Transcript Slide 1

More Satellite Orbits
Introduction to Space Systems and Spacecraft Design
Space Systems Design
More Orbits
Importance of Orbits to Mission
•
When should you start analyzing orbits to satisfy mission
requirements?
•
Can the orbit effect any of the following in the mission design?
― Revisit time of satellite to a point on earth?
― Amount of data that can be transferred between the satellite
and ground?
― Space radiation environment?
― Power generation for the satellite?
― Thermal control on the satellite?
― Launch costs?
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Orbit References
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Systems
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N
Orbit References
Orbit Types
GEO – Geosynchronous Orbit
LEO – Low Earth Orbit
S
Around Equator
HEO – Highly Elliptical Orbit
S
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Orbit With Respect to Sun
Noon-Midnight
(max eclipse)
Inclined
(partial eclipse)
Sun
Eclipse
Terminator Orbit - Twilight
(no eclipse)
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Orbit With Respect to Sun
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Orbit With Respect to Sun
Equinox
Earth's Axis
Summer
Winter
Sun
Equinox
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Spacecraft Orbital Velocity and Orbit Period
Spacecraft Velocity
Orbit Period
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Spacecraft Orbital Velocity and Orbit Period -2
What is ISS altitude?
h = (150) (1.852) = 278 km
= 17,142 mi/hour
convert
km/s
mi/hour
X (km/s) x 60s/m x 60m/hour x (1/1.6) mi/km = X (km/s) x 2250 mi/hour
V = (7.739 km/s) x 2250 mi/hour
= 17,142 mi/hour
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Equations to Remember
Vcir = 631.3481 r-1/2 km/sec
Vesc = 892.8611 r-1/2 km/sec
r
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- is from center of the earth
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Changing Orbits
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LEO – Low Earth Orbit
from a shuttle launch – 280 km
35,786 km
V = 3.0727 km/s
GEO
N
280 km
V = 7.738 km/s
LEO
S
How?
Want to Change Orbit
LEO to GEO
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Changing Orbits
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How?
35,786 km
V = 3.0727 km/s
GEO
1. Change to a GTO (GEO transfer Orbit)
For GTO
Va
Want:
Vp = 10.169 km/s
Va = 1.606 km/s
2. Circularize orbit
Need
Vp
LEO
V = 3.0727 km/s for GEO
Change V = 3.0727-1.606 = 1.4667 km/s
3. Burn at Va to increase V to 3.0727 km/s
for circular orbit at GEO
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Other Ways to Change Orbits
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Other Ways to Change Orbits
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Orbits Perturbations
Now you have an orbit for your satellite.
1.
Will it stay where you put it?
2.
Is there anything that will change the orbit
once you have it there?
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Orbits Perturbations
Special Effects on Orbits
Equinox
Winter
Summer
Sun
Equinox
What happens to the orbit plane
as the earth rotates around the
sun?
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Orbits Perturbations
What effects the orbit?
J2 effect
J22/J3 effect
Lunar gravity
Solar gravity
Solar pressure
Atmospheric drag
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Orbits Perturbations
Solar Pressure/Radiation
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Orbits Perturbations
Solar Pressure/Radiation
Using solar radiation
for propulsion.
Solar Sails
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Orbits Perturbations
Atmospheric Drag
Drag Coefficient
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Orbits Perturbations
Atmospheric Drag
Ballistic Coefficient
Bc = K (Mass/Cross Sectional Area)
How do they go through the atmosphere?
Which stays in orbit longer – a bowling ball or a soccer ball of
the same size?
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Orbits Perturbations
Atmospheric Drag
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Orbits Perturbations
Atmospheric Drag
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Orbits Perturbations
Earth-moon tidal friction mechanism
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Orbits Perturbations
Earth non-spherical effect
East-West drift occurs because the equator
is not perfectly circular, so satellites drift
slowly towards one of two longitudinal
stable points.
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Orbit References – GEO Station Keeping
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Orbits Perturbations
Earth non-spherical effect
Due to luni-solar perturbations and the
ellipticity of the Earth equator, an object
placed in a GEO without any stationkeeping would not stay there. It would
start building up inclination at an initial
rate of about 0.85 degrees per year.
After 26.5 years the object would have
an inclination of 15 degrees, decreasing
back to zero after another 26.5 years
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Orbits Perturbations
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Earth non-spherical effect
N
Inclination
S
What is the effect of this?
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Orbits Perturbations
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Inclination
> 900 Orbit
< 900 Orbit
N
N
> 90o
< 90o
S
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Orbits Perturbations
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Earth non-spherical effect
Oblatness causes
rotation counter
clockwise
N
I > 90o
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Oblatness causes
rotation clockwise
N
Prograde Orbit
I < 90o
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Orbits Perturbations
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Earth non-spherical effect
Orbit rotates to
maintain same angle
with sun
Sun
Synchronous
Orbit
a
Equinox
Summer
a
Winter
a
Sun
Equinox
a
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Orbits Perturbations
Earth non-spherical effect
Sun
Synchronous
Orbit
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Orbits Perturbations
Earth non-spherical effect
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Orbits Perturbations
Sun Synchronous Inclination
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Orbits Perturbations
Earth non-spherical effect
Special Molniya orbit has a stable orbit that is
used by Russians to have high latitude
communications – 2 satellites.
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Orbits Perturbations
Earth non-spherical effect
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Orbits Perturbations
Earth non-spherical effect
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Orbits Perturbations
Earth non-spherical effect
Effects are secular and accumulative
Which are these?
J2 effect
J22/J3 effect
Lunar gravity
Solar pressure
Atmospheric drag
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Orbits Perturbations
Earth non-spherical effect
GEO satellites have drift due to non-spherical earth
1. East-west drift
2. North-south drift
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Orbit References – GEO Station Keeping
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Special Orbits
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Geostationary Orbit
N
S
Geosynchronous Orbit
N
S
Zero Inclination GEO Orbits
Inclination GEO Orbits
Satellite appears stationery to
earth observer
Satellite appears go N-S & EW
in a figure 8 to earth observer
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GEO Orbits Characteristics
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GEO Orbits Characteristics
N
S
What is the maximum latitude that a
GEO satellite can be viewed?
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GEO Orbits Characteristics
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GEO Orbits Characteristics
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LEO Satellite Orbits
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LEO Orbits Characteristics
Footprint
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LEO Orbits Characteristics
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LEO Orbits Characteristics
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LEO Orbits Characteristics
What is elevation angle on
ground antenna?
How do you find Di? Use law of cosines.
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Objects in Orbit
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Objects in Orbit
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Importance of Orbits to Mission
• When should you start analyzing orbits to satisfy mission
requirements?
• Can the orbit effect any of the following in the mission design?
―
―
―
―
―
―
Revisit time of satellite to a point on earth?
Amount of data that can be transferred between the satellite
and ground?
Space radiation environment?
Power generation for the satellite?
Thermal control on the satellite?
Launch costs?
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Questions?
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