Celestial Mechanics - Low Orbiting Satellites
A predominant section of Celestial Mechanics is the satellite visualization sections. The image below was generated from the orbits of Low Orbiting Satellites of the Earth, based on data from SSR's (Satellite Situation Reports) collected from the public domain that date from 1994 to the present. Our viewpoint is as if we are standing on the surface of the earth, roughly around the Los Angeles area, looking skyward.
In order to generate the image, the data was parsed into MEL, a scripting language used by the 3D animation program Maya, which was then rendered into animation frames. The animation was then sped up to roughly 500x, so the viewer is exposed to the sheer scope of objects that are constantly in orbit. The average speed of an LEO satellite is 17,000 MPH, and the average size is between 1 and 2 meters across. Their functions vary from observation, to data collection, to communication, to military usage. The rings visible in this particular visualization are the satellites' line of site ring, which is the elliptical area of the Earth's surface that each satellite can "see". When each line of site ring is rendered, it is possible to see the scope of observation that is taking place.
Below is a still from an animation generated from data in SSR's from June to November, 2005, and a handful of interesting satellites that are currently above the earth. Click the image to toggle the listed satellite locations. Even though they are among hundreds others, the short list of individual satellites shows you many unique functions.
These satellites are chosen at random, they are listed only to illustrate variety. Their statistics are pulled from an SSR that was taken in June, 2005. You may download the SSR in the Downloads section. The satellite information was referenced from various public domain sources.
------------------------------------------------------------------------------- INT-ID/Name CATALOG# SOURCE PERIOD INCL APOGEE PERIGEE RCS -------------------------------------------------------------------------------
ORBVIEW 1 (MICROLAB), launched 04/03/1995 1995-017b 23546 orb 98.6 70.0 701 684 1.2886
Description
Microlab 1 is a minisatellite that was launched by a Pegasus rocket carried aloft by an
L-1011 aircraft flying out of Vanderberg AFB. The main instrument is a global lightning
mapper; the other is a radio receiver to monitor the transmission from any GPS spacecraft
that appears near the horizon and to infer the atmospheric temperature and humidity, and
the ionospheric total electron content along the path between the GPS and Microlab
spacecraft.
Dicipline
Earth Science, Space Physics
WESTPAC, launched 07/10/1998 1998-043d 25397 isra 101.2 98.5 815 814 0.1853
Description
Formerly known as WPLTN-1, Westpac was an Australia geodetic satellite for the joint
venture between Australia's Electro Optics and the Russian Space Agency. It was spherical in
shape with laser reflectors. It served as a target for the Western Pacific Laser Tracking Network.
Dicipline
Earth Science
IRIDIUM 17, launched 07/09/1997 1997-034a 24869 us 100.4 86.4 779 776 5.8569
Description
Iridium 17 was part of a planned commercial communications network
comprised of a constellation of 66 LEO spacecraft. The system uses L-Band
to provide global communications services through portable handsets. A total
of 125 spacecraft were built by Lockheed for more than $700M. Commercial
service began in 1998. The system employs 15-20 ground
stations with a master control complex in Landsdowne, VA, a backup in Italy,
and a third engineering center in Chandler, AZ. The spacecraft was 3-axis
stabilized, with a hydrazine propulsion system. It had 2 solar panels with
1-axis articulation. The system employed L-Band using FDMA/TDMA to provide
voice at 4.8 kbps and data at 2400 bps with 16 dB margin. Each satellite
had 48 spot beams for Earth coverage and used Ka-Band for crosslinks and
ground commanding.
Dicipline
Communications
TRMM, launched 11/27/1997 1997-073b 25062 us 90.1 28.5 284 278 n/a
Description
The Tropical Rainfall Measuring Mission (TRMM) is a joint mission
between NASA and the Japan Aerospace Exploration Agency (JAXA)
designed to monitor and study rainfall over the global tropics and
subtropics. The launch vehicle is provided by Japan and
the satellite by NASA. The TRMM spacecraft is planned to be a free-flyer launched
on an expendable Japanese HII rocket with a low-altitude, non-sun-synchronous orbit.
The orbital position of the spacecraft is determined
by the TDRSS ranging system. The minimum mission life for TRMM is three years. See
http://trmm.gsfc.nasa.gov for more information
Dicipline
Earth Science
UNISAT 2, launched 12/20/2002 2002-058c 27607 saud 97.9 64.6 716 600 0.0832
Description
Unisat is a 12kg, Italian Picosat that was launched from Baikonur by a Dnepr rocket on the Dec/20/2002. It
carries a camera and sensors for picking up debris and aerosol.
Dicipline
Engineering
NOAA 16 DEB, launched 09/21/2000 2002-037g 27476 cis 119.8 63.5 1883 1464 0.6095
Description
NOAA 16 continues the fourth-generation of operational, polar orbiting,
meteorological satellite series (NOAA K-N) operated by the National Environmental Satellite
Service (NESS) of the National Oceanic and Atmospheric Administration (NOAA).
The goal of the NOAA/NESS polar orbiting program is to provide output products used in meteorological
prediction and warning, oceanographic and hydrologic services, and space environment
monitoring. The spacecraft power is provided by a direct energy transfer system from the
single solar array which is comprised of eight panels of solar cells.
Dicipline
CHAMP, launched 07/15/2000 2000-039a 26404 it 87.2 87.2 143 128 2.6401
Description
CHAMP (CHAllenging Minisatellite Payload) is a German environmental research
minispacecraft that carries instruments for collecting geophysical, oceanographic, and
meteorological data. The 500 kg, triaxially stabilized spacecraft was launched by a
Kosmos-3M rocket from Plesetsk with two other satellites.
Dicipline
Earth Science
HETE 2, launched 10/09/2000 2000-060b 26560 fr 89.1 7.9 359 102 29.8363
Description
The High Energy Transient Explorer 2 (HETE-2) is designed to detect
cosmic gamma-ray bursts (GRBs) and help determine their origin and nature.
The goal of the mission is to continuously scan the sky and identify occurences of GRBs,
establish precise locations and transmit coordinates
in near real time. The instruments are also used to establish relative
GRB rates and intensities in the soft X-ray, mid X-ray, and gamma-ray bands, perform
spectroscopy of gamma-ray bursts, measure the intensities,
time histories, and spectra of soft gamma-ray repeater bursts, X-ray bursts, and black
hole X-ray transients.
The spacecraft is basically a rectangular cube, roughly one meter by half a meter
by half a meter, with four solar panel petals protruding from the bottom. The bottom
section of the spacecraft holds the power, communications, and attitude control and the
upper section the science instruments. Power is supplied by the solar panels, which are
made of honeycomb aluminum with a silicon substrate.
Attitude control is achieved by a
momentum wheel and three orthogonal magnetic torque coils, controlled by inputs from
two magnetometers, twelve sun sensors, and an optical camera.
HETE-2 is placed in a 592 km x 640 km elliptical Earth orbit. The spacecraft
always points in the anti-solar direction and all bursts detected will be at least
120 degrees from the Sun. The field of view will be centered roughly on the ecliptic.
Over the course of a year approximately 60% of the sky will be surveyed. When GRB's
are detected, summary burst data are sent immediately to listen-only equatorial ground
stations and are forwarded to observers via the GRB coordinates network within less
than 10 seconds of burst detection. The planned operating life is 18 months with
probable mission extensions for an additional 6 months or more.
Dicipline
Astronomy
CUTE-1, launched 06/30/2003 2003-031d 27843 ca 101.4 98.7 833 817 0.3909
Description
CUTE 1 is a Japanese (Tokyo Institute of Technology) one kilogram nanosatellite
that was launched by a Rokot rocket from Plesetsk on 30 June 2003.
Dicipline
Technology Applications
OSCAR 29, launched 09/16/1987 1987-080a 18361 us 107.1 90.2 1176 1013 1.2421
Description
OSCAR 29 was a US Navy navigation satellite launched by a Scout G rocket.
Transit, one of the first operational satellite systems, was also known as the
Navy Navigation Satellite (NNS).
The Transit spacecraft were developed for updating the inertial navigation
systems on board US Navy Polaris submarines, and later for civilian use.
Transit receivers used the known characteristics of the satellite's orbit, measured
the Doppler shift of the satellite's radio signal, and thereby calculated the
receivers position on the earth. As a single spacecraft travelled overhead,
the user measured the Doppler shift over a 15 minute period by receiving
timing marks and satellite orbital information on two separate frequencies,
149.99 and 399.97 MHz. These signals were corrected for ionospheric refraction
and the information was then fed into the users navigation system.
Individual Transit satellites operated for over 10 years. Technical break- throughs
during the program included gravity gradient stabilization, the use of radio-isotope
thermoelectic generators (RTG), and navigation satellite technologies later used in
the GPS system. Transit was superseded by the Navstar global positioning system. The
use of the satellites for navigation was discontinued at the end of 1996 but the
satellites continued transmitting and became the Navy Ionospheric Monitoring System (NIMS).
Dicipline
Navigation & Global Positioning
WIRE, launched 03/05/1999 1999-010d 25645 cis 1468.7 5.2 36501 36343 1.3609
Description
The Wide-field Infrared Explorer (WIRE) was a two-color, solid hydrogen-cooled,
infrared imaging telescope designed to study starburst galaxies and to search for protogalaxies.
The science goals of WIRE were to: (1) determine what fraction of the luminosity of the universe
at a redshift of >0.5 is due to starburst galaxies; (2) assess how fast and in what ways starburst
galaxies evolve; and, (3) examine whether luminous protogalaxies are common at redshifts <3.
In order to accomplish these goals, WIRE was to conduct a four month survey at 12 and 25
micrometers over an area of between ten and several hundred square degrees of the sky.
The WIRE telescope itself had an entrace aperture of 30 cm and a 32 x 32 arc-minute field of
view.
Shortly after launch, while the spacecraft was still tumbling early after orbit insertion,
the telescope cover came off prematurely. This resulted in the exposure of the cryogenic
materials to light, warming them at a high rate causing outgassing and increasing the rate
of spin of the spacecraft beyond the ability of the reaction wheels to slow it. Although
ground controllers began work to decrease the excess spin of the spacecraft, they were not
able to do so in time to prevent the total loss of the frozen hydrogen used to cool the
primary science instrument. Attempts to recover control of the spacecraft were successful,
though as a result of the coolant loss, science data was not obtainable.
Dicipline
Astronomy
MOS 1A (MOMO 1), launched 02/19/1987 1987-017b 17526 cis 104.6 82.9 1007 946 5.2732
Description
The Marine Observation Satellite (MOS-1) was Japan's first earth observation satellite.
The three-axis stabilized spacecraft carried a Multispectral Electronic
Self-scanning Radiometer (MESSR) that collected data from both land and sea,
a Visible and Thermal Infrared Radiometer (VTIR) to measure sea surface
temperature, a Microwave Scanning Radiometer (MSR) to provide information
on sea ice, snowfall, water vapor content at the ocean and in the atmosphere,
and a Data Collection System (DCS) transponder to collect observation data
from drifting buoys. The spacecraft had a box-type shape with deployable solar
panels. It was composed of two cubes, a bus module and a mission module, on
which the three sensors were mounted. The spacecraft followed a sun-synchronous
orbit with equatorial crossings in the descending node maintained between 10:00
a.m. and 11:00 a.m. local time. The mission life was designed to be 2 years.
Dicipline
Earth Science
ROCSAT 2, launched 05/20/2004 2004-017b 28253 us 478.8 12.0 27592 201 17.0990
Description
Rocsat 2 is a Taiwanese (ROC) remote sensing satellite that was launched
from Vandenberg AFB by a Taurus XL rocket at 17:47 UT on 19 May 2004. The 750 kg
satellite carries imaging instruments to take pictures of crop yields in Taiwan,
natural disasters, and oil spills on land and ocean, and to image high altitude
red lightning strokes called sprites.
Dicipline
Earth Science
TRANSAT, launched 10/28/1977 1977-105b 10456 cis 87.8 62.8 183 152 n/a
Description
Transit-O 11 was a US Navy navigation satellite launched by a Scout D rocket, and is part of the Transit
Network. (See Number 10).
Individual Transit satellites operated for over 10 years. Technical break- throughs
during the program included gravity gradient stabilization, the use of radio-isotope
thermoelectic generators (RTG), and navigation satellite technologies later used in
the GPS system. Transit was superseded by the Navstar global positioning system.
The use of the satellites for navigation was discontinued at the end of 1996 but
the satellites continued transmitting and became the Navy Ionospheric Monitoring
System (NIMS).
Dicipline
Navigation & Global Positioning
EO 1, launched 11/21/2000 1975-017c 26618 us 91.7 63.1 605 107 1.9752
Description
EO 1 (Earth Observing mission 1) is the first spacecraft in the American
New Millennium Program (NMP) and was launched by a Delta 2 rocket from Vandenberg
AFB. The 573 kg spacecraft carries three well-developed instruments
(and seven technology-test items) to image Earth's surface in numerous wavelength
bands. The Hyperion is a grating-imaging spectrometer and will image the surface i
n 220 spectral bands covering 0.4-2.5 micron wavelengths at a resolution of 30
meters. It is expected to provide better crop estimates, and better mineral
resource areas than are being provided by Landsat 7. The Advanced Land Imager
(ALI) is a wide field (15 deg x 1.26 deg) reflective optics telescope that will
provide images in 10 wavelength bands covering 0.4-2.4 microns with a spatial
resolution of 30 meters. It is designed to produce images that are directly
comparable to the ones from the ETM+ (Enhanced Thematic Mapper Plus) instrument
on board Landsat 7, and thus provide continuity of data. The third instrument,
LAC (LEISA Atmospheric Corrector) covers the 0.890-1.600 micron wavelength IR
band by means of a wedged etalon filter and three arrays (256 x 256) of In-Ga
detectors, each array covering a five deg swath width with a spatial resolution
of 250 meters. It will aid in correcting the data from the other instruments for
water vapor and cirrus cloud variations. Among the new technology test/demonstration
items is the XPAA (X-band Phased Array Antenna) with 64 elements powered by a 160 W
transmitter that sends data at a rate of 105 MB per second. Additional information on
EO 1 can be obtained from
http://eo1.gsfc.nasa.gov/.
Dicipline
Earth Science
MAROC TUBSAT, launched 12/10/2001 2001-056c 27003 paki 105.1 99.5 1014 985 0.3536
Description
Maroc-Tubsat is a Moroccan microsatellite that was launched by a Zenit rocket from
Baikonur on Dec/10/2001. Its mission was to test a 3-dimensional attitude control system that will be incorperated
in a future remote sensing mission.
Dicipline
Engineering
COBE, launched 11/18/1989 1989-088b 20321 cis 87.8 64.8 186 147 n/a
Description
The purpose of the Cosmid Background Explorer (COBE) satellite mission was to take precise measurements
of the diffuse radiation over the Earth. The experiment module contained the instruments and a container filled with 650 litres
of liquid helium, wich a conical sun shade. The satellite rotated at 1rpm around the axis of symmetry to control systematic
errors in the anisotropy measurements, and to allow observations of the zodiacal light at various
solar elongation angles. With this orbit and spin-axis orientation, the instruments performed a complete scan of the celestial
sphere every six months. Instrument operations were terminated in 1993, and the satellite has been converted into a test satellite.
Dicipline
Astronomy
Downloads
SSR from June, 2005 supplied by Peterson Air Force Base, CO. SSR_2005.TXT (4,426 kb)
Parsed SSR, listing only currently active satellites for June, 2005. LEOs_parse.txt (1,111 kb)
Large JPEG image of the satellite visualization. JPEG Image (1400x1400, 1,549 kb)
Large TGA image of the satellite visualization. Targa Image(1400x1400, 5,880 kb)
Satellite Tracking Resources
space-track.org - The source of our SSR's for this project
FreeFall - Satellite tracking software
Introduction to Visual Satellite Observing - Informative article by Jeff Hunt
Visually Observing Satellites - Useful links from Ed Cannon
dransom.org - A great Space Shuttle and satellite tracking resource
http://users2.ev1.net/~mmccants/ - Satellite Tracking for Austin TX