Geosynchronous Satellite Problem

Slides:



Advertisements
Similar presentations
Earth-Moon-Sun System
Advertisements

Chapter S1 Celestial Timekeeping and Navigation
Chapter S1 Celestial Timekeeping and Navigation
Axial tilt is an astronomical term regarding the inclination angle of Earth’s rotational axis in relation to a perpendicular to its orbital plane Solar.
Celestial Coordinates
The Reason for the Seasons
Physics 101 Astronomy Dr. Brian Davies Office: 532 Currens Hall, Office Hours: M Tu W F 11-noon
Analemma Time Mean Solar Time: Time based on the average time between meridian crossings of the Sun. Each day is exactly 24 hours. Apparent Solar Time:
The Earth Rotates.
Latitude & Longitude.
Latitude & Longitude.
The Celestial Sphere The 88 official constellations cover the celestial sphere. If you do not have a model of the celestial sphere to bring to class, you.
The Earth-Moon-Sun System
Motion in the Sky. Discussion How do we estimate how far away things are from us in everyday life?
The Seasons, Solstices and Equinoxes
Earth Science 22.2B Motions Earth-Moon System
Chapter 5 Dynamics of Uniform Circular Motion. Circular Motion If the acceleration is in the same direction as the velocity i.e., parallel to the velocity,
Announcements Clear sky patrol has not yet started We will start using PRS units this week, make sure that you have one.
AST 111 Lecture 7 Eclipses, Solar and Sidereal Days, Precession.
Introduction to Positional Astronomy The Night Sky  Nick Devereux 2006.
Lesson 3 Notes Seasons on Earth What Causes Seasons?
Satellites D. Crowley, 2008.
1 Lecture 29 Measuring Time on Earth Ozgur Unal. 2  What time is it in your hometown at the moment?  What time is it in NYC?
Measuring Earth Midterm Review Topics: Earth’s true shape & evidence Positions on Earth (Latitude, Longitude, Angle of Polaris) Time Zones.
1. Earth and its Moon 2 © Zanichelli editore 2015.
Chapter 0: Charting the Heavens. Units of Chapter 0 The “Obvious” View Earth’s Orbital Motion The Motion of the Moon The Measurement of Distance Science.
AstroLab-2 Locating Stars in the Sky Merav Opher-Fall 2004.
Earth’s Rotation Earth rotates counterclockwise Earth is tilted on its axis 23.5 degrees.
Earth’s Moon - using radar we find the distance to the Moon to be 384,000 km (this is the length of the orbit’s semi-major axis).
Motion in the Sky. Discussion What is a year? Discussion What is a day?
Applications of our understanding of ‘G’ Fields Calculate the gravitational potential at the surface of the Earth (Data on data sheet). Answer = Now state.
Satellite Systems Presented By Sorath Asnani Mehran University of Engineering & Technology, Jamshoro.
35,000 feet = 6.62 miles 50 miles 250 miles  400 km 22,236 miles 363,000 to 405,000 km (approx 240,000 miles) This is the distance at which satellites.
Chapter: The Sun-Earth-Moon System
Chapter S1 Celestial Timekeeping and Navigation
Grab a piece of lined paper and your Unit 4 packets, and a BOOK
© 2017 Pearson Education, Inc.
Ancient astronomers believed that the stars were attached to a celestial sphere surrounding the Earth.
Lecture 7: Satellite Networks By: Adal ALashban.
Mapping: Locating Positions on Earth
12-4 Angle Measures and Segment Lengths
Lesson 3: Seasons on earth notes
Kepler’s Laws of Orbital Motion
Revolution and Rotation
Starter………. Write a new lesson title: ‘Solar System and Satellites’.
The Night Sky.
Gravitation.
AIM: The Earth Sun System
Earth Motions Astronomy Page 8 ©Mark Place,
Rank these objects by distance
Orbital Mechanics Basic Orbits Include:
Today! From Earth’s Perspective: Celestial Motion: Stellar Motion
SATELLITES.
Planet Report 3rd Grade Your name.
Communication System That Support the GMDSS
Satellites D. Crowley, 2008.
Naked Eye Astronomy The Cycles of the Sun Summer Winter
How Do We Use Earth’s Motion to Determine the Length of a Day?
Seasons.
Natural Sciences and Technology Grade 6
Satellite Meteorology
The Reasons for Seasons
Our Moving Planet.
Chapter 9: Earth and Space
Kepler’s 3rd Law Examples
Kepler’s Laws (see video)
Communication Systems
Week 3.
What is the Relationship Between Latitude and Polaris?
Presentation transcript:

Geosynchronous Satellite Problem

What Is a Geosynchronous Orbit? A geosynchronous orbit is simply an orbit that allows the satellite to remain apparently stationary above the same location on Earth. In order for a satellite's orbit to remain stationary above the same location on Earth, the satellite's orbital period (the time required for one complete orbit) needs to equal the Earth's rotational period - one day. Because the satellite orbits at the same rate the Earth rotates, the satellite remains stationary above the same longitude on Earth.   In addition for the satellite orbit to be truly geostationary, the orbit must not be inclined to the equator. Otherwise the satellite will oscillate in a north south direction above the same longitude.

Applications of Geosynchronous Orbits Anyone with a satellite TV receiver knows that the receiving antenna remains pointed toward the satellite at the same position in the sky. The receiver does not need to move to track the satellite because these satellites are in geosynchronous orbits. The fact that it is not necessary for a receiver or transmitter to move to track a satellite that is in a geosynchronous orbit makes these orbits particularly useful for communications satellites.

Earth's Rotational Period One might think Earth's rotational period is 24 hours, but it is actually 3 minutes and 56 seconds faster. A solar day, or 24 hours is Earth's apparent rotational period using the Sun as a reference. However the true rotational period of the Earth must be measured using the stars, rather than the Sun, as a reference. The day measured using stars as a reference is called a sidereal day. The length of the sidereal and solar days differ by nearly 4 minutes because the Earth travels almost a degree in its orbit around the Sun each day.

Problem A satellite is in geosynchronous orbit. Determine the height above the surface of Earth such a satellite must orbit. Determine the satellite’s speed. * It is ok if you use 24 hours for the period of earth rather than 23 hours 56 minutes.