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Columbia launches from LC-39B
|Mission type||Satellite deployment|
|Mission duration||4 days, 22 hours, 50 minutes, 18 seconds|
|Distance travelled||2,890,000 kilometers (1,800,000 mi)|
|Spacecraft||Space Shuttle Columbia|
|Launch mass||122,536 kilograms (270,146 lb)|
|Landing mass||99,783 kilograms (219,984 lb)|
|Payload mass||22,781 kilograms (50,224 lb)|
|Members||Eileen M. Collins
Jeffrey S. Ashby
Steven A. Hawley
Catherine G. Coleman
|Start of mission|
|Launch date||23 July 1999, 16:31UTC|
|Launch site||Kennedy LC-39B|
|End of mission|
|Landing date||28 July 1999, 03:20UTC|
|Landing site||Kennedy SLF Runway 33|
|Perigee||260 kilometres (160 mi)|
|Apogee||280 kilometres (170 mi)|
STS-93 marked the 95th launch of the Space Shuttle, the 26th launch of Columbia, and the 21st night launch of a Space Shuttle. Eileen Collins became the first female shuttle Commander on this flight. Its primary payload was the Chandra X-ray Observatory. It would also be the last mission of Columbia until March 2002. During the interim, Columbia would be out of service for upgrading, and would not fly again until STS-109. The launch was originally scheduled for 20 July but the launch was aborted at T-8 seconds. The successful launch of the flight occurred three days later.
|Commander||Eileen M. Collins
|Pilot||Jeffrey S. Ashby
|Mission Specialist 1||Steven A. Hawley
|Mission Specialist 2||Catherine G. Coleman
|Mission Specialist 3||Michel Tognini, CNES
Problems during ascent
During STS-93 ignition sequence, a gold pin used to plug an oxidizer post in the Space Shuttle's number three or right engine came loose and was violently ejected, striking the engine nozzle's inner surface and tearing open three cooling tubes containing hydrogen. These ruptures resulted in a small leak downstream of the main combustion chamber. This anomalous event and the automatic response to the leak by the engine's controller did not violate any launch commit criteria and liftoff proceeded normally. However, approximately five seconds after liftoff, an electrical short disabled one primary and one secondary controller on two of the three main engines. In response to this failure, the engines automatically switched to their backup controllers. (The short was later discovered to have been caused by poorly routed wiring which had rubbed on an exposed screw head. This wiring issue led to a program-wide inspection of the wiring in all orbiters.) Because of the leak in the right engine, its controller sensed a decrease in thrust or power--measured indirectly as main combustion chamber pressure--since the leaking hydrogen was not being burned in the SSME's two pre-burners or the main combustion chamber. To bring the engine back up to the commanded thrust level, the controller opened the oxidizer values a bit more than normal. The hydrogen leak and increased oxidizer flows resulted in the right engine being forced away from the desired hydrogen/oxygen mixing ratio of 6.03 and ran hotter than normal due to the mixture being closer to the stoichiometric ratio of 8:1. The increased oxidizer consumption during ascent resulted in a premature shutdown of all three engines near the end of the projected burn due to low liquid oxygen level sensed in the External Tank. Despite the premature shutdown, the vehicle safely achieved orbit and was able to complete the mission as planned. This incident brought on a maintenance practice change which required damaged oxidizer posts to be removed and replaced as opposed to being intentionally plugged, as was the practice beforehand.
Three days previously, in the first launch attempt, the launch was stopped at T-0:08 seconds, just prior to the SSMEs' ignition sequence, due to a senior console operator manually triggering a cutoff in the countdown. It was later determined that the console operator, monitoring the hydrogen gas concentration in the Space Shuttle's aft compartment where the three SSMEs where located, was fooled by the gas detector's purge cycle which generated a dangerously high, but spurious, reading in the last seconds of the countdown.
The primary objective of the STS-93 mission was to deploy the Chandra X-ray Observatory (formerly the Advanced X-ray Astrophysics Facility) with its Inertial Upper Stage booster. At its launch, Chandra was the most sophisticated X-ray observatory ever built. It is designed to observe X-rays from high energy regions of the universe, such as hot gas in the remnants of exploded stars.
Other payloads on STS-93 included the Midcourse Space Experiment (MSX), the Shuttle Ionospheric Modification with Pulsed Local Exhaust (SIMPLEX), the Southwest Ultraviolet Imaging System (SWUIS), the Gelation of Sols: Applied Microgravity Research (GOSAMR) experiment, the Space Tissue Loss – B (STL-B) experiment, a Light mass Flexible Solar Array Hinge (LFSAH), the Cell Culture Module (CCM), the Shuttle Amateur Radio Experiment – II (SAREX – II), EarthKAM, Plant Growth Investigations in Microgravity (PGIM), the Commercial Generic Bioprocessing Apparatus (CGBA), the Micro-Electrical Mechanical System (MEMS), and the Biological Research in Canisters (BRIC).
The Shuttle Ionespheric Modification with Pulsed Local Exhaust (SIMPLEX) payload activity researched the source of Very High Frequency (VHF) radar echoes caused by the orbiter and its OMS engine firings. The Principal Investigator (PI) used the collected data to examine the effects of orbital kinetic energy on ionospheric irregularities and to understand the processes that take place with the venting of exhaust materials.
The Southwest Ultraviolet Imaging system (SWUIS) was based around a Maksutov-design ultraviolet (UV) telescope and a UV-sensitive, image-intensified Charge-Coupled Device (CCD) camera that frames at video frame rates. Scientists can obtain sensitive photometric measurements of astronomical targets.
The objective Gelation of Sols: Applied Microgravity Research (GOSAMR) experiment was to investigate the influence of microgravity on the processing of gelled sols. In particular, the purpose was to demonstrate that composite ceramic precursors composed of large particulates and small colloidal sols can be produced in space with more structural uniformity.
The focus of the Space Tissue Loss – B (STL-B) experiment was direct video observation of cells in culture through the use of a video microscope imaging system with the objective of demonstrating near real-time interactive operations to detect and induce cellular responses.
The Light mass Flexible Solar Array Hinge (LFSAH) payload consists of several hinges fabricated from shape memory alloys. Shape memory deployment hinges offered controlled shockless deployment of solar arrays and other spacecraft appendages. LFSAH demonstrated this deployment capability for a number of hinge configurations.
The objectives of the Cell Culture Module (CCM) were to validate models for muscle, bone, and endothelial cell biochemical and functional loss induced by microgravity stress; to evaluate cytoskeleton, metabolism, membrane integrity and protease activity in target cells; and to test tissue loss medications.
The Shuttle Amateur Radio Experiment (SAREX-II) demonstrated the feasibility of amateur short-wave radio contacts between the shuttle and ground-based amateur radio operators. SAREX also served as an educational opportunity for schools around the world to learn about space by speaking directly to astronauts aboard the shuttle via amateur radio.
The EarthKAM payload conducted Earth observations using the Electronic Still Camera (ESC) installed in the overhead starboard window of the Aft Flight Deck.
The Plant Growth Investigations in Microgravity (PGIM) payload experiment used plants to monitor the space flight environment for stressful conditions that affect plant growth. Because plants cannot move away from stressful conditions, they have developed mechanisms that monitor their environment and direct effective physiological responses to harmful conditions.
The Commercial Generic Bioprocessing Apparatus (CGBA) payload hardware allows for sample processing and stowage functions. The Generic Bioprocessing Apparatus – Isothermal Containment Module (GBA-ICM) is temperature controlled to maintain a preset temperature environment, controls the activation and termination of the experiment samples, and provides an interface for crew interaction, control and data transfer.
The Micro-Electrical Mechanical System (MEMS) payload examines the performance, under launch, microgravity, and reentry conditions of a suite of MEMS devices. These devices include accelerometers, gyroscopes, and environmental and chemical sensors. The MEMS payload is self-contained and requires activation and deactivation only.
The Biological Research in Canisters (BRIC) payload was designed to investigate the effects of space flight on small arthropod animals and plant specimens. The flight crew was available at regular intervals to monitor and control payload/experiment operations.
Columbia's landing at Kennedy Space Center marked the twelfth night landing in the Shuttle program's history. Five had been at Edwards Air Force Base in California and the rest KSC. To date, there had been 19 consecutive landings at KSC and 25 of the last 26 had been there.
|Attempt||Planned||Result||Turnaround||Reason||Decision point||Weather go (%)||Notes|
|1||20 Jul 1999, 12:36:00 am||scrubbed||---||excessive hydrogen detected||(T-0:07)|
|2||22 Jul 1999, 12:28:00 am||scrubbed||1 day, 23 hours, 52 minutes||weather|
|3||23 Jul 1999, 12:24:00 am||success||0 days, 23 hours, 56 minutes|
In 2001, Coin World reported the revelation (via a FOIA document request) that the Mint had struck 39 examples of the 2000 Sacagawea dollar in gold in June 1999 at the West Point Mint. The planchets came from specially prepared ½ troy-oz $25 American Gold Eagle Bullion Planchets. Why they were struck is not known; speculation is that this was an attempt by the mint to offer "Premium" collectibles in conjunction with the newly released Sacagawea dollar in 2000.
Twenty-seven were soon melted and the remaining 12 were on board Space Shuttle Columbia for the July 1999 STS-93 mission. Two examples then popped up at two separate events; one during a Private Congressional Dinner in August 1999, and another example at the Official First-Strike ceremonies in November. The coins remained at Mint Headquarters under lock and key until they were transferred in 2001 to Fort Knox. The strikes are considered to be illegal due to the Coinage regulations in place.
In 2007, the Mint announced  it would for the first time publicly display the 12 space-flown gold dollars at the American Numismatic Association's World's Fair of Money in Milwaukee, WI.
Sleeping shuttle astronauts were often awakened with a short piece of music, a tradition that apparently began during Apollo 15. Each track was specially chosen, sometimes by their families, and usually had a special meaning to an individual member of the crew, or was applicable to their daily activities.
|Day 2||"Beep Beep"||Louis Prima||wav[dead link] mp3[dead link]
|Day 3||"Brave New Girls"||Teresa||wav[dead link] mp3[dead link]
|Day 4||"Someday Soon"||Suzy Bogguss||wav[dead link] mp3[dead link]
|Day 5||"The Sound of Silence"||Simon and Garfunkel||wav[dead link] mp3[dead link]
|Day 6||"A Little Traveling Music"||Barry Manilow||wav[dead link] mp3[dead link]
- Greene, William D. "Inside The J-2X Doghouse: Engine Control — Open versus Closed Loop". Liquid Rocket Engines (J-2X, RS-25, general). NASA. Retrieved 22 October 2014.
- Hale, Wayne. "STS-93: Keeping Eileen on the Ground, Part 1". http://waynehale.wordpress.com/. Retrieved 22 October 2014.
- Four Nerve-Racking Space Shuttle Launch Aborts
- Fries, Colin (20 April 2010). "Chronology of Wakeup Calls" (PDF). NASA. Retrieved 24 May 2010.
- NASA (11 May 2009). "STS-93 Wakeup Calls". NASA. Retrieved 31 July 2009.
- NASA PAO page about STS-93
- STS-93 Archives
- STS-93 Video Highlights
- "US Mint to show unseen gold space coins". collectSPACE. http://www.collectspace.com/news/news-071407a.html. Retrieved 2007-07-16.]
- STS-93 JSC Ascent Audio