Astro Complete

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Last updated 12:33 AM on 5/10/26
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140 Terms

1
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Kepler (not including his laws)

Sun = center of universe

Planets rotate around the sun in elliptical orbits

2
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What are keplers laws

1) The orbit of each planet about the Sun is an ellipse with the Sun at one focus

2) A planet moves faster in the part of its orbit nearer the Sun and slower when farther from the Sun, sweeping out equal areas in equal times.

3) Most distant planets orbit the Sun at slower average speeds, obeying the relationship p2=a3

3
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Newton

1665:

Invented calculus

Law of gravitation

First reflective telescope

1667:

Mathematical principals of natural philosophy

Newton's laws of motion

4
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Key people (ancient)

knowt flashcard image
5
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What chronological order do the ancients go in?

Aristotle, Ptolemy, Copernicus, Brahe, Kepler, Galileo, Newton

6
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What chronological order do the moderns go in?

Tsiolkovsky, Goddard, Von Brahn

7
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Konstantin Tsiolkovsky

Father of Russian cosmonautics

Invented the delta v equation

Demonstrated why rockets would be needed for space exploration

8
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Robert Goddard

Father of modern rocketry

Experiments with both solid and liquid fueled rockets were basis for development of ballistic missile, earth-orbiting satellites, and interplanetary exploration

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Werner von Braun

Created the V2 rocket

10
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What year was Sputnik

1957

11
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What year was laika

1957

12
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What year was Sputnik 3

1958

13
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In what order were GRAB-1 (first successful recon sat), Sputnik, and USAFA Dept. Astro created?

Sputnik, Dept Astro, GRAB-1

14
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In what order were GPS, returnable first-stage rocket, and sea-launched ASAT created?

GPS, ASAT, first stage

15
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What year did the us launch their first satellite, and what was the name

Explorer 1, 1958

16
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In 1958 & 1960, what programs did the US create

1958:

Air force's space and ballistic missile program

NASA

1960:

NRO

17
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When was AF space command first established

1982

18
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When was the US space command and US space force established

2019

19
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What altitude is orbit sustained

130 km

20
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What altitude does space begin, what it it called

100 km, karman line

21
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Why do objects stay in orbit at 130 km

Drag decreases as density decreases

22
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What are the effects on spacecraft from Charged particles

Spacecraft charging, Sputtering (sandblasting): Degrade solar panels, impact optics sensing. Mitigate by making redundant systems or shielding components

23
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What are the effects of EM radiation

Generate electrical power = good, Heats up spacecraft = good and bad, Damage electrical equipment = bad, Disrupt communications = bad

Mitigate by making redundant systems or shielding components

24
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What are the effects of a Free fall environment

Makes fluid measurements and delivery more difficult "sloshy" = bad, but allows us to develop super alloys and medicines = good.

No mitigation

25
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What are the effects of Earth’s atmosphere

Drag: Difficult to predict but negligible above 600 km. Atomic oxygen: weakens structures and degrades sensors.

Mitigate through new coatings and physical protections.

26
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What are the effects of the vacuum of space

Outgassing, cold welding, Limited heat transfer: conduction (can lead to cold welding), convection (there's no airflow), radiation (works great)

Mitigation: none

27
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What are the effects of micrometeoroids and space junk

Can cause lots of damage at high speeds, difficult to track (the SSN is tracking 60,000 pieces)

28
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What are the different manmade hazards

Space debris (old satellites, rocket bodies, launch vehicle shrouds), EM interference, and EMP

29
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What are all orbits shaped like

Conic sections:

Circle

Ellipse

Parabola

Hyperbola

30
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When does a satellite stay in orbit

Horizontal velocity allows the horizon to drop away before the spacecraft

31
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For a orbit, what is the tradeoff for a satellite between

Coverage, latency, and vulnerability

32
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What are LEO orbits and give some characteristics and missions

Low earth orbits

Closer and faster

Better resolution with worse coverage

ISR, communications

33
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What are MEO orbits, give characteristics, and missions

Medium earth orbit: between leo and geo

Moderate coverage, affected by radiation belts

PNT (GPS, Galileo, GLONASS, BeiDou)

34
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What are GEO orbits and give some characteristics and missions

Geo-synchronous/stationary earth orbits Closer

Farther away and slower

Better coverage and worse resolution

Continuous comms, missile warning, weather

35
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What are HEO orbits and give some characteristics and missions

Highly elliptical orbit with long dwell over high latitudes

Great for polar coverage

Communications, ISR, missile warnings

36
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What are the 6 Military Space Ops

SATCOM, PNT, Combat Power Projection, SDA, ISR, Detections Monitoring and Warning

37
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Describe PNT usage, satellite coverage, and examples

Precision strike, logistics, maneuver support

Requires 4 satellites for location and time

GPS, JDAM, Blue force tracker

38
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Describe SATCOM usage and examples

Beyond line of sight communications

Enables global C2 and secure links

Military SATCOM networks, AEHF

39
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Describe ISR usage

Imagery and signals intelligence

Detects changes across the em spectrum

Supports operation planning and situational awareness

40
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What does the SDA do

Tracks over 60000 objects in orbit

Prevents collisions and identifies threats

Uses ground and space based sensors

41
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Describe the core military mission of Detections Monitoring and Warning usage and examples

Infrared sensors detect launches

Strategic and tactical alerting

Weather satellites aid mission planning

SBIRS constellation

42
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Describe core military mission of Combat Power Projection usage

Space superiority is necessary precondition for joint force success

Space control includes

Orbital strike, space link interdiction, and terrestrial strike via jamming, EM, cyber, kinetic strikes

43
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What are the components of a space system (threat assessment)

Space segment, link segment, ground segment, user segment

44
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What is the USSF doctrine

Maps the operational environment of space to provide warfighters a complete picture of the threat environments fused with intelligence

45
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What are the four dimensions of space domain awareness

Physical, virtual, information, and human

46
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What is the defense/mitigaiton against electronic warfare

Nulling, frequency hopping, proliferation, direct attack

47
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Defense/mitigation for cyber attacks

Cybersecurity, Encryption, Nulling

48
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What is directed energy

Offer broad range of effects using lasers, high powered microwave or millimeter wave emitters, and particle beam weapons

49
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Defense/mitigation for directed energy

Physical hardening, shielding, coatings

Proliferation

Decoys

Direct attacks

50
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Defense/mitigation against orbital threats

Proliferation

Maneuver

Decoys

Direct attacks

51
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Defense/mitigation against ASAT kinetic weapons

Proliferation

Maneuver

Decoys

Direct attack

52
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Defense/mitigation against high altitude nuclear detonation

Radiation hardening

53
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What are the 2BEOM assumptions?

  • Drag negligible​

  • No Maneuvers​

  • No 3rd body​

  • Only Forces are due to gravity​

  • Mass of Earth >> Satellite​

  • Earth is a point mass​

  • Mass of Satellite is constant​

  • Inertial Frame

54
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Which assumptions are false?

Earth as point mass - it is actually oblate, causing the J2 effect, affecting RAAN and Arg. Perigee

Drag as negligible - it is not, it actually affects a (semimajor axis) and e (eccentricity)

55
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What orbits take advantage of the J2 effect?

Molniya (63 degrees, highly eccentric, focuses on northern hemisphere)

Tundra (115 degrees, almost geostationary but not over equator)

Sun-synchronous (passes same spot at same time every day)

56
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Active Sensor and examples

Emit electromagnetic radiation and collect reflection - SAR, liDar

57
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Passive Sensor and examples

Collect electromagnetic radiation emitted or reflected by subject - visible, infrared

58
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Stephan Boltzmann Law

Defines the total power (W) emitted by an object given a temperature

<p>Defines the total power (W) emitted by an object given a temperature</p>
59
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Weins Law

Defines the wavelength of peak emission

<p>Defines the wavelength of peak emission</p>
60
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Field of View

Angle that a satellite can see

61
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Swath Width

The distance the satellite can see on the ground

62
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What limits the minimum altitude of a satellite?

Swath width

63
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What limits the maximum altitude of a satellite?

Resolution

64
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Spatial Resolution

The size of the smallest object that can be identified in an image

<p>The size of the smallest object that can be identified in an image</p>
65
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Ground Sampling Distance

Distance between the centers of two consecutive pixel measurements on the ground. Ex: GSD=1 then each pixel is 1m x 1m

66
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National Image Interpretability Rating Scale (NIIRS)

Subjective scale of readability assigned to an image by an analyst

67
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Electromagnetic Field

Accelerated electric charge that creates radiation waves that convey/carry energy

68
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Antennas

Transducer between guided RF wave and Free space RF wave, usually metallic

69
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Gain

the ratio of power/RF energy directed in a particular direction, ie how strong your RF energy is

70
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Loss

Gain less than 1

71
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Isotropic Radiator

The baseline measurement where gain=0 and goes in any direction

72
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Modulation

Putting information (the message signal) onto an RF carrier by altering the pure carrier signal (wave)

73
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AM (amplitude modulation)

a high or low amplitude corresponds to 0 or 1

<p>a high or low amplitude corresponds to 0 or 1 </p>
74
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FM (frequency modulation)

where the instantaneous frequency shifts to, compared to the carrier frequency, corresponds to 0 or 1

<p>where the instantaneous frequency shifts to, compared to the carrier frequency, corresponds to 0 or 1</p>
75
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Phase shift keying

the length of the phase corresponds to a 0 or 1

<p>the length of the phase corresponds to a 0 or 1</p>
76
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Uplink

ground station to satellite

77
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Crosslink

satellite to satellite

78
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Downlink

satellite to ground station

79
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Wien’s Law

max wavelength (lambda max) = 2898/T (temp in Kelvin)

80
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Free Space Loss

Signal spread out on surface of a sphere centered on the transmit antenna, as signal goes further the sphere expands and the power is dispersed, leading to loss

81
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Figure of Merit for an Antenna

A single quantitative measure that combines the most important antenna performance characteristics into one value so different antennas can be compared for a specific mission or application

82
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Gr/T

Figure of Merit for receive antennas, gain of antenna over Temperature, measures how well it can receive weak signals compared to the noise it produces

83
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RF noise

Pn = k *T * B , more noise = higher equivalent temperature

84
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Signal to Noise Ratio (SNR)

Quality rating of RF link, bigger is better, C/N = Signal power/ noise power

85
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Eb/No

The SNR in digital satcom

86
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Equivalent Isotropic Radiated Power (EIRP)

Figure of merit for transmit antennas, RF power equivalent to that radiated from a single point in all directions

87
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Closed loop control system

Input, Controller, Actuator, Plant, Output, Sensor

88
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Difference between open and closed loop systems

Open loop systems do not have a sensor - they cannot gather feedback from the system and use it to make decisions in the future

89
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Input

An order

90
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Controller

Translates and inputs order into an action command

91
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Actuator

Takes commands from controller

92
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Plant

System being manipulated

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Output

desired effect

94
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Sensor

Measures output and gives info to controller

95
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Attitude

The rotational orientation of an object with respect to a particular reference frame

96
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Disturbance Torques

Aerodynamic Drag, Gravity Gradient, Solar Radiation Pressure, Magnetic Torque

97
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Active Actuators

Thrusters, Magnetorquers, Reaction wheel, Momentum wheel, Control Moment Gyro

98
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Passive Actuators

Gravity-gradient stabilization, spin stabilization, dampers

99
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Attitude Sensors

sun/earth/star sensors, gyroscope, magnetometer, differential GPS

100
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Equation to find period from altitude/height

where a = Radius(earth) + h

<p>where a = Radius(earth) + h</p>