIT SATELLITE COMMUNICATION NETWORKS. Bachelor of Science thesis
AINOA GARCÍA MARTÍ LOW EARTH ORBIT SATELLITE COMMUNICATION NETWORKS Bachelor of Science thesis Examiner: D.Sc. Taneli Riihonen Examiner and topic approved by the Faculty Council of the Faculty of Computing
More information3. Lunar Motions & Eclipses. Lunar Phases: Static & Dynamic. Static & Dynamic Lunar Phases. Earth & Moon: Both Show Phases!
3. Lunar Motions & Eclipses Lunar motions & lunar phases Lunar axial rotation & orbital revolution Eclipses & the line of nodes Lunar eclipses Solar eclipses Relative Earth-Moon-Sun distances Lunar Motions
More informationLecture 1d: Satellite Orbits
Lecture 1d: Satellite Orbits Outline 1. Newton s Laws of Motion 2. Newton s Law of Universal Gravitation 3. Kepler s Laws 4. Putting Newton and Kepler s Laws together and applying them to the Earth-satellite
More information1. In Young s double slit experiment, when the illumination is white light, the higherorder fringes are in color.
TRUE-FALSE STATEMENTS: ELECTRICITY: 1. Electric field lines originate on negative charges. 2. The flux of the electric field over a closed surface is proportional to the net charge enclosed by the surface.
More informationCS6956: Wireless and Mobile Networks Lecture Notes: 2/4/2015
CS6956: Wireless and Mobile Networks Lecture Notes: 2/4/2015 [Most of the material for this lecture has been taken from the Wireless Communications & Networks book by Stallings (2 nd edition).] Effective
More informationObserving the Night Sky: Locating Objects
Observing the Night Sky: Locating Objects As I left the house this morning, there was a bright bluish light above and to the left of my neighbors house (approximately East) and a big very bright object
More informationPHYS 1303 Final Exam Example Questions
PHYS 1303 Final Exam Example Questions (In summer 2014 we have not covered questions 30-35,40,41) 1.Which quantity can be converted from the English system to the metric system by the conversion factor
More informationA SIMULATION OF THE MOTION OF AN EARTH BOUND SATELLITE
DOING PHYSICS WITH MATLAB A SIMULATION OF THE MOTION OF AN EARTH BOUND SATELLITE Download Directory: Matlab mscripts mec_satellite_gui.m The [2D] motion of a satellite around the Earth is computed from
More informationEARTHS SHAPE AND POLARIS PRACTICE 2017
1. In the diagram below, letters A through D represent the locations of four observers on the Earth's surface. Each observer has the same mass. 3. Which diagram most accurately shows the cross-sectional
More informationSection 13. Orbit Perturbation. Orbit Perturbation. Atmospheric Drag. Orbit Lifetime
Section 13 Orbit Perturbation Orbit Perturbation A satellite s orbit around the Earth is affected by o Asphericity of the Earth s gravitational potential : Most significant o Atmospheric drag : Orbital
More informationThe Earth, Moon, and Sky. Lecture 5 1/31/2017
The Earth, Moon, and Sky Lecture 5 1/31/2017 From Last Time: Stable Orbits The type of orbit depends on the initial speed of the object Stable orbits are either circular or elliptical. Too slow and gravity
More informationRadial Acceleration. recall, the direction of the instantaneous velocity vector is tangential to the trajectory
Radial Acceleration recall, the direction of the instantaneous velocity vector is tangential to the trajectory 1 Radial Acceleration recall, the direction of the instantaneous velocity vector is tangential
More informationScientists observe the environment around them using their five senses.
Earth Science Notes Topics 1: Observation and Measurement Topic 2: The Changing Environment Review book pages 1-38 Scientists observe the environment around them using their five senses. When scientists
More informationRemote Sensing in Meteorology: Satellites and Radar. AT 351 Lab 10 April 2, Remote Sensing
Remote Sensing in Meteorology: Satellites and Radar AT 351 Lab 10 April 2, 2008 Remote Sensing Remote sensing is gathering information about something without being in physical contact with it typically
More informationNAVIGATION THEORY QUESTIONS Basics of Navigation
NAVIGATION THEORY QUESTIONS Basics of Navigation Q610065 look at it The angle between the plane of the ecliptic and the plane of equator is approx? 23.5 degrees In which two months of the year is the difference
More informationQuestion 8.1: the following: (a) You can shield a charge from electrical forces by putting it inside a hollow conductor. Can you shield a body from the gravitational influence of nearby matter by putting
More informationFUNDAMENTALS OF REMOTE SENSING FOR RISKS ASSESSMENT. 1. Introduction
FUNDAMENTALS OF REMOTE SENSING FOR RISKS ASSESSMENT FRANÇOIS BECKER International Space University and University Louis Pasteur, Strasbourg, France; E-mail: becker@isu.isunet.edu Abstract. Remote sensing
More informationRAPID GEOSYNCHRONOUS TRANSFER ORBIT ASCENT PLAN GENERATION. Daniel X. Junker (1) Phone: ,
RAPID GEOSYNCHRONOUS TRANSFER ORBIT ASCENT PLAN GENERATION Daniel X. Junker (1) (1) LSE Space GmbH, Argelsrieder Feld 22, 82234 Wessling, Germany, Phone: +49 160 9111 6696, daniel.junker@lsespace.com Abstract:
More informationCIRCULAR MOTION AND SHM : Higher Level Long Questions.
CIRCULAR MOTION AND SHM : Higher Level Long Questions. ***ALL QUESTIONS ARE HIGHER LEVEL**** Circular Motion 2012 Question 12 (a) (Higher Level ) An Olympic hammer thrower swings a mass of 7.26 kg at the
More informationAST 103 Midterm 1 Review Exam is 3/3/08 in class
AST 103 Midterm 1 Review Exam is 3/3/08 in class Exam is closed book/closed notes. Formulas will be provided. Bring a No. 2 pencil for the exam and a photo ID. Calculators are OK, but will not be needed.
More informationINTRODUCTION: Ptolemy geo-centric theory Nicolas Copernicus Helio-centric theory TychoBrahe Johannes Kepler
INTRODUCTION: Ptolemy in second century gave geo-centric theory of planetary motion in which the Earth is considered stationary at the centre of the universe and all the stars and the planets including
More informationa. 0.1 AU b. 10 AU c light years d light years
1 AST104 Sp2006: EXAM 1 Multiple Choice Questions: Mark the best answer choice on the bubble form. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1.
More informationSpace Environment & Technology Space Policy and Law Course 2018
Space Environment & Technology Space Policy and Law Course 2018 Professor Alan Smith Mullard Space Science Laboratory University College London 15 October 2018 Orbits and Space The Space Environment The
More informationCOMPARISON OF ANGLES ONLY INITIAL ORBIT DETERMINATION ALGORITHMS FOR SPACE DEBRIS CATALOGUING
COMPARISON OF ANGLES ONLY INITIAL ORBIT DETERMINATION ALGORITHMS FOR SPACE DEBRIS CATALOGUING Fran Martinez Fadrique, Alberto Águeda Maté, Joan Jorquera Grau, Jaime Fernández Sánchez, Laura Aivar García
More information14.1 Earth Satellites. The path of an Earth satellite follows the curvature of the Earth.
The path of an Earth satellite follows the curvature of the Earth. A stone thrown fast enough to go a horizontal distance of 8 kilometers during the time (1 second) it takes to fall 5 meters, will orbit
More informationElectricity & Magnetism Study Questions for the Spring 2018 Department Exam December 4, 2017
Electricity & Magnetism Study Questions for the Spring 2018 Department Exam December 4, 2017 1. a. Find the capacitance of a spherical capacitor with inner radius l i and outer radius l 0 filled with dielectric
More informationa. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU
1 AST104 Sp04: WELCOME TO EXAM 1 Multiple Choice Questions: Mark the best answer choice. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1. A galaxy
More informationGirish K.P.
SATELLITE COMMUNICATION SYSTEMS Girish K.P. Communication satellites bring the world to you anywhere and any time.. What exactly is a satellite? The word satellite originated from the Latin word Satellit
More informationPH2200 Practice Final Exam Summer 2003
INSTRUCTIONS 1. Write your name and student identification number on the answer sheet. 2. Please cover your answer sheet at all times. 3. This is a closed book exam. You may use the PH2200 formula sheet
More informationIII. Spherical Waves and Radiation
III. Spherical Waves and Radiation Antennas radiate spherical waves into free space Receiving antennas, reciprocity, path gain and path loss Noise as a limit to reception Ray model for antennas above a
More informationName Period 4 th Six Weeks Notes 2013 Weather
Name Period 4 th Six Weeks Notes 2013 Weather Radiation Convection Currents Winds Jet Streams Energy from the Sun reaches Earth as electromagnetic waves This energy fuels all life on Earth including the
More informationis a revolution relative to a fixed celestial position. is the instant of transit of mean equinox relative to a fixed meridian position.
PERIODICITY FORMULAS: Sidereal Orbit Tropical Year Eclipse Year Anomalistic Year Sidereal Lunar Orbit Lunar Mean Daily Sidereal Motion Lunar Synodical Period Centenial General Precession Longitude (365.25636042
More informationLecture 19: The Moon & Mercury. The Moon & Mercury. The Moon & Mercury
Lecture 19: The Moon & Mercury The Moon & Mercury The Moon and Mercury are similar in some ways They both have: Heavily cratered Dark colored surfaces No atmosphere No water They also have some interesting
More informationCan you shield a body from the gravitational influence of nearby matter by putting it inside a hollow sphere or by some other means?
Question 8.1: the following: You can shield a charge from electrical forces by putting it inside a hollow conductor. Can you shield a body from the gravitational influence of nearby matter by putting it
More informationPHYS 101 Previous Exam Problems. Gravitation
PHYS 101 Previous Exam Problems CHAPTER 13 Gravitation Newton s law of gravitation Shell theorem Variation of g Potential energy & work Escape speed Conservation of energy Kepler s laws - planets Orbits
More informationSAPTARSHI CLASSES PVT. LTD.
SAPTARSHI CLASSES PVT. LTD. NEET/JEE Date : 13/05/2017 TEST ID: 120517 Time : 02:00:00 Hrs. PHYSICS, Chem Marks : 360 Phy : Circular Motion, Gravitation, Che : Halogen Derivatives Of Alkanes Single Correct
More informationlightyears observable universe astronomical unit po- laris perihelion Milky Way
1 Chapter 1 Astronomical distances are so large we typically measure distances in lightyears: the distance light can travel in one year, or 9.46 10 12 km or 9, 600, 000, 000, 000 km. Looking into the sky
More informationMapping Earth s Surface Chapter 2 Section 3
Mapping Earth s Surface Chapter 2 Section 3 Day 1 Objective I will understand maps can be used to find locations on Earth and to represent information about features on Earth s Surface I will understand
More informationUNIVERSITY OF TECHNOLOGY, SYDNEY
THllS PAPER MUST NOT BE REMOVED TO BE RETURNED AT THE END OF THE EXAMINA'TION UNIVERSITY OF TECHNOLOGY, SYDNEY NAME: STUDENT NUMBER: COURSE: AUTUMN SEMESTER EXAMINATION 2007 Subject Number: 91 120 GIs
More informationRate of area swept by the radial vector from the centre of the orbit. Rate of area swept by the radial vector from the centre of the earth
Q Questions 1 Which of the following quantites remains constant for a satellite in an elliptical orbit around the earth? Kinetic energy Product of speed and radial distance from the centre of the earth
More informationAST111, Lecture 1b. Measurements of bodies in the solar system (overview continued) Orbital elements
AST111, Lecture 1b Measurements of bodies in the solar system (overview continued) Orbital elements Planetary properties (continued): Measuring Mass The orbital period of a moon about a planet depends
More informationConceptual Physics Fundamentals
Conceptual Physics Fundamentals Chapter 6: GRAVITY, PROJECTILES, AND SATELLITES This lecture will help you understand: The Universal Law of Gravity The Universal Gravitational Constant, G Gravity and Distance:
More information= o + t = ot + ½ t 2 = o + 2
Chapters 8-9 Rotational Kinematics and Dynamics Rotational motion Rotational motion refers to the motion of an object or system that spins about an axis. The axis of rotation is the line about which the
More informationMAE 180A: Spacecraft Guidance I, Summer 2009 Homework 4 Due Thursday, July 30.
MAE 180A: Spacecraft Guidance I, Summer 2009 Homework 4 Due Thursday, July 30. Guidelines: Please turn in a neat and clean homework that gives all the formulae that you have used as well as details that
More informationQ1. (a) Explain what is meant by the gravitational potential at a point in a gravitational field (2)
PhysicsAndMathsTutor.com 1 Q1. (a) Explain what is meant by the gravitational potential at a point in a gravitational field............. Use the following data to calculate the gravitational potential
More informationUNIVERSITY OF CAMBRIDGE INTERNATIONAL EXAMINATIONS General Certificate of Education Advanced Level
UNIVERSITY OF CAMBRIDGE INTERNATIONAL EXAMINATIONS General Certificate of Education Advanced Level *1643892600* PHYSICS 9702/42 Paper 4 A2 Structured Questions October/November 2011 2 hours Candidates
More informationOrbits in Geographic Context. Instantaneous Time Solutions Orbit Fixing in Geographic Frame Classical Orbital Elements
Orbits in Geographic Context Instantaneous Time Solutions Orbit Fixing in Geographic Frame Classical Orbital Elements Instantaneous Time Solutions Solution of central force motion, described through two
More information1. The bar graph below shows one planetary characteristic, identified as X, plotted for the planets of our solar system.
1. The bar graph below shows one planetary characteristic, identified as X, plotted for the planets of our solar system. Which characteristic of the planets in our solar system is represented by X? A)
More informationCircular vs. Elliptical Orbits for Persistent Communications
5th Responsive Space Conference RS5-2007-2005 Circular vs. Elliptical Orbits for Persistent Communications James R. Wertz Microcosm, Inc. 5th Responsive Space Conference April 23 26, 2007 Los Angeles,
More informationGRAVITATION CONCEPTUAL PROBLEMS
GRAVITATION CONCEPTUAL PROBLEMS Q-01 Gravitational force is a weak force but still it is considered the most important force. Why? Ans Gravitational force plays an important role for initiating the birth
More information