Discovery Program
The Discovery Program is a series of Solar System exploration missions funded by the US National Aeronautics and Space Administration through its Planetary Missions Program Office. Each mission has a cost cap, at a lower level than a mission from NASA's New Frontiers or Flagship Programs. As a result, Discovery missions tend to be more focused on a specific scientific goal.
The Discovery Program was founded in 1990 to implement then-NASA Administrator Daniel S. Goldin's policy of "faster, better, cheaper" planetary science missions. Existing NASA programs had specified mission targets and objectives in advance, then sought bidders to construct and operate them. In contrast, Discovery missions are solicited through a call for proposals on any science topic, and assessed through peer review. Selected missions are led by a scientist called the Principal Investigator and may include contributions from industry, universities, or government laboratories.
The Discovery Program also includes Missions of Opportunity, which fund US participation in spacecraft operated by other space agencies. It can also be used to re-purpose an existing NASA spacecraft for a new mission.
, the most recently-selected Discovery missions are Lucy and Psyche, the thirteenth and fourteenth missions in the program.
History
In 1989, NASA's Solar System Exploration Division began to define a new strategy for Solar System exploration up to the year 2000. This included a Small Mission Program Group that investigated missions that would be low cost and allow focused scientific questions to be addressed in shorter time than existing programs. The result was a request for rapid studies of potential missions and NASA committed funding in 1990. The new program was called 'Discovery'.The panel assessed several concepts that could be implemented as low-cost programs, selecting NEAR Shoemaker as the first mission.
NEAR became the first launch in the Discovery Program on February 17, 1996. The second mission, Mars Pathfinder, launched on December 4, 1996, carrying the Sojourner rover to Mars.
Missions
Standalone missions
Missions of opportunity
These provide opportunities to participate in non-NASA missions by providing funding for a science instrument or hardware components of an instrument, or for an extended mission for a spacecraft that may different from its original purpose.- ASPERA-3, an instrument designed to study the interaction between the solar wind and the atmosphere of Mars, is flying on board the European Space Agency's Mars Express orbiter. Launched in June 2003, it has been orbiting Mars since December 2003. The Principal Investigator is David Winningham of Southwest Research Institute.
- Moon Mineralogy Mapper is a NASA-designed instrument placed on board the ISRO's Chandrayaan orbiter selected in February 2005. Launched in 2008, it was designed to explore the Moon's mineral composition at high resolution. M3's detection of water on the Moon was announced in September 2009, one month after the mission ended. The Principal Investigator was Carle Pieters of Brown University.
- Extrasolar Planet Observation and Deep Impact Extended Investigation was selected in July 2007. It was a series of two new missions for the existing Deep Impact probe following its success at Tempel 1:
- * The Extrasolar Planet Observations and Characterization mission used the Deep Impact high-resolution camera in 2008 to better characterize known giant extrasolar planets orbiting other stars and to search for additional planets in the same system. The Principal Investigator was L. Drake Deming of NASA's Goddard Space Flight Center.
- * The Deep Impact eXtended Investigation of Comets mission used the Deep Impact mission's spacecraft for a flyby mission to a second comet, Hartley 2. The goal was to take pictures of its nucleus to increase our understanding of the diversity of comets. The flyby of Hartley 2 was successful with closest approach occurring on November 4, 2010. Michael A'Hearn of the University of Maryland was the Principal Investigator.
- was selected in July 2007 together with the EPOXI extension. It was a new mission for the Stardust spacecraft to fly by comet Tempel 1 in 2011 and observe changes since the Deep Impact mission visited it in July 2005. Later in 2005, Tempel 1 made its closest approach to the Sun, possibly changing the surface of the comet. The flyby was completed successfully on February 15, 2011. Joseph Veverka of Cornell University is the Principal Investigator.
- Strofio is a unique mass spectrometer that is part of the SERENA instrument package on board the European Space Agency's BepiColombo/Mercury Planetary Orbiter spacecraft. Strofio will study the atoms and molecules that compose Mercury's atmosphere to reveal the composition of the planet's surface. Stefano Livi of Southwest Research Institute is the Principal Investigator.
- MEGANE is an instrument planned to fly aboard the Martian Moons Exploration, a Japanese Aerospace Exploration Agency probe to Phobos and Deimos launching in 2024. MEGANE includes a gamma-ray spectrometer and a neutron spectrometer. David J. Lawrence of Johns Hopkins University is the Principal Investigator.
- In addition, the Lunar Reconnaissance Orbiter has been managed under the Discovery Program since the Lunar Precursor Robotic Program was terminated.
Mission timeline
Proposals and concepts
However often the funding comes in, there is a selection process with perhaps two dozen concepts. These sometimes get further matured and re-proposed in another selection or program. An example of this is Suess-Urey Mission, which was passed over in favor of the successful Stardust mission, but was eventually flown as Genesis, while a more extensive mission similar to INSIDE was flown as Juno in the New Frontiers program. Some of these concepts went on to become actual missions, or similar concepts were eventually realized in another mission class. This list is a mix of previous and current proposals.Additional examples of Discovery-class mission proposals include:
- Whipple, space-observatory to detect objects in the Oort cloud by transit method.
- Io Volcano Observer
- Comet Hopper
- Titan Mare Explorer
- Suess-Urey, similar to the later Genesis mission.
- Hermes, a Mercury orbiter.
- INSIDE Jupiter, an orbiter that would map Jupiter's magnetic and gravity fields in an effort to study the giant planet's interior structure. The concept was further matured and implemented as Juno in the New Frontiers program.
- The Dust Telescope is a space observatory that would measure various properties of incoming cosmic dust. The dust telescope would combine a trajectory sensor and a mass spectrometer, to allow the elemental and even isotopic composition to be analyzed.
- OSIRIS was an asteroid observation and sample return mission concept selected in 2006 for further concept studies. It was further matured and launched September 8, 2016 as OSIRIS-REx in the New Frontiers Program.
- Small Body Grand Tour, an asteroid rendezvous mission. This 1993 concept reviews possible targets for what became NEAR 4660 Nereus and 2019 Van Albada. Other targets considered for an extended mission included Encke's comet, 433 Eros, 1036 Ganymed, 4 Vesta, and 4015 Wilson–Harrington.
- Comet Coma Rendezvous Sample Return, a spacecraft designed to rendezvous with a comet, make extended observations within the cometary coma, gently collect multiple coma samples, and return them to Earth for study.
- Micro Exo Explorer would use a new form of micro-electric propulsion, called 'Micro Electro-fluidic-spray Propulsion' to travel to a near Earth object and gather important data.
Mars focused
- Pascal, a Mars climate network mission.
- MUADEE
- Phobos Surveyor is an orbiter mission concept to the Mars moon Phobos, which would also deploy special rovers for the moon's low gravity environment.
- PCROSS, based on LCROSS but to Mars' moon Phobos.
- Merlin mission would place a lander on Mars' moon Deimos.
- Mars Moons Multiple Landings Mission, would conduct multiple landings on Phobos and Deimos.
- Hall is a Phobos and Deimos sample return mission.
- Aladdin was a Discovery-class Phobos and Deimos sample return mission. It was a finalist in the 1999 Discovery selection, with a planned launch in 2001 and return of the samples by 2006. Sample collection was intended to work by sending projectiles into the moons, then collecting the ejecta by means of a collector spacecraft flyby.
- Mars Geyser Hopper is a lander that would investigate the springtime carbon dioxide Martian geysers found in regions around the south pole of Mars.
- MAGIC is an orbiter that would provide images of the Martian surface at 5–10 cm/pixel, permitting resolution of features as small as 20–40 cm.
- Red Dragon, a Mars lander and sample return.
Lunar focused
- Lunar sample return from the South Pole–Aitken basin. No geologic model adequately accounts for all of the characteristics of the area and disagreements are fundamental.
- EXOMOON, in situ investigation on Earth's Moon.
- PSOLHO, would use the Moon as an occulter to look for exoplanets.
- Lunette, a lunar lander.
- Twin Lunar Lander, a geophysics mission to the Moon.
Venus focused
- Venus Multiprobe, proposed for a 1999 launch, would have dropped 16 atmospheric probes into Venus, and fall slowly to the surface, making pressure and temperature measurements.
- Vesper was a concept for a Venus orbiter focused on studying that planet's atmosphere. It was one of three concepts to receive funds for further study in the 2006 Discovery selection. Osiris and GRAIL were the other two, and eventually GRAIL was chosen and went on to be launched.
- V-STAR is a Venus atmosphere sample return mission. While returning samples from the surface of Venus has noted difficulties, a Discovery-class sample return from the upper atmosphere is being proposed. Something along the lines of Stardust mission but using a free-return trajectory.
- VEVA is an in atmosphere probe for Venus. The centerpiece is a 7-day balloon flight through the atmosphere accompanied by various tiny probes dropped deeper into the planet's thick gases.
- Venus Pathfinder, a long-duration Venus lander.
- RAVEN, a Venus orbiter radar mapping mission.
- VALOR, a Venus mission to study its atmosphere with a balloon. Twin balloons would circumnavigate the planet over 8 Earth-days.
- Venus Aircraft, a robotic atmospheric flight on Venus' atmosphere using a long-duration solar-powered aircraft system. It would carry 1.5 kg of scientific payload and it must contend with violent wind, heat and a corrosive atmosphere.
- Venus Landsailing Rover, a rover concept that would be propelled by the wind force on its vertical wingsail. Conceived in 2012, the project has since made progress in developing electronic components that would allow the vehicle to operate for 50 days on the surface of Venus without a cooling system.
Selection process
Discovery 1 and 2
The first two Discovery missions were Near Earth Asteroid Rendezvous and Mars Pathfinder. These initial missions did not follow the same selection process that started once the program was under-way. Mars Pathfinder was salvaged from the idea for a technology and EDL demonstrator from the Mars Environmental Survey program. Also, one of the goals of Pathfinder was to support the Mars Surveyor program. Later missions would be selected by a more sequential process involving Announcements of Opportunity.In the case of NEAR, a working group for the program recommended that the first mission should be to a near-Earth asteroid. A series of proposals limited to missions to a near-Earth asteroid missions was reviewed in 1991. What would be the NEAR spacecraft mission was formally selected in December 1993, after which a 2-year development period would follow prior to launch. NEAR was launched on February 15, 1996, and arrived to orbit asteroid Eros on February 14, 2000. Mars Pathfinder launched on December 4, 1996, and landed on Mars on July 4, 1997, bringing along with it the first NASA Mars rover, Pathfinder.
Discovery 3 and 4
In August 1994, NASA made an Announcement of Opportunity for the next proposed Discovery missions. There were 28 proposals submitted to NASA in October 1994:- ASTER- Asteroid Earth Return
- Comet Nucleus Penetrator
- Comet Nucleus Tour
- Cometary Coma Chemical Composition
- Diana
- FRESIP-A mission to Find the Frequency of Earth-sized Inner Planets
- Hermes Global Orbiter
- Icy Moon Mission
- Interlune-One
- Jovian Integrated Synoptic Telescope
- Lunar Discovery Orbiter
- Mainbelt Asteroid Exploration/Rendezvous
- Mars Aerial Platform
- Mars Polar Pathfinder
- Mars Upper Atmosphere Dynamics, Energetics and Evolution
- Mercury Polar Flyby
- Near Earth Asteroid Returned Sample
- Origin of Asteroids, Comets and Life on Earth
- PELE: A Lunar Mission to Study Planetary Volcanism
- Planetary Research Telescope
- Rendezvous with a Comet Nucleus
- Small Missions to Asteroids and Comets
- Venus Composition Probe
- Venus Environmental Satellite
Discovery 5 and 6
In October 1997, NASA selected Genesis and CONTOUR as the next Discovery missions, out of 34 proposals that were submitted in December 1996.The five finalists were:
- Aladdin
- Comet Nucleus Tour
- Genesis
- Mercury Surface, Space Environment, Geochemistry and Ranging mission
- Venus Environmental Satellite
Discovery 7 and 8
In 1998 five finalists had been selected to receive US$375,000 to further mature their design concept. The five proposals were selected out of about 30 with the goal of achieving the best science. Those missions were:
- Aladdin
- Deep Impact
- MESSENGER
- INSIDE Jupiter
- Vesper
Discovery 9 and 10
26 proposals were submitted to the 2000 Discovery solicitation, with budget initially targeted at US$300 million. Three candidates were shortlisted in January 2001 for a phase-A design study: Dawn, Kepler space telescope, and INSIDE Jupiter. INSIDE Jupiter was similar to a later New Frontiers mission called Juno; Dawn was a mission to asteroids Vesta and Ceres, and Kepler was a space telescope mission aimed to discover extrasolar planets. The three finalists received US$450,000 to further mature the mission concept.In December 2001, Kepler and Dawn were selected for flight. At this time, only 80 exoplanets had been detected, and that was part of the mission of Kepler, to look for more exoplanets, especially Earth-sized. Both Kepler and Dawn were initially projected for launch in 2006.
The Discovery Program fell on hard-times after this, with several missions experiencing cost overruns, and the CONTOUR mission experiencing an engine failure in orbit. Although both Dawn and Kepler would become widely praised success stories, they missed their somewhat ambitious 2006 launch target, launching in 2007 and 2009 respectively. Kepler would go on to receive several mission extensions, and Dawn successfully orbited both Vesta and Ceres. Nevertheless, the next selection would take longer than previous as the program selection of new missions slowed down. As the successes of the new missions enhanced the image of the Discovery Program, the difficulties began to fade from the limelight. Also, the number of active missions in development or active began to increase as the program ramped up.
Discovery 11
The Announcement of Opportunity for this Discovery mission was released in April 2006. There were three finalists for this Discovery selection including GRAIL, OSIRIS, and VESPER. OSIRIS was very similar to the later OSIRIS-REx mission, an asteroid sample-return mission to 101955 Bennu, and Vesper, a Venus orbiter mission. A previous proposal of Vesper had also been a finalist in the 1998 round of selection. The three finalists were announced in October 2006 and awarded US$1.2 million to further develop their proposals for the final round.In November 2007 NASA selected the GRAIL mission as the next Discovery mission, with a goal of mapping lunar gravity and a 2011 launch. There were 23 other proposals that were also under consideration. The mission had a budget of US$375 million which included construction and launch.
Discovery 12
For this cycle, 28 proposals were received in 2010; 3 were for the Moon, 4 for Mars, 7 for Venus, 1 for Jupiter, 1 to a Jupiter Trojan, 2 to Saturn, 7 to asteroids, and 3 to comets. Out of the 28 proposals, three finalists received US$3 million in May 2011 to develop a detailed concept study:- InSight, a Mars lander.
- Titan Mare Explorer, a lake lander for Saturn's moon Titan with methane-ethane lakes.
- Comet Hopper to study cometary evolution by landing on a comet multiple times and observing its changes as it interacts with the Sun.
Discovery 13 and 14
In February 2014, NASA released a Discovery Program 'Draft Announcement of Opportunity' for launch readiness date of December 31, 2021. On September 30, 2015, NASA selected five mission concepts as finalists, each received $3 million for one-year of further study and concept refinement.- Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging
- Venus Emissivity, Radio Science, InSAR Topography and Spectroscopy
- Near-Earth Object Camera
- Lucy
- Psyche
Discovery 15 and 16
On December 22, 2018, NASA released a draft of its Discovery 2019 Announcement of Opportunity, which outlined its intent to select up to two missions with launch readiness dates of July 1, 2025 – December 31, 2026 and/or July 1, 2028 – Dec. 31, 2029 as Discovery 15 and 16, respectively. The final Announcement of Opportunity was released on April 1, 2019, and proposal submissions were accepted between then and July 1, 2019.Finalists were announced on February 13, 2020. The final selections will be made in 2021. Finalists are:
- DAVINCI+ is a Venus atmospheric probe.
- Io Volcano Observer would be an orbiter to Jupiter to perform at least nine flybys of Jupiter's moon Io, which is volcanically active
- Trident would conduct a flyby of Neptune and its moon Triton.
- VERITAS, a Venus orbiter concept to map with high resolution the surface of Venus.
;Asteroids, comets, Centaurs, interplanetary dust
- Centaurus, a reconnaissance mission to explore multiple Centaurs via flybys as a way to learn about Solar System and planet formation.
- Chimera, a mission concept to orbit the highly active Centaur 29P/Schwasmann-Wachmann 1, to study the evolutionary middle ground between the Trans Neptunian Objects and Jupiter Family Comets.
- FOSSIL would place a spacecraft in an Earth-trailing orbit to determine the composition of the local and interplanetary dust cloud.
- MANTIS, is a mission concept that would flyby 14 asteroids covering a wide range of types and masses.
- HOVER, is a Venus orbiter concept that would perform spectral studies from the top of the atmosphere to the surface. Its main goal is understanding the mechanics of the Venus climate and atmospheric super-rotation.
- Moon Diver would deploy a lunar rover to rappel down a deep pit to analyze the exposed geological layers and investigate if the pit connects to a lava tube.
- Lunar Compass Rover was a concept to explore a nearside magnetic region and swirl, and would answer some outstanding questions in planetary science, including planetary magnetism, space plasma physics, space weathering, planetary geology, and the lunar water cycle. A proposal for Lunar Compass was not submitted to this Discovery round.
- ISOCHRON would perform a robotic lunar sample-return of the youngest mare basalts.
- NanoSWARM is a concept that proposes a lunar orbiter to investigate lunar swirls, space weathering, lunar water, lunar magnetism, and small-scale magnetospheres.
- COMPASS is a mission concept for a Mars orbiter to research the Martian climate record through the study of its ice deposits and their interaction with current climate. This mission is led by the Lunar and Planetary Laboratory at the University of Arizona and the Laboratory for Atmospheric and Space Physics at the University of Colorado, Boulder.
- Icebreaker Life is a mission concept led by Goddard Space Flight Center for a lander to search for direct signs of life on Mars via biomarker detection via a focus on sampling ice-cemented ground for its potential to preserve and protect biomolecules or biosignatures.
- MAGIC is an orbiter reconnaissance concept to Jupiter's moon Callisto.
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