In its collecting configuration, the Genesis spacecraft exposed several types of solar wind collectors, as well as ion and electron monitors.
|Operator||NASA / JPL|
|Major contractors||Lockheed Martin Space Systems|
|Mission type||Sample return|
|Launch date||2001-08-08, 16:13:40 UTC
(11 years, 9 months, and 9 days ago)
|Launch vehicle||Delta II 7326|
|Launch site||Space Launch Complex 17A
Cape Canaveral Air Force Station
|Mission duration||December 3, 2001 –
April 22, 2004
( 2 years, 5 months, and 19 days)
(currently in sleep mode)
|Satellite of||Earth L1, Sun|
|Landing site||Dugway Proving Ground (crashed)|
|Mass||494 kg (1,090 lb)|
|Power||254.0 W (Solar array / Ni-H2 batter)|
|Spectral band||GE-2, Trans. 9, C-band|
Genesis was a NASA sample return probe which collected a sample of solar wind and returned it to Earth for analysis. It was the first NASA sample return mission to return material since the Apollo Program, and the first to return material from beyond the orbit of the Moon. Genesis was launched on August 8, 2001, and crash-landed in Utah on September 8, 2004, after a design flaw prevented the deployment of its drogue parachute. The crash contaminated many of the sample collectors, and although most were damaged, many of the collectors were successfully recovered.
The Genesis science team demonstrated that some of the contamination could be removed or avoided, and that the solar wind could be analyzed using a variety of approaches. It is relatively easy to detect the solar wind, but the precision measurements are difficult and techniques are still being refined in laboratories worldwide. Nonetheless, in March 2008 scientists stated that they believed that all of the mission's major science objectives would be achieved successfully.
The mission’s primary science objectives, as paraphrased from the original proposal fact sheet, were:
- To obtain precise solar isotopic abundances of ions in the solar wind, as essentially no data having a precision sufficient for solving planetary science problems are available;
- To obtain greatly improved solar elemental abundances by factor of 3-10 in accuracy over what is in the literature;
- To provide a reservoir of solar matter for 21st century science to be archived similarly as the lunar samples.
Note that the mission's science objectives refer to the composition of the Sun, not that of the solar wind. Scientists desire a sample of the Sun because evidence suggests that the outer layer of the Sun preserves the composition of our early solar nebula. Therefore, knowing the elemental and isotopic composition of the outer layer of the Sun is effectively the same as knowing the elemental and isotopic composition of our nebula. We could then use that data to model how planets and other solar-system objects formed and then extend those results to understanding stellar evolution and the formation of solar systems elsewhere in the universe.
Clearly, the ideal scientific option would be to send a spacecraft to the Sun itself and collect some solar plasma; however, obtaining solar matter is difficult because of the intense heat of the Sun’s superheated gases, as well as the dynamic electromagnetic environment of the solar corona, whose flares regularly interfere with the electronics of distant spacecraft. Fortunately, the Sun continuously sheds some of its outer layer in the form of solar wind, and data collected prior to the Genesis mission suggests that the rock-forming elements are thought to maintain their relative proportions throughout the process of solar wind formation.
Accordingly, in order to meet the mission science objectives, the Genesis spacecraft was designed to collect solar wind ions and return them to Earth for analysis. Genesis carried several different solar-wind collectors, all of which passively collected solar wind; that is, the collectors sat in space facing the sun, while the ions in the solar-wind crashed into them at speeds over 200 km/s and, on impact, buried themselves in the surface of the collectors. This passive collection is a process similar to that used by the semi-conductor industry to make certain types of devices, and a simulation of the process is given by the free-access program SRIM.
Most of the Genesis collectors continuously sampled all of the solar wind which the spacecraft encountered (the "bulk solar wind"). However, the spacecraft also carried three arrays of collectors which were deployed when specific “regimes” (fast, slow, coronal mass ejections) of solar wind were encountered, as determined by the electron- and ion- monitors on board. These deployable collector arrays were designed to provide data to test the hypothesis that the rock-forming elements keep their relative proportions throughout the processes which form the solar wind.
There was a third type of collector on Genesis: the concentrator, which collected bulk solar wind, but was discriminating in that it electrostatically repelled hydrogen and had enough voltage to focus the lighter solar wind elements onto a small target, concentrating those ions by a factor of ~20. The objective of the concentrator was to bring back a sample with enhanced amounts of solar wind ions to make it possible for analysts to precisely measure the isotopes of the light elements.
Mission profile 
Genesis was a Discovery-class mission of the NASA Jet Propulsion Laboratory (JPL) at the California Institute of Technology. The spacecraft was designed and built by Lockheed Martin Space Systems at a total mission cost of US$264 million.
NASA launched the craft on a Delta II 7326 rocket on August 8, 2001 at 16:13:40 UTC from Cape Canaveral. Following launch, Genesis cruised to the Earth-Sun L1 then performed a Lissajous orbit insertion maneuver, entering an elliptical orbit about L1 on November 16, 2001. Genesis exposed its collector arrays on 3 December, and began collecting solar wind particles. The collection process ended after 850 days, on April 1, 2004, with the spacecraft completing five halo loops around L1. Genesis began its return to Earth on April 22, 2004. The return phase included an orbital detour toward the Earth L2 so that the craft could be recovered during the daytime, as a direct approach would have forced it to be recovered at night. After completing one halo loop about L2, the spacecraft returned to Earth for a planned September 8, 2004 recovery.
Recovery phase 
Following completion of the collection phase, the collector arrays were stowed in a sample return capsule, and the spacecraft returned to Earth. As the capsule was approaching Earth and at the first stages of re-entry, all appeared well.
Extensive planning had been conducted for the capsule's retrieval. A normal parachute landing might have damaged the delicate samples, so the mission design called for a mid-air retrieval of the sample return capsule. About 33 km above the ground, a drogue parachute was to be deployed to slow descent. Then, at a height of 6.7 km, a large parafoil was to be deployed to slow descent further and leave the capsule in stable flight. A helicopter, with a second helicopter as a backup, was then to attempt to catch the capsule by its parachute on the end of a five-meter hook. Once retrieved, the capsule would have been soft-landed.
The sample return capsule entered Earth's atmosphere over northern Oregon at 16:55 UTC September 8, 2004, with a velocity of approximately 11.04 km/s (24,706 mph). Due to a design flaw in a deceleration sensor, parachute deployment was never triggered, and the spacecraft's descent was slowed only by its own air resistance. The planned mid-air retrieval could not be carried out, and the capsule crashed into the desert floor of the Dugway Proving Ground in Tooele County, Utah, at about 86 metres per second (311 km/h (193 mph)).
The capsule broke open on impact, and part of the inner sample capsule was also breached. The damage was less severe than might have been expected given its velocity; it was to some extent cushioned by falling into fairly soft muddy ground.
Sample extraction and results 
Unfired pyrotechnic devices in the parachute deployment system and toxic gases from the batteries delayed the recovery team’s approach to the crash site. After all was made safe, the damaged sample-return capsule was secured and moved to a clean room for inspection; simultaneously a crew of trained personnel scoured the site for collector fragments and sampled the local desert soil to archive as a reference by which to identify possible contaminants in the future. Recovery efforts by Genesis team members at the Utah Test and Training range – which included inspecting, cataloging and packaging various collectors — took four weeks.
Initial investigations showed that some wafers had crumbled to dust on impact, but others were largely intact. Desert dirt entered the capsule, but not liquid water. Because the solar wind particles were expected to be embedded in the wafers, whereas the contaminating dirt was thought likely just to lie on the surface, it was thought possible to separate the dirt from the samples.
The analysis team hoped to extract some useful data from the capsule. Roger Wiens, of the Los Alamos National Laboratory stated on September 10, 2004 that because much of the inner canister was still intact, and despite serious contamination, "We should be able to meet many, if not all, of our primary science goals". On September 21, 2004 the extraction was said to be going well, with wafer fragments beginning to be extracted from the science canister. NASA announced on January 27, 2005, that a first sample piece of an aluminum wafer was sent to scientists at Washington University in St. Louis for analysis.
On April 20, 2005, NASA announced that scientists at the Johnson Space Center in Houston had removed the four solar-wind collectors from an instrument called the concentrator and found them in excellent shape. The concentrator's targets collected solar-oxygen ions during the mission and would be analyzed to measure solar-oxygen isotopic composition, the highest-priority measurement objective for Genesis.
After three years, scientists at Washington University published detailed neon and argon isotope fractionation findings. Argon and neon isotopes in samples of three types of solar wind (fast, slow, and coronal mass ejections from the Sun’s surface) were captured and quantified. The findings effectively discount some theoretical models of stellar genesis.[clarification needed] This more precise data complements knowledge gained from earlier lunar argon measurements.
Kevin McKeegan, UCLA Cosmochemistry Professor, announced on 10 March 2008 that analysis of a silicon wafer from Genesis showed that the Sun has a higher proportion of oxygen-16 than does the Earth. The measurement was made after a beam of cesium atoms was used to remove the upper 20 nm of the wafer. This implies that an unknown process depleted oxygen-16 from the Sun's disk of protoplanetary material prior to the coalescence of dust grains that formed the Earth.
Unexpectedly, it was not terrestrial desert soil introduced in the crash that proved most difficult to deal with during the sample analysis process but the craft's own flight-introduced compounds such as lubricants and craft-building materials.
Fate of spacecraft bus 
After releasing the sample return capsule on September 8, 2004, the spacecraft bus traveled back toward the Earth-Sun Lagrange Point (L1). A trajectory correction maneuver was performed on November 6, 2004, permitting the spacecraft bus to eventually leave L1 if it was not used for an extended mission. Final commands were transmitted to the bus on December 2, 2004, placing Genesis into hibernation. While in this "safe" mode, it will continue transmitting information about its condition, autonomously pointing its solar arrays toward the Sun. The spacecraft bus left L1 around February 1, 2005, staying in a heliocentric orbit leading the Earth.
Mishap Investigation Board (MIB) 
A 16-member NASA Mishap Investigation Board (MIB) was appointed, including experts on pyrotechnics, avionics, and other specialties. The MIB started its work on September 10, 2004, when it arrived at Dugway Proving Ground. It determined that all scientific hardware meant to be curated by the Johnson Space Center could be released and were not needed for the work of the board. Both JPL and Lockheed Martin began to prepare flight data and other records for the MIB.
It was announced[who?] on September 23, 2004, that the capsule, having had the science material extracted, would be moved to the Lockheed Martin Space Systems facility near Denver, Colorado, for MIB use.
A first possible root cause of the failed deployment of the parachutes was announced in an October 14 press release. Lockheed Martin had built the system with an acceleration sensor's internal mechanisms wrongly oriented (a G-switch was installed backwards), and design reviews had not caught the mistake. The intended design was to make an electrical contact inside the sensor at 3 g (29 m/s²), maintaining it through the maximum expected 30 g (290 m/s²), and breaking the contact again at 3 g to start the parachute release sequence. Instead, no contact was ever made.
NASA investigation board chair Michael Ryschkewitsch noted that none of the stringent review procedures at NASA had picked up a mistake, saying, "It would be very easy to mix this up."
This mishap is similar to the original event that inspired Edward A. Murphy, Jr. to formulate the now-famous Murphy's Law: an accelerometer installed backwards. On January 6, 2006, Ryschkewitsch revealed that a pre-test procedure on the craft was skipped by Lockheed Martin, and he noted that the test could have easily detected the problem.
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- The NASA Stardust mission launched two years before Genesis, but did not return to Earth until two years after Genesis's return.
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- Klein, John; Manning, Rob; Barry, Ed; Donaldson, Jim; Rivellini, Tom; Battel, Steven; Savino, Joe; Lee, Wayne; Dalton, Jerry; Underwood, Mark; Surampudi, Rao; Accord, Arden; Perkins, Dave; Barrow, Kirk; Wilson, Bob. "Genesis failure investigation report : JPL Failure Review Board, Avionics Sub-Team". JPL Publication 05-2. Jet Propulsion Laboratory. Retrieved 19 October 2011.
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- Meshik, Alex; Mabry, Jennifer; Hohenberg, Charles; Marrocchi, Yves; Pravdivtseva, Olga; Burnett, Donald; Olinger, Chad; Wiens, Roger; Reisenfeld, Dan; Allton, Judith; McNamara, Karen; Stansbery, Eileen; Jurewicz, Amy J. G. (18 October 2007). "Constraints on Neon and Argon Isotopic Fractionation in Solar Wind". Science 318 (5849): 433–435. Bibcode:2007Sci...318..433M. doi:10.1126/science.1145528. PMID 17947578. Retrieved 2007-10-20.
- UCLA Department of Earth and Space Sciences
- Jones, Nicola (18 October 2007). "Crashed spacecraft yields data". naturenews. doi:10.1038/news.2007.175. Retrieved 2007-10-20.
- "Genesis science "a work in progress"". NASA. 2005. Retrieved November 30, 2012.
- "Genesis spacecraft bus flies solo". NASA. 2005. Retrieved November 30, 2012.
- McKee, Maggie (15 October 2004). "Genesis crash linked to upside-down design". New Scientist. Retrieved 2006-04-24.
- Oberg, James (21 October 2004). "'Murphy's Law' rules outer space... And NASA still needs to learn how to evade it". MSNBC. Retrieved 2006-04-24.
- Associated Press (2006-01-07). "Official: Genesis Pre-Launch Test Skipped". Space.com. Retrieved 2006-04-24.[dead link]
|Wikimedia Commons has media related to: Genesis (spacecraft)|
- "Genesis Mission Home Page". JPL. Retrieved 2008-05-21.
- Genesis Mission Profile by NASA's Solar System Exploration
- "Impact video" (QuickTime movie). Retrieved 2006-04-20.
- Associated Press (23 September 2004). "Genesis Capsule to Be Sent to Colorado". SPACE.com. Retrieved 2006-04-24.
- Pegg Jr., Ed (7 September 2004). "Manifolds in the Genesis mission". Math Games. Mathematical Association of America. Retrieved 2006-04-24.
- "MegaSIMS Home Page". UCLA. Retrieved 2008-12-05.