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ASEN 5050 SPACEFLIGHT DYNAMICS Mission Orbits, Constellation Design

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ASEN 5050 SPACEFLIGHT DYNAMICS Mission Orbits, Constellation Design Prof. Jeffrey S. Parker University of Colorado Boulder Lecture 35: Orbits * – PowerPoint PPT presentation

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Title: ASEN 5050 SPACEFLIGHT DYNAMICS Mission Orbits, Constellation Design


1
ASEN 5050SPACEFLIGHT DYNAMICSMission Orbits,
Constellation Design
  • Prof. Jeffrey S. Parker
  • University of Colorado Boulder

2
Announcements
  • STK Lab 3 due Friday 12/5
  • STK Lab 4 due 12/12
  • Planetary ephemerides should be changed to DE421
    instead of Default
  • Final Exam on 12/12, due 12/18
  • Take-home, open book open notes
  • Final project and exam due 12/18

3
Schedule from here out
  • 12/3 Mission Orbits, Constellation Design
  • 12/5 Spacecraft Navigation
  • 12/8 Final Review, part 1
  • 12/10 Final Review, part 2
  • 12/12 Deep Impact

4
Final Project
  • Due 12/18. If you turn it in by 12/12, Ill
    forgive 5 pts of deductions.
  • Worth 20 of your grade, equivalent to 6-7
    homework assignments.
  • Final Exam is worth 25.
  • Find an interesting problem and investigate it
    anything related to spaceflight mechanics (maybe
    even loosely, but check with me).
  • Requirements Introduction, Background,
    Description of investigation, Methods, Results,
    Conclusions, References.
  • You will be graded on quality of work, scope of
    the investigation, and quality of the
    presentation. The project will be built as a
    webpage, so take advantage of web design as much
    as you can and/or are interested and/or will help
    the presentation.

5
Final Project
  • Instructions for delivery of the final project
  • Build your webpage with every required file
    inside of a directory.
  • Name the directory LastName_FirstName i.e.,
    Parker_Jeff/
  • there are a lot of duplicate last names in this
    class!
  • You can link to external sites as needed.
  • Name your main web page index.html
  • i.e., the one that you want everyone to look at
    first
  • Make every link in the website a relative link,
    relative to the directory structure within your
    named directory.
  • We will move this directory around, and the links
    have to work!
  • Test your webpage! Change the location of the
    page on your computer and make sure it still
    works!
  • Zip everything up into a single file and upload
    that to the D2L dropbox.

6
Space News
  • Japans Hayabusa 2 launched last night!

7
Space News
  • Japans Hayabusa 2 launched last night!

8
Space News
  • Orions Exploration Flight Test 1 Thurs 12/4 at
    704 am Eastern Time (504 am Mountain!).
    Duration 4.5 hours.

9
ASEN 5050SPACEFLIGHT DYNAMICSMission Orbits
  • Prof. Jeffrey S. Parker
  • University of Colorado Boulder

10
Satellite Populations
Molniya
51.5
28.5
11
Satellite Populations
12
Satellite Populations
Molniya, GNSS
13
Satellite Populations
Gabbard classes
GEO
GNSS
GTO
ISS
14
Satellite Populations
15
Frozen Orbits
  • Molniya orbits are designed to have a critical
    inclination, such that the argument of perigee
    does not change over time.
  • Example plots for NROSS frozen orbit
    characteristics

16
Repeat Groundtracks
  • Exact Repeat Groundtracks
  • A satellites ground track returns to exactly the
    same latitude/longitude that it began.
  • Should occur within 50 days for this
    classification
  • The satellite never flies over much of the Earth.
  • Near-exact Repeat Groundtracks
  • A satellites ground track returns to a point
    very near its starting point.
  • The drift provides a dense coverage of the Earth.

17
Repeat Groundtracks
  • Example exact repeat groundtracks

18
Repeat Groundtracks
The nodal crossings occur in a pattern
19
Some Period Definitions
20
General Perturbation Techniques
  • The secular change of the orbital elements due to
    J2 is given from the Lagrange Planetary Equations
    as

21
Nodal Period
22
Exact Repeat Constraint
23
Altitude/Inclination vs NERP/K
NERP/K
24
Groundtrack Drift
25
TOPEX Crosstrack Drift
26
Altimetry Missions
  • Consider Topex/Poseidon, Jason, Jason-2, and the
    like.
  • They perform remote sensing operations of the
    ocean surface, including measuring the sea
    surface height, sea surface smoothness,
    temperature, etc.
  • Driving requirements
  • The orbit must be very well known and well
    determined.
  • A meter error in height may make the ocean height
    estimation off by a meter very significant!
  • The orbit should pass over a large portion of the
    oceans surface.
  • The orbit should pass over the same points within
    a reasonably short time period.
  • The fly-over period should not alias any effects
    that significantly contribute to the motion of
    water in the ocean, such as tides.

27
Altimetry Missions
  • Parke et al. (1987) developed the following
    requirements for the orbit of Topex/Poseidon
  • The satellites altitude must be known to within
    14 cm
  • The orbit should be compatible with that sort of
    OD requirement. I.e., it would not work to orbit
    too close to the atmosphere or in an unstable
    resonance with the gravity field.
  • Minimize the spatial and temporal aliases on
    surface geotrophic currents, geoid variations,
    etc.
  • Subsatellite groundtrack should repeat within 1
    km.
  • Tidal aliases will not be aliased into
    semiannual, annual, or zero frequencies or to
    frequencies close to these.
  • The global grid of subsatellite points must
    extend as far south as the southern limit of the
    Drake Passage (62 deg S)
  • The ascending and descending tracks must cross at
    sufficiently large angles to resolve the 2D
    geostrophic current.

28
Altimetry Missions
  • Station Keeping
  • Atmospheric drag is one of the largest effects
    that drives the ground track away from its
    reference, and therefore must be compensated for
    using maneuvers.
  • For a circular orbit and neglecting the Earths
    rotation
  • The loss of energy over time due to drag

29
Altimetry Missions
  • The loss of energy over time due to drag

Varies with time
30
Altimetry Missions
  • The change in energy over time
  • Integrate
  • Integrate over one orbit period

31
Altimetry Missions
  • The change in energy over time
  • Integrate
  • If drag were estimated with 50 accuracy, then
    the orbit error for the satellite will be lt 1 cm
    for a satellite above 1100 km.
  • Recommendation remain above 1100 km and
    preferably above 1300 km.

32
Altimetry Missions
  • Effects of Solar Radiation Pressure.
  • Since solar panels are virtually always pointing
    toward the Sun, there is always a force acting on
    the satellite, and it changes the circular
    orbits semimajor axis

33
Altimetry Missions
  • Circular orbits

Minimum between 1200 1300 km
34
Altimetry Missions
  • Altitude
  • Desirable to be as high as possible for OD
  • Desirable to be 1200 1300 km for station
    keeping
  • Good for link budgets too
  • Desirable to be below 1500 km for radiation Van
    Allen Belts!

35
Altimetry Missions
  • Polar Crossing Angle psi

36
Altimetry Missions
Desirable gt 40 deg
37
Altimetry Missions
Less Desirable
Desirable gt 40 deg
38
Altimetry Missions
  • Orbit Period Considerations
  • Tidal Aliasing
  • Want to avoid this

39
Altimetry Missions
  • Tidal Aliasing, the frequencies, periods, and
    amplitudes of the most significant tidal
    constituents

40
Primary Lunar Tide
41
Vertical displacement
  • If the Earths surface was in equilibrium with
    the potential from the moon, the vertical
    displacement of the surface would be in the shape
    of an ellipsoid elongated toward the moon.

42
The Principal Tide M2
  • The largest component of the tides is associated
    with the potential due to the moon and with the
    frequency of the motion of the Earth-moon system
    around its center of mass.
  • The time from high moon to high moon1 lunar day
    (1 1 day/ 27.5 days) 24 hours 50.47 minutes
  • High tide separation is half of this
  • 12 hours 25 minutes
  • However, this component, like all of the
    semi-diurnal (and diurnal) tides is not in
    equilibrium with the potential.
  • A phase difference between high moon and high
    tide has been known for centuries. The high tide
    generally lags behind the high moon.

43
Tidal friction
  • If there were no dissipation in the Earth
    systems, tides would lie directly under MP
  • However, friction creates a delay in the tidal
    response.
  • The Earths surface reacts to the tidal potential
    due to MP with a lag. The tides peak 30 minutes
    later.

44
Altimetry Missions
  • Tidal Aliasing, the frequencies, periods, and
    amplitudes of the most significant tidal
    constituents

45
Altimetry Missions
  • Tidal Aliasing, the frequencies, periods, and
    amplitudes of the most significant tidal
    constituents

46
Altimetry Missions
  • In each cycle, the altimeter samples the phase of
    each tide.
  • A sun-synchronous altimeter sampling the S2
    constituent would find a frozen tide with an
    infinite aliasing period.
  • ERS-1, ERS-2, Envisat, and NPOESS all did this.
  • Otherwise, the change in phase of the tide during
    one repeat period T is
  • The primary alias period

47
Altimetry Missions
  • For Topex/Poseidons 9.916-day repeat period
    orbit, the primary alias periods are

48
Altimetry Missions
  • For Topex/Poseidons 9.916-day repeat period
    orbit, the primary alias periods are

Each of these is different by at least several
days
49
Altimetry Missions
  • If tidal aliasing does occur and/or the tidal
    frequencies or their aliasing frequencies
    overlap, there are ways to resolve the alias.
  • Use along-track data
  • Use cross-over points

50
Altimetry Missions
  • Spatial vs. Temporal Resolution

51
Altimetry Missions
  • Tide Gauges and Ground Track Placement

52
Altimetry Missions
53
Topex/Poseidons Options
  • 1335 km, 64.80 deg inclination
  • 1252 km, 62.01 deg inclination
  • 1255 km, 65.84 deg inclination
  • 1173 km, 62.69 deg
  • Option 1 first choice, Option 3 as backup if a
    frozen orbit is desired.
  • Topex/Poseidon was placed in an exact repeat
    groundtrack orbit with 127 revolutions per 10-day
    cycle.

54
ASEN 5050SPACEFLIGHT DYNAMICSConstellation
Design
  • Prof. Jeffrey S. Parker
  • University of Colorado Boulder

55
Constellation Designs
  • GPS
  • 6 circular orbits, 12-sidereal hour period, 55
    deg inclination
  • 4 satellites per orbit, evenly spaced over 360
    deg
  • Galileo, a Walker Delta 56 deg27/3/1
  • 3 orbital planes, 56 deg inclination
  • 9 satellites per orbit, evenly spaced over 360
    deg
  • Iridium, a near-polar Walker Star
  • 6 orbital planes, 86.4 deg inclination
  • 11 satellites per orbit, evenly spaced over 180
    deg

56
Constellation Designs
  • A-train (Afternoon Sun-Synch, coordinated)
  • BGAN
  • Compass Navigation system
  • Disaster Monitoring Constellation
  • Globalstar
  • GLONASS
  • Orbcomm
  • RapidEye
  • Sirius Satellite Radio
  • TDRSS
  • XM Satellite Radio

And others!
57
A-Train
  • Coordinated constellation of French, American,
    Japanese, Canadian satellites
  • Sun-Synch
  • 98.14 deg inclination
  • 130 pm solar time equatorial crossing
  • GCOM-W1 (SHIZUKU), JAXA
  • Aqua (4 min behind), USA
  • CloudSat (2.5 min behind), USA and CSA
  • CALIPSO (15 sec behind), CNES, USA
  • Aura (15 min behind Aqua)
  • PARASOL (now retired)
  • OCO-2

58
Compass / BeiDou-1
  • Chinese navigation system
  • Geostationary orbits
  • The area that can be serviced is from longitude
    70E to 140E and from latitude 5N to 55N.

59
BeiDou-2
  • Chinese navigation system
  • Supersedes BeiDou-1
  • 35 satellites, completed by 2020
  • 5 in geostationary orbit
  • 27 in MEO
  • 3 in inclined geosynch orbit
  • Plans for up to 75 or more satellites, covering
    urban canyons

60
GPS
  • 6 circular orbits, 12-sidereal hour period, 55
    deg inclination
  • 4 satellites per orbit, evenly spaced over 360
    deg

61
Disaster Monitoring Constellation
  • International, coordinated, Sun-Synch orbit
  • 1015 am local time Northward equator crossing

62
Globalstar
  • LEO
  • 50 satellites
  • Inclination 52 deg
  • 1400 km altitude
  • Communication, short latency
  • 5 ms 1-way light time.

63
Iridium
  • 66 active satellites
  • LEO 781 km altitude, inclination 86.4 deg
  • 11 satellites in each of 6 orbital planes
  • Iridium NEXT 2nd generation communication system
  • 66 more satellites, launched 10 at a time on
    Falcon 9 launches

64
Orbcomm
  • 29 satellites
  • LEO 775 km altitude
  • Telecommunication system

65
RapidEye
  • German geospatial information provider.
  • 5 satellites in the same orbital plane.
  • Altitude 630 km
  • Sun-synchronous, 1100 am ascending time, 97.8
    deg inclination

66
Sirius
  • 3 satellites
  • Highly elliptical, geosychronous orbits (Tundra
    orbits)
  • Each satellite spends 16 hours over the
    continental US per orbit.
  • XM Satellites 2 geostationary satellites.

67
TDRSS
  • Tracking and Data Relay Satellite System
  • A dozen GEO satellites some equatorial and some
    just off of the equator.
  • Navigation and communication, largely of NASAs
    assets.

68
Announcements
  • STK Lab 3 due Friday 12/5
  • Any issues with v9 versus v10?
  • STK Lab 4 due 12/12
  • Any issues with v9 versus v10?
  • Final Exam on 12/12, due 12/18
  • Take-home, open book open notes
  • Final project and exam due 12/18
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