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1 Orbital Mechanics Flashcards

(50 cards)

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1
Q

What is Kepler’s 1st Law?

A

Law of Ellipses

The centre of the larger of two orbiting bodies will one of the foci. With the orbital plane passing through that bodies centre.

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2
Q

What is Kepler’s 2nd Law?

A

Law of Equal Areas

A line joining a body and its orbiting satellite sweeps out equal areas in any given time. The satellite will therefore slow down at apogee and speed up at perigee.

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3
Q

What is Kepler’s 3rd Law?

A

Law of Harmonics

The square of the orbital period is proportional to the cube of the semi-major axis. Regardless of eccentricity, the period of an orbit is solely dependent on the size of the semi-major axis.

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4
Q

What is Newton’s 1st Law?

A

The Law of Inertia

An object will remain at rest or in constant motion in a straight line unless acted on by an external force.

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5
Q

What is Newton’s 2nd Law?

A

Law of Changing Momentum

The time rate of change of momentum (acceleration) is proportional to the force applied.

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6
Q

What is Newton’s 3rd Law?

A

Action - Reaction

For every action (force) there is an equal and opposite reaction.

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7
Q

What is the Law of Universal Gravitation?

A

The force of attraction between two bodies is…

directly proportional to the product of their masses…

and inversely proportional to the square of the distance between them.

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8
Q

Linear Momentum is…

A

Mass x Velocity

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9
Q

Angular Momentum is…

A

The resistance of a spinning object to change its spin rate/direction.

IMPORTANT: Angular momentum remains constant for an orbiting object which is not torqued.

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10
Q

Every orbit has an associated …. level.

A

Energy

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11
Q

Energy of a body in orbit is conversed. Transforming between ….. and ….. energy?

A

Kinetic and Potential

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12
Q

Mechanical energy =

A

KINETIC energy + POTENTIAL energy

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13
Q

Specific Mechanical Energy is….

A

ME normalised for satellite mass.

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14
Q

What is the difference between ME and SME?

A

Normalised for satellite mass

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15
Q

What coordinate reference frame do we use?

A

Earth Centred Inertial - ECI

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16
Q

What 4 things are used in the ECI reference system?

A

Origin (Centre of Gravity)
Fundamental Plane (Equatorial plane at 1200 01 Jan 2000 (J2000))
Principal Direction (Constant. Vernal Equinox - Quasars v. far away)
Normal Direction

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17
Q

What is Perigee?

A

Point at which an object is CLOSEST to the Earth in its orbit

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18
Q

What is Apogee?

A

Point at which an object is FURTHEST AWAY to the Earth in its orbit

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19
Q

Name the 6 COEs

A 
Semi Major Axis
Eccentricity
Inclination
Right Ascension of Ascending Node
Argument of Perigee
True Anomaly
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20
Q

In COE the Semi Major Axis describes what aspect of an orbit?

A

Size

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21
Q

In COE the Eccentricity describes what aspect of an orbit?

22
Q

In COE the Inclination describes what aspect of an orbit?

23
Q

In COE the RAAN describes what aspect of an orbit?

24
Q

In COE the Argument of Perigee describes what aspect of an orbit?

25
In COE the True Anomaly describes what aspect of an orbit?
Satellite Position
26
What line of a TLE contains information about the satellite, launch, time of TLE etc?
Line 1
27
What line of a TLE contains information about the orbit of a satellite?
Line 2
28
What are the 4 different orbit types?
LEO MEO HEO HEO
29
Describe a LEO (alt., per. and common uses)
Altitude - 150 km to 2,000 km Period - approx. 90 mins Polar Orbits Sun-Synchronous Orbits
30
Describe a MEO (alt., per. and common uses)
Altitude - 2,000 km to 35,862 km Period - approx. 11hr 58 mins Semi-synchronous
31
Name the 2 HEOs
Molniya Tundra
32
Describe a Molniya orbit (alt. and per.)
Altitude - 600 km to 40,000 km | Period - approx. 11 hr 58 mins
33
Describe a Tundra orbit (alt. and per.)
Altitude - 25,000 km to 46,000 km Period - approx. 23 hr 56 mins Inclination: 63.4 deg
34
Describe a GEO (alt. and per.)
Altitude - 35,862 km | Period - 23 hrs 56 mins
35
Describe a Polar Orbit
Passes over the N and S poles each revolution. Inclination = 90 deg Altitude between 200 km to 1,000 km Can observe the entire planet over a given period Used for reconnaissance and Earth observation
36
Describe a Sun-Synchronous Orbit (SSO)
Near-Polar Orbit (inclination approx. 98 deg) Passes over given point on Earth’s surface at same local mean solar time Same surface illumination each time it passes overhead Extensively used for IMINT gathering
37
Describe a Semi-Synchronous Orbit
Orbital period equal half that of the rotational period of the Earth (relative to the stars) Assuming prograde orbit it will pass over the same point on Earth’s surface pass after pass Typically used for GNSS such as GPS
38
Describe a Geosynchronous Earth Orbit (GEO)
Orbital period equal to that of the Earth’s rotational period
39
Describe a Geostationary Earth Orbit (GSO)
A special GEO that is perfectly aligned with the Earth’s equator This means it will appear to ‘hover’ over the same point on the Earth’s surface
40
Define the Semi Major Axis COE
Half the distance from Apogee to Perigee
41
Define the Eccentricity COE
Ratio of the distance between foci of the elliptical orbit and the Major Axis
42
Define the Inclination COE
Angle between the FUNDAMENTAL and ORBITAL planes... measured in a WESTWARD direction... at the ASCENDING NODE. 0 deg or 180 deg = equatorial 90 deg = polar <90 deg = prograde
43
Define the RAAN COE
The angle between the PRINCIPLE DIRECTION and the ASCENDING NODE... measured in an EASTWARD direction. 0 deg <= RAAN < 360 deg
44
Define the Argument of Perigee COE
Angle between the ASCENDING NODE and the point of PERIGEE... measured in the direction of travel.
45
Define the True Anomaly COE
Angle between PERIGEE and the objects position... measured in the direction of travel.
46
What happens to an orbits ground track over time?
Travels Westward
47
From a ground track how can we determine an orbits INCLINATION?
Prograde: max latitude of ground track Retrograde: 180 deg - max latitude of ground track
48
From a ground track how can we determine an orbits PERIOD?
By dividing nodal displacement by 15 deg/hr
49
From a ground track how can we determine an orbits Semi Major Axis?
From Kepler’s 3rd Law (harmonics). If the period is known.
50
From a ground track how can we determine an orbits ECCENTRICITY?
Circular orbits: Symmetrical Eccentric: Asymmetrical

Space I (9 decks)

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