MAVEN

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Mars Atmosphere and Volatile Evolution
MAVEN spacecraft model.png
Artist's rendering of the MAVEN spacecraft bus
Names
  • MAVEN
  • Mars Atmosphere and Volatile Evolution
Mission typeMars atmospheric research
Operator NASA
COSPAR ID 2013-063A OOjs UI icon edit-ltr-progressive.svg
SATCAT no. 39378
Website Official website
Mission duration2 years (planned)
Science phase extended indefinitely
9 years, 2 months, 29 days (in progress)
Spacecraft properties
Manufacturer Lockheed Martin Space Systems
Launch mass2,454 kg (5,410 lb) [1]
Dry mass809 kg (1,784 lb)
Payload mass65 kg (143 lb)
Dimensions2.3 m × 2.3 m × 2 m
Power1135 watts [2]
Start of mission
Launch date18 November 2013, 18:28:00 UTC
Rocket Atlas V 401 (AV-038)
Launch site Cape Canaveral, SLC-41
Contractor United Launch Alliance
Orbital parameters
Reference system Areocentric orbit
Regime Elliptic orbit
Periareon altitude 150 km (93 mi)
Apoareon altitude 6,200 km (3,900 mi)
Inclination 75°
Period 4.5 hours
Mars orbiter
Orbital insertion22 September 2014, 02:24 UTC [3]
MSD 50025 08:07 AMT
MAVEN Mission Logo.png
Maven mission logo  

MAVEN is a NASA spacecraft orbiting Mars to study the loss of that planet's atmospheric gases to space, providing insight into the history of the planet's climate and water. [4] The name is an acronym for "Mars Atmosphere and Volatile Evolution" while the word maven also denotes "a person who has special knowledge or experience; an expert". [5] [6] MAVEN was launched on an Atlas V rocket from Cape Canaveral Air Force Station, Florida, on 18 November 2013 UTC and went into orbit around Mars on 22 September 2014 UTC. The mission is the first by NASA to study the Mars atmosphere. The probe is analyzing the planet's upper atmosphere and ionosphere to examine how and at what rate the solar wind is stripping away volatile compounds.

Contents

The principal investigator for the mission is Shannon Curry at the University of California, Berkeley. She took over from Bruce Jakosky of the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder, who proposed and led the mission until 2021. [4] The project cost $582.5 million to build, launch, and operate through its two-year prime mission. [7]

Pre-launch

MAVEN - Atlas V ignition (18 November 2013) MAVEN Launch2-full.jpg
MAVEN – Atlas V ignition (18 November 2013)

Proposed in 2006, the mission was the second of NASA's Mars Scout Program, which had previously yielded Phoenix. It was selected for development for flight in 2008. [8]

On 2 August 2013, the MAVEN spacecraft arrived at Kennedy Space Center, in Florida to begin launch preparations. [9]

On 1 October 2013, only seven weeks before launch, a government shutdown caused suspension of work for two days and initially threatened to force a 26-month postponement of the mission. With the spacecraft nominally scheduled to launch on 18 November 2013, a delay beyond 7 December 2013 would have caused MAVEN to miss the launch window as Mars moved too far out of alignment with the Earth. [10]

However, two days later, on 3 October 2013, a public announcement was made that NASA had deemed the 2013 MAVEN launch so essential to ensuring future communication with current NASA assets on Mars — the rovers Opportunity and Curiosity — that emergency funding was authorized to restart spacecraft processing in preparation for an on-time launch. [11]

Objectives

MAVEN's interplanetary journey to Mars

Features on Mars that resemble dry riverbeds and the discovery of minerals that form in the presence of water indicate that Mars once had a dense enough atmosphere and was warm enough for liquid water to flow on the surface. However, that thick atmosphere was somehow lost to space. Scientists suspect that over millions of years, Mars lost 99% of its atmosphere as the planet's core cooled and its magnetic field decayed, allowing the solar wind to sweep away most of the water and volatile compounds that the atmosphere once contained. [12]

The goal of MAVEN is to determine the history of the loss of atmospheric gases to space, providing answers about Martian climate evolution. By measuring the rate with which the atmosphere is currently escaping to space and gathering enough information about the relevant processes, scientists will be able to infer how the planet's atmosphere evolved over time. The MAVEN mission's primary scientific objectives are:

Timeline

MAVEN launched from the Cape Canaveral Air Force Station (CCAFS) on 18 November 2013, using an Atlas V 401 launch vehicle. [13] [14] It reached Mars on 22 September 2014, and was inserted into an elliptic orbit approximately 6,200 km (3,900 mi) by 150 km (93 mi) above the planet's surface. [14]

In October 2014, as the spacecraft was being fine-tuned to start its primary science mission, the comet Siding Spring was also performing a close flyby of Mars. The researchers had to maneuver the craft to mitigate harmful effects of the comet, but while doing so, were able to observe the comet and perform measurements on the composition of expelled gases and dust. [15]

On 16 November 2014, investigators completed MAVEN's commissioning activities and began its primary science mission, scheduled to last one year. [16] During that time, MAVEN had observed a nearby comet, measured how volatile gases are swept away by solar wind, and performed four "deep dips" down to the border of the upper and lower atmospheres to better characterize the planet's entire upper atmosphere. [17] In June 2015, the science phase was extended through September 2016, allowing MAVEN to observe the Martian atmosphere through the entirety of the planet's seasons. [18]

On 3 October 2016, MAVEN completed one full Martian year of scientific observations. It had been approved for an additional 2-year extended mission through September 2018. All spacecraft systems were still operating as expected. [19]

In March 2017, MAVEN's investigators had to perform a previously unscheduled maneuver to avoid colliding with Phobos the following week. [20]

On 5 April 2019, the navigation team completed a two-month aerobraking maneuver to lower MAVEN's orbit and enable it to better serve as a communications relay for current landers as well as the rover Perseverance . This new elliptic orbit is approximately 4,500 km (2,800 mi) by 130 km (81 mi). With 6.6 orbits per Earth day, the lower orbit allows more frequent communication with rovers. [21]

As of September 2020, the spacecraft is continuing its science mission as well, with all instruments still operating and with enough fuel to last at least until 2030. [21]

On August 31, 2021, Shannon Curry became the Principal Investigator of the mission. [22]

NASA became aware of failures in the MAVEN's inertia measurement units (IMU) in late 2021, necessary for the probe to maintain its orbit; having already moved from the main IMU to the backup one in 2017, they saw the backup ones showing signs of failure. In February 2022, both IMUs had appeared to lost the ability to perform its measurement properly. After doing a heartbeat termination to restore the use of the backup IMU, NASA engineers set to reprogram MAVEN to use an "all stellar" mode using star positions to maintain its altitude, eliminating the reliance on the IMUs. This was put into place in April 2022 and completed by May 28, 2022, but during this period, MAVEN could not be used for scientific observations or to relay communications to Earth from the rovers Curiosity and Perseverance and the Insight lander. Reduced communication was handled by other Mars orbiters. [23]

Animation of MAVEN's trajectory around the Sun .mw-parser-output .legend{page-break-inside:avoid;break-inside:avoid-column}.mw-parser-output .legend-color{display:inline-block;min-width:1.25em;height:1.25em;line-height:1.25;margin:1px 0;text-align:center;border:1px solid black;background-color:transparent;color:black}.mw-parser-output .legend-text{} MAVEN * Mars * Earth * Sun Animation of MAVEN trajectory around Sun.gif
Animation of MAVEN's trajectory around the Sun
   MAVEN ·   Mars  ·  Earth ·  Sun
Animation of MAVEN's trajectory around Mars from September 22, 2014 to September 22, 2016 MAVEN * Mars Animation of MAVEN trajectory around Mars.gif
Animation of MAVEN's trajectory around Mars from September 22, 2014 to September 22, 2016
   MAVEN ·   Mars
MAVEN aerobraking to a lower orbit - in preparation for the Mars 2020 mission (February 2019) MavenAerobrakingDiagram-20190211.jpg
MAVEN aerobraking to a lower orbit – in preparation for the Mars 2020 mission (February 2019)

Spacecraft overview

MAVEN was built and tested by Lockheed Martin Space Systems. Its design is based on those of Mars Reconnaissance Orbiter and 2001 Mars Odyssey . The orbiter has a cubical shape of about 2.3 m × 2.3 m × 2 m (7 ft 7 in × 7 ft 7 in × 6 ft 7 in) high, [24] with two solar arrays that hold the magnetometers on both ends. The total length is 11.4 m (37 ft). [25]

Relay telecommunications

MAVEN's Electra UHF radio transceiver Pia17952 electra transceiver dsc09326 0.jpg
MAVEN's Electra UHF radio transceiver

NASA's Jet Propulsion Laboratory provided an Electra ultra high frequency (UHF) relay radio payload which has a data return rate of up to 2048 kbit/s. [26] The highly elliptical orbit of the MAVEN spacecraft may limit its usefulness as a relay for operating landers on the surface, although the long view periods of MAVEN's orbit have afforded some of the largest relay data returns to date of any Mars orbiter. [27] During the mission's first year of operations at Mars — the primary science phase — MAVEN served as a backup relay orbiter. In the extended mission period of up to ten years, MAVEN will provide UHF relay service for present and future Mars rovers and landers. [18]

Scientific instruments

Solar Wind Electron Analyzer (SWEA) measures solar wind and ionosphere electrons. Main swea5 full.jpg
Solar Wind Electron Analyzer (SWEA) measures solar wind and ionosphere electrons.
Magnetometer of MAVEN MAVEN -- Magnetometer.jpg
Magnetometer of MAVEN
SEP instrument of MAVEN Solar Energetic Particles.jpg
SEP instrument of MAVEN

The University of Colorado Boulder, University of California, Berkeley, and Goddard Space Flight Center each built a suite of instruments for the spacecraft, and they include: [28]

Built by the University of California, Berkeley Space Sciences Laboratory:

Built by the University of Colorado Boulder Laboratory for Atmospheric and Space Physics:

Built by Goddard Space Flight Center:

SWEA, SWIA, STATIC, SEP, LPW, and MAG are part of the Particles and Fields instrument suite, IUVS is the Remote Sensing instrument suite, and NGIMS is its own eponymous suite.

Cost

MAVEN Development and Prime Mission Costs MAVEN Development and Prime Mission Costs.svg
MAVEN Development and Prime Mission Costs

MAVEN cost US$582.5 million to build, launch, and operate for its prime mission, nearly US$100 million less than originally estimated. Of this total, US$366.8 million was for development, US$187 million for launch services, and US$35 million was for the 2-year prime mission. On average, NASA spends US$20 million annually on MAVEN's extended operations. [7]

Results

Atmospheric loss

Mars loses water into its thin atmosphere by evaporation. There, solar radiation can split the water molecules into their components, hydrogen and oxygen. The hydrogen, as the lightest element, then tends to rise far up to the highest levels of the Martian atmosphere, where several processes can strip it away into space, to be forever lost to the planet. This loss was thought to proceed at a fairly constant rate, but MAVEN's observations of Mars's atmospheric hydrogen through a full Martian year (almost two Earth years) show that the escape rate is highest when Mars's orbit brings it closest to the Sun, and only one-tenth as great when it is at its farthest. [39]

On 5 November 2015, NASA announced that data from MAVEN shows that the deterioration of Mars's atmosphere increases significantly during solar storms. That loss of atmosphere to space likely played a key role in Mars's gradual shift from its carbon dioxide–dominated atmosphere – which had kept Mars relatively warm and allowed the planet to support liquid surface water – to the cold, arid planet seen today. This shift took place between about 4.2 and 3.7 billion years ago. [40] Atmospheric loss was especially notable during an interplanetary coronal mass ejection in March 2015. [41]

PIA18613-MarsMAVEN-Atmosphere-3UV-Views-20141014.jpg
Mars – escaping atmosphere – carbon, oxygen, hydrogen (MAVEN – UV – 14 October 2014). [42]

Different types of aurora

In 2014, MAVEN researchers detected widespread aurora throughout the planet, even close to the equator. Given the localized magnetic fields on Mars (as opposed to Earth's global magnetic field), aurora appear to form and distribute in different ways on Mars, creating what scientists call diffuse aurora. Researchers determined that the source of the particles causing the aurorae were a huge surge of electrons originating from the Sun. These highly energetic particles were able to penetrate far deeper into Mars's atmosphere than they would have on Earth, creating aurora much closer to the surface of the planet (~60 km as opposed to 100–500 km on Earth). [43]

Scientists also discovered proton aurora, different from the so-called typical aurora which is produced by electrons. Proton aurora were previously only detected on Earth. [44]

Interaction with a comet

The fortuitous arrival of MAVEN just before a flyby of the comet Siding Spring gave researchers a unique opportunity to observe both the comet itself as well as its interactions with the Martian atmosphere. The spacecraft's IUVS instrument detected intense ultraviolet emissions from magnesium and iron ions, a result from the comet's meteor shower, which were much stronger than anything ever detected on Earth. [45] The NGIMS instrument was able to directly sample dust from this Oort Cloud comet, detecting at least eight different types of metal ions. [46]

Detection of metal ions

In 2017, results were published detailing the detection of metal ions in Mars's ionosphere. This is the first time metal ions have been detected in any planet's atmosphere other than Earth's. It was also noted that these ions behave and are distributed differently in the atmosphere of Mars given that the red planet has a much weaker magnetic field than our own. [47]

Impacts on future exploration

In September 2017, NASA reported a temporary doubling of radiation levels on the surface of Mars, as well as an aurora 25 times brighter than any observed earlier. This occurred due to a massive, and unexpected, solar storm. [48] The observation provided insight into how changes in radiation levels might impact the planet's habitability, helping NASA researchers understand how to predict as well as mitigate effects on future human Mars explorers.

See also

Related Research Articles

<i>2001 Mars Odyssey</i> NASA orbiter for geology and hydrology

2001 Mars Odyssey is a robotic spacecraft orbiting the planet Mars. The project was developed by NASA, and contracted out to Lockheed Martin, with an expected cost for the entire mission of US$297 million. Its mission is to use spectrometers and a thermal imager to detect evidence of past or present water and ice, as well as study the planet's geology and radiation environment. It is hoped that the data Odyssey obtains will help answer the question of whether life existed on Mars and create a risk-assessment of the radiation that future astronauts on Mars might experience. It also acts as a relay for communications between the Curiosity rover, and previously the Mars Exploration Rovers and Phoenix lander, to Earth. The mission was named as a tribute to Arthur C. Clarke, evoking the name of his and Stanley Kubrick's 1968 film 2001: A Space Odyssey.

<span class="mw-page-title-main">Solar wind</span> Stream of charged particles from the Sun

The solar wind is a stream of charged particles released from the upper atmosphere of the Sun, called the corona. This plasma mostly consists of electrons, protons and alpha particles with kinetic energy between 0.5 and 10 keV. The composition of the solar wind plasma also includes a mixture of materials found in the solar plasma: trace amounts of heavy ions and atomic nuclei of elements such as C, N, O, Ne, Mg, Si, S, and Fe. There are also rarer traces of some other nuclei and isotopes such as P, Ti, Cr, and 58Ni, 60Ni, and 62Ni. Superimposed with the solar-wind plasma is the interplanetary magnetic field. The solar wind varies in density, temperature and speed over time and over solar latitude and longitude. Its particles can escape the Sun's gravity because of their high energy resulting from the high temperature of the corona, which in turn is a result of the coronal magnetic field. The boundary separating the corona from the solar wind is called the Alfvén surface.

<span class="mw-page-title-main">Pioneer Venus project</span> Two spacecraft send to Venus in 1978

The Pioneer Venus project was part of the Pioneer program consisting of two spacecraft, the Pioneer Venus Orbiter and the Pioneer Venus Multiprobe, launched to Venus in 1978. The program was managed by NASA's Ames Research Center.

<i>Nozomi</i> (spacecraft) Failed Mars orbiter

Nozomi was a Japanese Mars orbiter that failed to reach Mars due to electrical failure. It was constructed by the Institute of Space and Astronautical Science, University of Tokyo and launched on July 4, 1998, at 03:12 JST with an on-orbit dry mass of 258 kg and 282 kg of propellant. The Nozomi mission was terminated on December 31, 2003.

<span class="mw-page-title-main">Mars 96</span> Failed Mars mission

Mars 96 was a failed Mars mission launched in 1996 to investigate Mars by the Russian Space Forces and not directly related to the Soviet Mars probe program of the same name. After failure of the second fourth-stage burn, the probe assembly re-entered the Earth's atmosphere, breaking up over a 320 km (200 mi) long portion of the Pacific Ocean, Chile, and Bolivia. The Mars 96 spacecraft was based on the Phobos probes launched to Mars in 1988. They were of a new design at the time and both ultimately failed. For the Mars 96 mission the designers believed they had corrected the flaws of the Phobos probes, but the value of their improvements was never demonstrated due to the destruction of the probe during the launch phase.

Atmospheric escape is the loss of planetary atmospheric gases to outer space. A number of different mechanisms can be responsible for atmospheric escape; these processes can be divided into thermal escape, non-thermal escape, and impact erosion. The relative importance of each loss process depends on the planet's escape velocity, its atmosphere composition, and its distance from its star. Escape occurs when molecular kinetic energy overcomes gravitational energy; in other words, a molecule can escape when it is moving faster than the escape velocity of its planet. Categorizing the rate of atmospheric escape in exoplanets is necessary to determining whether an atmosphere persists, and so the exoplanet's habitability and likelihood of life.

<span class="mw-page-title-main">Atmosphere of Mars</span> Layer of gases surrounding planet Mars

The atmosphere of Mars is the layer of gases surrounding Mars. It is primarily composed of carbon dioxide (95%), molecular nitrogen (2.8%), and argon (2%). It also contains trace levels of water vapor, oxygen, carbon monoxide, hydrogen, and noble gases. The atmosphere of Mars is much thinner than Earth's. The average surface pressure is only about 610 pascals (0.088 psi) which is less than 1% of the Earth's value. The currently thin Martian atmosphere prohibits the existence of liquid water on the surface of Mars, but many studies suggest that the Martian atmosphere was much thicker in the past. The higher density during spring and fall is reduced by 25% during the winter when carbon dioxide partly freezes at the pole caps. The highest atmospheric density on Mars is equal to the density found 35 km (22 mi) above the Earth's surface and is ≈0.020 kg/m3. The atmosphere of Mars has been losing mass to space since the planet's core slowed down, and the leakage of gases still continues today. The atmosphere of Mars is colder than Earth's. Owing to the larger distance from the Sun, Mars receives less solar energy and has a lower effective temperature, which is about 210 K. The average surface emission temperature of Mars is just 215 K, which is comparable to inland Antarctica. Although Mars' atmosphere consists primarily of carbon dioxide, the greenhouse effect in the Martian atmosphere is much weaker than Earth's: 5 °C (9.0 °F) on Mars, versus 33 °C (59 °F) on Earth. This is because the total atmosphere is so thin that the partial pressure of carbon dioxide is very weak, leading to less warming. The daily range of temperature in the lower atmosphere is huge due to the low thermal inertia; it can range from −75 °C (−103 °F) to near 0 °C (32 °F) near the surface in some regions. The temperature of the upper part of the Martian atmosphere is also significantly lower than Earth's because of the absence of stratospheric ozone and the radiative cooling effect of carbon dioxide at higher altitudes.

<span class="mw-page-title-main">Terraforming of Mars</span> Hypothetical modification of Mars into a habitable planet

The terraforming of Mars or the terraformation of Mars is a hypothetical procedure that would consist of a planetary engineering project or concurrent projects, with the goal to transform Mars from a planet hostile to terrestrial life to one that can sustainably host humans and other lifeforms free of protection or mediation. The process would involve the modification of the planet's extant climate, atmosphere, and surface through a variety of resource-intensive initiatives, and the installation of a novel ecological system or systems.

<span class="mw-page-title-main">Climate of Mars</span> Climate patterns of the terrestrial planet

The climate of Mars has been a topic of scientific curiosity for centuries, in part because it is the only terrestrial planet whose surface can be easily directly observed in detail from the Earth with help from a telescope.

<span class="mw-page-title-main">Magnetospheric Multiscale Mission</span> Four NASA robots studying Earths magnetosphere (2015-present)

The Magnetospheric Multiscale (MMS) Mission is a NASA robotic space mission to study the Earth's magnetosphere, using four identical spacecraft flying in a tetrahedral formation. The spacecraft were launched on 13 March 2015 at 02:44 UTC. The mission is designed to gather information about the microphysics of magnetic reconnection, energetic particle acceleration, and turbulence⁠ — processes that occur in many astrophysical plasmas. As of March 2020, the MMS spacecraft have enough fuel to remain operational until 2040.

<span class="mw-page-title-main">Bruce Jakosky</span> American scientist

Bruce Martin Jakosky is a professor of Geological Sciences and associate director of the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado, Boulder. He has been involved with the Viking, Solar Mesosphere Explorer, Clementine, Mars Observer, Mars Global Surveyor, Mars Odyssey, Mars Science Laboratory and MAVEN spacecraft missions, and is involved in planning future spacecraft missions.

<span class="mw-page-title-main">C/2013 A1 (Siding Spring)</span> Oort cloud comet

C/2013 A1 is an Oort cloud comet discovered on 3 January 2013 by Robert H. McNaught at Siding Spring Observatory using the 0.5-meter (20 in) Uppsala Southern Schmidt Telescope.

<span class="mw-page-title-main">Heliophysics Science Division</span>

The Heliophysics Science Division of the Goddard Space Flight Center (NASA) conducts research on the Sun, its extended Solar System environment, and interactions of Earth, other planets, small bodies, and interstellar gas with the heliosphere. Division research also encompasses geospace—Earth's uppermost atmosphere, the ionosphere, and the magnetosphere—and the changing environmental conditions throughout the coupled heliosphere.

The following outline is provided as an overview of and topical guide to Mars:

SWAP (<i>New Horizons</i>)

SWAP is a science instrument aboard the unmanned New Horizons space probe, which was designed to fly by dwarf planet Pluto. SWAP was designed to record Solar Wind en route, at, and beyond Pluto. At Pluto, SWAP's purpose was to record the relationship between the solarwind and ions and/or material entering space from the atmosphere of Pluto.

<span class="mw-page-title-main">Pluto Energetic Particle Spectrometer Science Investigation</span> Instrument on the New Horizons space probe

Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI), is an instrument on the New Horizons space probe to Pluto and beyond, it is designed to measure ions and electrons. Specifically, it is focused on measuring ions escaping from the atmosphere of Pluto during the 2015 flyby. It is one of seven major scientific instruments aboard the spacecraft. The spacecraft was launched in 2006, flew by Jupiter the following year, and went onto flyby Pluto in 2015 where PEPSSI was able to record and transmit back to Earth its planned data collections.

REX (<i>New Horizons</i>)

REX or Radio Science Experiment is an experiment on the New Horizons space probe to determine various aspects of the atmosphere of Pluto during the 2015 flyby.

<span class="mw-page-title-main">Shannon Curry</span> American planetary physicist

Shannon Curry is the Principal Investigator of the NASA Mars Scout mission MAVEN. She is a planetary physicist and the Deputy Assistant Director of Planetary Science at the Space Sciences Laboratory at the University of California, Berkeley.

Jane Lee Fox is a physicist known for her research on the atmosphere of planets including Mars and Venus.

References

  1. ↑ "MAVEN". NASA's Solar System Exploration website. Retrieved 1 December 2022.
  2. ↑ 'MAVEN' Mission PowerPoint PD-icon.svg This article incorporates text from this source, which is in the public domain .
  3. ↑ Brown, Dwayne; Neal-Jones, Nancy; Zubritsky, Elizabeth (21 September 2014). "NASA's Newest Mars Mission Spacecraft Enters Orbit around Red Planet". NASA. Retrieved 22 September 2014.PD-icon.svg This article incorporates text from this source, which is in the public domain .
  4. 1 2 "MAVEN Fact Sheet" (PDF).PD-icon.svg This article incorporates text from this source, which is in the public domain .
  5. ↑ @maven2mars (28 October 2013). "Fittingly, from #Hebrew, via #Yiddish, a "maven" is a trusted expert who understands and seeks to pass knowledge on to others. #MAVEN #Mars" (Tweet). Retrieved 7 March 2015– via Twitter.{{cite web}}: CS1 maint: numeric names: authors list (link)
  6. ↑ American Heritage Dictionary of the English Language (4th ed.). Boston: Houghton Mifflin. 2000. p.  1082. ISBN   0-395-82517-2 . Retrieved 7 March 2015. A person who has special knowledge or experience; an expert.
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  12. ↑ MAVEN Mission to Investigate How Sun Steals Martian Atmosphere By Bill Steigerwald (October 5, 2010) PD-icon.svg This article incorporates text from this source, which is in the public domain .
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  14. 1 2 "MAVEN Science Orbit" . Retrieved 18 September 2020.
  15. ↑ mars.nasa.gov. "NASA's MAVEN Studies Passing Comet and Its Effects". NASA's Mars Exploration Program. Retrieved 18 September 2020.PD-icon.svg This article incorporates text from this source, which is in the public domain .
  16. ↑ mars.nasa.gov. "MAVEN Completes Commissioning And Begins Its Primary Science Mission". NASA's Mars Exploration Program. Retrieved 18 September 2020.PD-icon.svg This article incorporates text from this source, which is in the public domain .
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  18. 1 2 MAVEN – FAQ
  19. ↑ "MAVEN Celebrates One Mars Year of Science". 3 October 2016. Retrieved 25 September 2020.
  20. ↑ "MAVEN Steers Clear of Mars Moon Phobos". 2 March 2017. Retrieved 25 September 2020.
  21. 1 2 "MAVEN Uses Red Planet's Atmosphere to Change Orbit". 5 April 2019. Retrieved 25 September 2020.
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  24. ↑ MAVEN Mission Primary Structure Complete NASA (26 September 2011) PD-icon.svg This article incorporates text from this source, which is in the public domain .
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  27. ↑ Newest NASA Mars Orbiter Demonstrates Relay Prowess NASA 10 November 2014 PD-icon.svg This article incorporates text from this source, which is in the public domain .
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  29. ↑ Mitchell, D. L.; Mazelle, C.; Sauvaud, J.-A.; Thocaven, J.-J.; Rouzaud, J.; Fedorov, A.; Rouger, P.; Toublanc, D.; Taylor, E.; Gordon, D.; Robinson, M. (1 April 2016). "Solar Wind Electron Analyzer for MAVEN". Space Science Reviews. 200 (1): 495–528. doi:10.1007/s11214-015-0232-1. ISSN   1572-9672. S2CID   14670274.
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  32. ↑ McFadden, J. P.; Kortmann, O.; Curtis, D.; Dalton, G.; Johnson, G.; Abiad, R.; Sterling, R.; Hatch, K.; Berg, P.; Tiu, C.; Gordon, D. (1 December 2015). "SupraThermal and Thermal Ion Composition (STATIC) Instrument for MAVEN". Space Science Reviews. 195 (1): 199–256. doi: 10.1007/s11214-015-0175-6 . ISSN   1572-9672.
  33. ↑ Larson, Davin E.; Lillis, Robert J.; Lee, Christina O.; Dunn, Patrick A.; Hatch, Kenneth; Robinson, Miles; Glaser, David; Chen, Jianxin; Curtis, David; Tiu, Christopher; Lin, Robert P. (1 December 2015). "Solar Energetic Particle Investigation for MAVEN". Space Science Reviews. 195 (1): 153–172. doi:10.1007/s11214-015-0218-z. ISSN   1572-9672. S2CID   122683322.
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