Orbital Mechanics and Satellite Orbits, Lab Reports of Astronomy

This document, from an ast 101 course in fall 2007, covers pre-lab preparation for orbiting earth lab. It explains two formulae for calculating satellite velocity and period, and how they relate to the distance from the center of the earth. It also discusses low earth orbits (leo), geostationary or geosynchronous orbit (geosynch), and the ideal location for a spaceport.

Typology: Lab Reports

Pre 2010

Uploaded on 08/09/2009

koofers-user-lrx
koofers-user-lrx 🇺🇸

10 documents

1 / 3

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
Our Corner of the Universe
AST 101, Fall 2007
ORBITING EARTH LAB
Week of October 2
PRE-LAB PREPARATION
We will be making use of two formulae:
P
r
r
GM
π
υυ
2
(2)(1) ==
Equation (1) relates the velocity of a satellite around the Earth to the mass, M, of the
Earth and r, the distance of the satellite from the center of the Earth. G is Newton's
constant.
Equation (2) relates the velocity to r, and P, the period (or time it takes for the satellite to
complete one orbit). Putting these two equations together we can relate P, the period of
the orbit, to the distance from the center of the Earth.
2
1
32
4
(3)
=GM
r
P
π
Or we can solve 3 for r and find the needed radius to achieve a given period
3
1
2
2
4
(4)
=
π
GMP
r
The motion of a satellite, the relationship between its orbital period and its height, is
completely determined by Newton's Laws and the law of gravity! Orbits just above the
atmosphere are called low Earth orbits or LEO. We need to be high enough to minimize
friction with the atmosphere or drag. A height of about 130 km is the minimum practical
height of a satellite.
Q. How long does it take a satellite this height to complete an orbit (use eq. 3)? If the
satellite were 250 km high, what would its period be? Notice that there is little difference
in time. All LEO have essentially the same period.
Q. Using equation (4) find the radius of an orbit that would cause a satellite to orbit
Earth with a period of one sidereal day, 23 hours and 56 minutes. Equation (3) and this
1
pf3

Partial preview of the text

Download Orbital Mechanics and Satellite Orbits and more Lab Reports Astronomy in PDF only on Docsity!

Our Corner of the Universe

AST 101, Fall 2007

ORBITING EARTH LAB

Week of October 2

PRE-LAB PREPARATION

We will be making use of two formulae:

P

r

r

GM π υ υ

Equation (1) relates the velocity of a satellite around the Earth to the mass, M , of the Earth and r , the distance of the satellite from the center of the Earth. G is Newton's constant.

Equation (2) relates the velocity to r , and P , the period (or time it takes for the satellite to complete one orbit). Putting these two equations together we can relate P , the period of the orbit, to the distance from the center of the Earth.

GM

r P

Or we can solve 3 for r and find the needed radius to achieve a given period

(^13)

2

2

4

P GM

r

The motion of a satellite, the relationship between its orbital period and its height, is completely determined by Newton's Laws and the law of gravity! Orbits just above the atmosphere are called low Earth orbits or LEO. We need to be high enough to minimize friction with the atmosphere or drag. A height of about 130 km is the minimum practical height of a satellite.

Q. How long does it take a satellite this height to complete an orbit (use eq. 3)? If the satellite were 250 km high, what would its period be? Notice that there is little difference in time. All LEO have essentially the same period.

Q. Using equation (4) find the radius of an orbit that would cause a satellite to orbit Earth with a period of one sidereal day, 23 hours and 56 minutes. Equation (3) and this

period yield a radius of 42,200 km. A satellite on orbit at that radius would be 35,800 km above Earth's surface.

LAB

A satellite on an equatorial orbit at 35,800 km above Earth traveling east, is in a geostationary or geosynchronous orbit , often called geosynch. Many communications and weather satellites are on geosynch. From vantage points on Earth, these satellites appear fixed in the sky. "Satellite" dishes aimed at these points may receive microwave signals from the satellites 24 hours a day. From the satellite's viewpoint, its transmitter can send signals to, and its cameras can see, nearly one-third of Earth's surface, although it cannot effectively reach high (north or south) latitudes. Geosynch is an example of a high orbit.

An ideal location for a spaceport would be the top of the highest mountain on Earth's equator. This would allow satellites to achieve orbit with the minimum expenditure of rocket fuel. Launching eastward takes advantage of Earth's rotation, which provides a velocity of 1670 km/hr eastward at the equator. The Kennedy Space Center, at Cape Canaveral, Florida, is the primary launch facility of the United States space program. The location was chosen to take advantage of year-round warm weather, the availability of then undeveloped land, of being relatively close to Earth's equator in then "secure" US territory, and also to be on the eastern seaboard. Being on the eastern seaboard places rockets that fail early during their launches over the Atlantic Ocean, where there are no cities to be damaged by the falling debris.

PROCEDURES

Apparatus: Globe of Earth, rolls of removable tape, drawing compass, millimeter scale, and meter stick.

A. Drawing Orbits to Scale

  1. Use a drawing compass and draw as accurately as possible a circle to represent Earth, at the scale of 1.00 cm = 1000 km. Then, using the same center and scale, draw a circle to represent the orbit of a satellite 130 km above Earth.
  2. Use a drawing compass to draw another circle to represent Earth at the scale of 1. cm = 5000 km. Then, using the same center and scale, draw a circle to represent the orbit of a satellite at geosynch.
  3. Draw free hand, as accurately as possible, a circle to represent Earth at the scale of 1.00 cm = 50,000 km. Do this by placing two small marks a distance apart to represent the diameter of Earth, and then sketch a circle of that diameter. Then, using the center of that circle, and the same scale, draw a circle with a drawing compass to represent the orbit of the Moon.
  4. On the drawing showing the orbit of the Moon around Earth, add to scale as accurately as possible a low Earth orbit and a geostationary orbit.