NASA’s SOFIA Discovers Water on Sunlit Surface of Moon

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

Credits: NASA/Daniel Rutter

NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) has confirmed, for the first time, water on the sunlit surface of the Moon. This discovery indicates that water may be distributed across the lunar surface, and not limited to cold, shadowed places.

SOFIA has detected water molecules (H2O) in Clavius Crater, one of the largest craters visible from Earth, located in the Moon’s southern hemisphere. Previous observations of the Moon’s surface detected some form of hydrogen, but were unable to distinguish between water and its close chemical relative, hydroxyl (OH). Data from this location reveal water in concentrations of 100 to 412 parts per million – roughly equivalent to a 12-ounce bottle of water – trapped in a cubic meter of soil spread across the lunar surface. The results are published in the latest issue of Nature Astronomy.

“We had indications that H2O – the familiar water we know – might be present on the sunlit side of the Moon,” said Paul Hertz, director of the Astrophysics Division in the Science Mission Directorate at NASA Headquarters in Washington. “Now we know it is there. This discovery challenges our understanding of the lunar surface and raises intriguing questions about resources relevant for deep space exploration.”

As a comparison, the Sahara desert has 100 times the amount of water than what SOFIA detected in the lunar soil. Despite the small amounts, the discovery raises new questions about how water is created and how it persists on the harsh, airless lunar surface.

Water is a precious resource in deep space and a key ingredient of life as we know it. Whether the water SOFIA found is easily accessible for use as a resource remains to be determined. Under NASA’s Artemis program, the agency is eager to learn all it can about the presence of water on the Moon in advance of sending the first woman and next man to the lunar surface in 2024 and establishing a sustainable human presence there by the end of the decade.

SOFIA’s results build on years of previous research examining the presence of water on the Moon. When the Apollo astronauts first returned from the Moon in 1969, it was thought to be completely dry. Orbital and impactor missions over the past 20 years, such as NASA’s Lunar Crater Observation and Sensing Satellite, confirmed ice in permanently shadowed craters around the Moon’s poles. Meanwhile, several spacecraft – including the Cassini mission and Deep Impact comet mission, as well as the Indian Space Research Organization’s Chandrayaan-1 mission – and NASA’s ground-based Infrared Telescope Facility, looked broadly across the lunar surface and found evidence of hydration in sunnier regions. Yet those missions were unable to definitively distinguish the form in which it was present – either H2O or OH.

“Prior to the SOFIA observations, we knew there was some kind of hydration,” said Casey Honniball, the lead author who published the results from her graduate thesis work at the University of Hawaii at Mānoa in Honolulu. “But we didn’t know how much, if any, was actually water molecules – like we drink every day – or something more like drain cleaner.”

SOFIA offered a new means of looking at the Moon. Flying at altitudes of up to 45,000 feet, this modified Boeing 747SP jetliner with a 106-inch diameter telescope reaches above 99% of the water vapor in Earth’s atmosphere to get a clearer view of the infrared universe. Using its Faint Object infraRed CAmera for the SOFIA Telescope (FORCAST), SOFIA was able to pick up the specific wavelength unique to water molecules, at 6.1 microns, and discovered a relatively surprising concentration in sunny Clavius Crater.

“Without a thick atmosphere, water on the sunlit lunar surface should just be lost to space,” said Honniball, who is now a postdoctoral fellow at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “Yet somehow we’re seeing it. Something is generating the water, and something must be trapping it there.”

Several forces could be at play in the delivery or creation of this water. Micrometeorites raining down on the lunar surface, carrying small amounts of water, could deposit the water on the lunar surface upon impact. Another possibility is there could be a two-step process whereby the Sun’s solar wind delivers hydrogen to the lunar surface and causes a chemical reaction with oxygen-bearing minerals in the soil to create hydroxyl. Meanwhile, radiation from the bombardment of micrometeorites could be transforming that hydroxyl into water.

How the water then gets stored – making it possible to accumulate – also raises some intriguing questions. The water could be trapped into tiny beadlike structures in the soil that form out of the high heat created by micrometeorite impacts. Another possibility is that the water could be hidden between grains of lunar soil and sheltered from the sunlight – potentially making it a bit more accessible than water trapped in beadlike structures.

For a mission designed to look at distant, dim objects such as black holes, star clusters, and galaxies, SOFIA’s spotlight on Earth’s nearest and brightest neighbor was a departure from business as usual. The telescope operators typically use a guide camera to track stars, keeping the telescope locked steadily on its observing target. But the Moon is so close and bright that it fills the guide camera’s entire field of view. With no stars visible, it was unclear if the telescope could reliably track the Moon. To determine this, in August 2018, the operators decided to try a test observation.

“It was, in fact, the first time SOFIA has looked at the Moon, and we weren’t even completely sure if we would get reliable data, but questions about the Moon’s water compelled us to try,” said Naseem Rangwala, SOFIA’s project scientist at NASA's Ames Research Center in California's Silicon Valley. “It’s incredible that this discovery came out of what was essentially a test, and now that we know we can do this, we’re planning more flights to do more observations.”

SOFIA’s follow-up flights will look for water in additional sunlit locations and during different lunar phases to learn more about how the water is produced, stored, and moved across the Moon. The data will add to the work of future Moon missions, such as NASA’s Volatiles Investigating Polar Exploration Rover (VIPER), to create the first water resource maps of the Moon for future human space exploration.

In the same issue of Nature Astronomy, scientists have published a paper using theoretical models and NASA's Lunar Reconnaissance Orbiter data, pointing out that water could be trapped in small shadows, where temperatures stay below freezing, across more of the Moon than currently expected. The results can be found here.

“Water is a valuable resource, for both scientific purposes and for use by our explorers,” said Jacob Bleacher, chief exploration scientist for NASA’s Human Exploration and Operations Mission Directorate. “If we can use the resources at the Moon, then we can carry less water and more equipment to help enable new scientific discoveries.”

SOFIA is a joint project of NASA and the German Aerospace Center. Ames manages the SOFIA program, science, and mission operations in cooperation with the Universities Space Research Association, headquartered in Columbia, Maryland, and the German SOFIA Institute at the University of Stuttgart. The aircraft is maintained and operated by NASA’s Armstrong Flight Research Center Building 703, in Palmdale, California.

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NASA Takes Delivery of First All-Electric Experimental Aircraft

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

NASA’s X-57 Maxwell, the agency’s first
all-electric X-plane and first crewed X-planed
in two decades. Credit NASA.

The first all-electric configuration of NASA’s X-57 Maxwell now is at the agency’s Armstrong Flight Research Center in Edwards, California.

The X-57, NASA’s first all-electric experimental aircraft, or X-plane – and the first crewed X-plane in two decades – was delivered by Empirical Systems Aerospace (ESAero) of San Luis Obispo, California on Wednesday, Oct. 2, in the first of three configurations as an all-electric aircraft, known as Modification II, or Mod II.

The X-57’s Mod II vehicle features the replacement of traditional combustion engines on a baseline Tecnam P2006T aircraft, with electric cruise motors. The delivery is a major milestone for the project, allowing NASA engineers to begin putting the aircraft through ground tests, to be followed by taxi tests and eventually, flight tests.

"The X-57 Mod II aircraft delivery to NASA is a significant event, marking the beginning of a new phase in this exciting electric X-plane project,” said X-57 Project Manager Tom Rigney. “With the aircraft in our possession, the X-57 team will soon conduct extensive ground testing of the integrated electric propulsion system to ensure the aircraft is airworthy. We plan to rapidly share valuable lessons learned along the way as we progress toward flight testing, helping to inform the growing electric aircraft market.”

While X-57’s Mod II vehicle begins systems validation testing on the ground, efforts in preparation for the project’s following phases, Mods III and IV, are already well underway, with the recent successful completion of loads testing on a new, high-aspect ratio wing at NASA Armstrong’s Flight Loads Laboratory. Following completion of tests, the wing, which will be featured on Mods III and IV configurations, will undergo fit checks on a fuselage at ESAero, ensuring timely transition from the project’s Mod II phase to Mod III.

“ESAero is thrilled to be delivering the MOD II X-57 Maxwell to NASA AFRC,” said ESAero President and CEO Andrew Gibson. “In this revolutionary time, the experience and lessons learned, from early requirements to current standards development, has the X-57 paving the way. This milestone, along with receiving the successfully load-tested MOD III wing back, will enable NASA, ESAero and the small business team to accelerate and lead electric air vehicle distributed propulsion development on the MOD III and MOD IV configurations with integration at our facilities in San Luis Obispo.”

A goal of the X-57 project is to help develop certification standards for emerging electric aircraft markets, including urban air mobility vehicles, which also rely on complex distributed electric propulsion systems. NASA will share the aircraft’s electric-propulsion-focused design and airworthiness process with regulators and industry, which will advance certification approaches for aircraft utilizing distributed electric propulsion.

The X-57 team is using a “design driver” as a technical challenge, to drive lessons learned and best practices. This design driver includes a 500% increase in high-speed cruise efficiency, zero in-flight carbon emissions, and flight that is much quieter for communities on the ground.

The X-57 project operates under the Integrated Aviation Systems Program’s Flight Demonstrations and Capabilities project, within NASA’s Aeronautics Research Mission Directorate.

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NASA's Dragonfly Drone Will Fly Around Titan

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

Dragonfly rotorcraft-lander approaching a site on
Saturn’s exotic moon, Titan. Taking advantage of
Titan’s dense atmosphere and low gravity, Dragonfly
will explore dozens of locations across the icy world,
sampling and measuring the compositions of Titan's
organic surface materials to characterize the
habitability of Titan’s environment and investigate
the progression of prebiotic chemistry.
Credits: NASA/JHU-APL

NASA has announced that our next destination in the solar system is the unique, richly organic world Titan. Advancing our search for the building blocks of life, the Dragonfly mission will fly multiple sorties to sample and examine sites around Saturn’s icy moon.

Dragonfly will launch in 2026 and arrive in 2034. The rotorcraft will fly to dozens of promising locations on Titan looking for prebiotic chemical processes common on both Titan and Earth. Dragonfly marks the first time NASA will fly a multi-rotor vehicle for science on another planet; it has eight rotors and flies like a large drone. It will take advantage of Titan’s dense atmosphere – four times denser than Earth’s – to become the first vehicle ever to fly its entire science payload to new places for repeatable and targeted access to surface materials.

Titan is an analog to the very early Earth, and can provide clues to how life may have arisen on our planet. During its 2.7-year baseline mission, Dragonfly will explore diverse environments from organic dunes to the floor of an impact crater where liquid water and complex organic materials key to life once existed together for possibly tens of thousands of years. Its instruments will study how far prebiotic chemistry may have progressed. They also will investigate the moon’s atmospheric and surface properties and its subsurface ocean and liquid reservoirs. Additionally, instruments will search for chemical evidence of past or extant life.

“With the Dragonfly mission, NASA will once again do what no one else can do,” said NASA Administrator Jim Bridenstine. “Visiting this mysterious ocean world could revolutionize what we know about life in the universe. This cutting-edge mission would have been unthinkable even just a few years ago, but we’re now ready for Dragonfly’s amazing flight.”

Dragonfly took advantage of 13 years’ worth of Cassini data to choose a calm weather period to land, along with a safe initial landing site and scientifically interesting targets. It will first land at the equatorial “Shangri-La” dune fields, which are terrestrially similar to the linear dunes in Namibia in southern Africa and offer a diverse sampling location. Dragonfly will explore this region in short flights, building up to a series of longer “leapfrog” flights of up to 5 miles (8 kilometers), stopping along the way to take samples from compelling areas with diverse geography. It will finally reach the Selk impact crater, where there is evidence of past liquid water, organics – the complex molecules that contain carbon, combined with hydrogen, oxygen, and nitrogen – and energy, which together make up the recipe for life. The lander will eventually fly more than 108 miles (175 kilometers) – nearly double the distance traveled to date by all the Mars rovers combined.

“Titan is unlike any other place in the solar system, and Dragonfly is like no other mission,” said Thomas Zurbuchen, NASA’s associate administrator for Science at the agency’s Headquarters in Washington. “It’s remarkable to think of this rotorcraft flying miles and miles across the organic sand dunes of Saturn’s largest moon, exploring the processes that shape this extraordinary environment. Dragonfly will visit a world filled with a wide variety of organic compounds, which are the building blocks of life and could teach us about the origin of life itself.”

Titan has a nitrogen-based atmosphere like Earth. Unlike Earth, Titan has clouds and rain of methane. Other organics are formed in the atmosphere and fall like light snow. The moon’s weather and surface processes have combined complex organics, energy, and water similar to those that may have sparked life on our planet.

Titan is larger than the planet Mercury and is the second largest moon in our solar system. As it orbits Saturn, it is about 886 million miles (1.4 billion kilometers) away from the Sun, about 10 times farther than Earth. Because it is so far from the Sun, its surface temperature is around -290 degrees Fahrenheit (-179 degrees Celsius). Its surface pressure is also 50 percent higher than Earth’s.

Dragonfly was selected as part of the agency’s New Frontiers program, which includes the New Horizons mission to Pluto and the Kuiper Belt, Juno to Jupiter, and OSIRIS-REx to the asteroid Bennu. Dragonfly is led by Principal Investigator Elizabeth Turtle, who is based at Johns Hopkins University’s Applied Physics Laboratory in Laurel, Maryland. New Frontiers supports missions that have been identified as top solar system exploration priorities by the planetary community. The program is managed by the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Planetary Science Division in Washington.

“The New Frontiers program has transformed our understanding of the solar system, uncovering the inner structure and composition of Jupiter’s turbulent atmosphere, discovering the icy secrets of Pluto’s landscape, revealing mysterious objects in the Kuiper belt, and exploring a near-Earth asteroid for the building blocks of life,” said Lori Glaze, director of NASA’s Planetary Science Division. “Now we can add Titan to the list of enigmatic worlds NASA will explore.”

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Israeli Space Tech Firm hiSky Expands to the UK

Peter Thomas -
L o n d o n ,   U K - 

Harwell Campus

An innovative company looking to make satellite communications more accessible and affordable is set to create over 100 high-tech jobs in London and Oxfordshire.

The Israeli company hiSky has established a UK limited company - hiSkySat Limited – based in London, with an R&D centre at Harwell to develop a satellite communications network management system (NMS) and operation centre.

The UK Space Agency provided £9 million of funding for hiSky to develop cutting-edge space telecoms technology at the Harwell Space Cluster, which is growing fast and already home to more than 90 space companies.

hiSky aims to be the world’s first low-cost satellite network operator, bringing innovative technology to voice and data satellite communications, and leveraging existing satellite capacity to reduce costs associated with building and launching new satellites.

Part of the new project will integrate and develop 5G networks into their ‘Smartellite’ satellite receiving terminal and carry out a demonstration to show how it can connect seamlessly between different satellites and operators. This will help roll out the next generation of Internet of Things technology, connecting machines and vehicles around the world and enabling remote monitoring of infrastructure such as power lines and wind turbines.

Science Minister Chris Skidmore said:

“The UK government’s modern Industrial Strategy and commitment to the European Space Agency are bringing innovative companies like OneWeb, SatixFy and hiSky to Britain."

“Our world-leading universities, modern regulatory environment, growing R&D spend and support for UK spaceports make this a great place to build a space business and create the high-skilled jobs of the future."

The UK Space Agency funding is allocated through the European Space Agency (ESA). This is targeted to support the development of hiSky’s satellite receiving terminals, operations and management software for the devices and to help establish hiSky as a Virtual Network Operator – a supplier of network services using existing infrastructure – in the UK.

Shahar Kravitz , CEO, hiSky said:

“We are honored to be partners with the UK Space Agency. It is our privilege to establish the first real low-cost global Virtual Satellite Network and to do it in the UK. hiSky’s cutting edge technology and solution was developed in order to meet with the consumers needs and can easily adjust to different satellite operators, including forthcoming Low Earth Orbit telcoms constellations."

“The UK Space Agency and Department for International Trade have been very supportive of our technology and our concept from the beginning. We are grateful for the chance given to us and look forward to grow within the UK."

ESA is independent of the European Union and has its European Centre for Space Applications and Telecommunications (ECSAT) in Harwell, Oxfordshire, reflecting the UK’s world-leading position in satellite communications.

Magali Vaissiere, ESA Director of Telecommunications and Integrated Applications said:

“Innovation and collaboration are the keys to keeping European industry at the forefront of the highly competitive global market for satellite communications. This is a great example of how partnering between the public and private sectors can drive the development of world-leading innovation."

Earlier this month the government announced ambitious plans for the UK to lead the new space age, including further support to enable small satellite launch and the creation of a new National Space Council to strengthen UK space strategy.

The UK’s investment in the ESA programme for telecommunications research and business applications (ARTES) has helped bring world-leading companies to the UK such as OneWeb and SatixFy.

The UK Space Agency, ESA and the Department for International Trade have worked together to bring hiSky to the UK.

The Harwell Space Cluster has grown by 19% over the past year, employing 950 people in 89 organisations including RAL Space, Oxford Space Systems and the Satellite Applications Catapult.

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Asteroid Mining not a Million Miles Away

Avi Cohen  -   
A d e l a i d e ,   A u s t r a l i a - 

Mining Asteroids is no longer science fiction.

Work by a team of University of Adelaide scientists to perfect metal and mineral extraction processes is bringing the possibility of mining the wealth contained within asteroids closer to reality. But science fiction won’t become fact until asteroid mining becomes economically as well as technically viable.

“Asteroids such as Bennu are closer to us than Adelaide is to Alice Springs about 1000 kilometres away in Earth’s near orbit,” says Professor Volker Hessel, Deputy Dean-Research from the University of Adelaide’s Faculty of Engineering, Computer & Mathematical Sciences (ECMS) and Professor in the School of Chemical Engineering.

“Advances in space exploration mean that these bodies which contain nickel, cobalt, and platinum as well as water and organic matter, are now within reach.”

Professor Hessel is developing an intensified continuous-flow metal solvent extraction process which is faster and more selective than existing processes and is fine-tuned to the specific raw materials found in asteroids.

“Continuous-flow chemistry is proven technology. The process extracts metal by mixing and separating solvents. Successive passes of the chemicals through the process results in complete extraction of the metals,” he says.

“Asteroid-born metals co-exist in different combinations and concentrations from those found in terrestrial rock, so one of the challenges that the team has is understanding how these may be successfully extracted. This new disruptive technology is needed as traditional technology does not provide the solution.”

The continuous-flow technology is scalable and can operate in zero gravity and a vacuum which makes space mineral extraction a reality. Professor Hessel’s US partner Space Tango is developing expanded flow chemistry capabilities in orbit. On 4 May they launched a mission that included, on board, the first processing lab assessing liquid separation. An array of space-focused companies is eyeing up the vast potential rewards on offer from the trillions of asteroids each worth millions of dollars in raw materials.

Professor Volker Hessel, Deputy Dean-Research from
the University of Adelaide’s Faculty of Engineering,
Computer & Mathematical Sciences (ECMS) and
Professor in the School of Chemical Engineering

“In the same way that colonialists and explorers exploited the resources of the New World about 400 years ago, today’s pioneering asteroid miners are reaching out to exploit riches in space,” says Professor Hessel.

“There are 17 missions currently underway for space resource exploitation. The NASA OSIRIS-Rex mission to Bennu asteroid will return with samples in 2023.

“Continuous-flow chemistry technology must be perfected to use as little water as possible. While launching costs are projected to fall in the mid-term, they will remain a serious point to consider. Instead of needing hundreds of tonnes of water to extract one tonne of metal, development of the technology may mean that less than 10 tonnes are required.

“Many alternative approaches are being investigated such as realigning asteroid orbits to make them more accessible, processing on the Moon, Mars or lower Earth orbit using available water, and processing on asteroids themselves or in the near-Earth orbit.

“Under the umbrella of the University’s ECMS Faculty space theme and our In-Situ Resource Utilisation (ISRU) laboratory we aim to perfect metal extraction technology using continuous-flow chemistry. This is only one piece of our holistic approach to the in-situ resource utilisation puzzle.

“Exploitation of the wealth locked up in asteroids will only become a reality when other disruptive elements come together and it is economically as well as technically viable,” says Professor Hessel.

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NASA Opens International Space Station to New Commercial Opportunities and Private Astronauts

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

Sunrise from the International Space Station

NASA is opening the International Space Station for commercial business so U.S. industry innovation and ingenuity can accelerate a thriving commercial economy in low-Earth orbit.

This move comes as NASA focuses full speed ahead on its goal of landing the first woman and next man on the Moon by 2024, where American companies also will play an essential role in establishing a sustainable presence.

NASA officials, including the agency’s Chief Financial Officer Jeff DeWit, will discuss details of the five-part near-term plan in a news conference at 10 a.m. EDT today. The news conference will air live on NASA Television and the agency’s website.

NASA will continue research and testing in low-Earth orbit to inform its lunar exploration plans, while also working with the private sector to test technologies, train astronauts and strengthen the burgeoning space economy. Providing expanded opportunities at the International Space Station to manufacture, market and promote commercial products and services will help catalyze and expand space exploration markets for many businesses.

The agency’s ultimate goal in low-Earth orbit is to partner with industry to achieve a strong ecosystem in which NASA is one of many customers purchasing services and capabilities at lower cost.

NASA will land the first woman on the Moon by 2024

NASA’s plan addresses both the supply-side and demand-side for a new economy, enabling use of government resources for commercial activities, creating the opportunity for private astronaut missions to the space station, enabling commercial destinations in low-Earth orbit, identifying and pursuing activities that foster new and emerging markets, and quantifying NASA’s long-term demand for activities in low-Earth orbit.

More than 50 companies already are conducting commercial research and development on the space station via the International Space Station U.S. National Laboratory, and their results are yielding great promise. In addition, NASA has worked with 11 different companies to install 14 commercial facilities on the station that support research and development projects for NASA and the ISS National Lab.

This effort is intended to broaden the scope of commercial activity on the space station beyond the ISS National Lab mandate, which is limited to research and development. A new NASA directive will enable commercial manufacturing and production and allow both NASA and private astronauts to conduct new commercial activities aboard the orbiting laboratory. The directive also sets prices for industry use of U.S. government resources on the space station for commercial and marketing activities.

Pricing released Friday is specific to commercial and marketing activities enabled by the new directive, reflects a representative cost to NASA, and is designed to encourage the emergence of new markets. As NASA learns how these new markets respond, the agency will reassess the pricing and amount of available resources approximately every six months and make adjustments as necessary.

To qualify, commercial and marketing activities must either:

• require the unique microgravity environment to enable manufacturing, production or development of a commercial application;
• have a connection to NASA’s mission; or
• support the development of a sustainable low-Earth orbit economy.

NASA’s directive enabling commercial and marketing activities aboard the space station addresses manufacturing, production, transportation, and marketing of commercial resources and goods, including products intended for commercial sale on Earth. NASA astronauts will be able to conduct coordinated, scheduled and reimbursable commercial and marketing activities consistent with government ethics requirements aboard the station.

To ensure a competitive market, NASA initially is making available five percent of the agency’s annual allocation of crew resources and cargo capability, including 90 hours of crew time and 175 kg of cargo launch capability, but will limit the amount provided to any one company.

NASA also is enabling private astronaut missions of up to 30 days on the International Space Station to perform duties that fall into the approved commercial and marketing activities outlined in the directive released Friday, with the first mission as early as 2020. A new NASA Research Announcement focus area issued today outlines the path for those future private astronaut missions.

The International Space Station

If supported by the market, the agency can accommodate up to two short-duration private astronaut missions per year to the International Space Station. These missions will be privately funded, dedicated commercial spaceflights. Private astronaut missions will use a U.S. spacecraft developed under NASA’s Commercial Crew Program.

The commercial entity developing the mission will determine crew composition for each mission and ensure private astronauts meet NASA’s medical standards and the training and certification procedures for International Space Station crew members. Market studies identified private astronaut missions to low-Earth orbit as a key element to demonstrate demand and reduce risk for future commercial destinations in low-Earth orbit.

In the long-term, NASA’s goal is to become one of many customers purchasing services from independent, commercial and free-flying habitable destinations in low-Earth orbit. A robust low-Earth orbit economy will need multiple commercial destinations, and NASA is partnering with industry to pursue dual paths to that objective that either go through the space station or directly to a free-flying destination.

As a first step, NASA is making one space station port and utilities available for industry to attach a commercial module to support commercial activities, and today is releasing a synopsis as Appendix I in NASA’s Next Space Technologies for Exploration Partnerships (NextSTEP) 2 Broad Agency Announcement (BAA). NASA expects to release the solicitation June 14, with awards made by the end of the fiscal year. The forward port of the station’s Harmony module will be available to industry for a finite period of time.

NASA will follow up with a synopsis for NextSTEP 2 Appendix K in July to partner with industry in the development of future free-flying commercial stations in low-Earth orbit.

NASA continues to seek and pursue opportunities to stimulate sustainable commercial demand in low-Earth orbit and, to that end, has added two new focus areas to the NASA Research Announcement soliciting proposals for commercial concepts. these focus areas include in-space manufacturing, regenerative medicine, bioengineering, and other fields that may lead to a scalable, financially self-sustaining demand for low-Earth orbit capabilities.

In addition, NASA is seeking targeted studies to better understand real and perceived barriers of potential new market entrants and to address broad ideas which could help stimulate demand. Successful proposals will define the path to broadly foster market growth, provide data-driven rationale to support the defined path, and lead to recommendations on which NASA, industry or other organizations could act. More details are available in the synopsis for NextSTEP 2 BAA Appendix J. NASA expects to release the solicitation for Appendix J on June 14 with awards made by the end of the fiscal year.

NASA also is working to increase the research and development community’s understanding of the potential value of microgravity research and the path to conducting research in low-Earth orbit by coordinating across the microgravity community to lower barriers to entry and refinement of research via drop towers, parabolic, and suborbital flights.

Astronaut Karen Nyberg Works with a Plant
Experiment aboard the International Space Station

NASA is providing a forecast of its minimum long-term, low-Earth orbit requirements, representing the type and amount of services that NASA intends to purchase when those services become commercially available. The goal is to reduce uncertainty for commercial destination providers about NASA as a customer, and to help them make decisions about which NASA requirements they are interested in fulfilling.

NASA also is providing details and estimated quantities for NASA crew accommodation, human research, biological and physical science research, technology demonstrations, and hosted science instruments. In addition, NASA intends to continue purchasing services for a national laboratory capability in low-Earth orbit. For example, NASA’s strategy research in the areas of space biology, physical sciences, and fundamental physics is driven by recommendations from the National Academy of Sciences (NAS).

Fundamental research and applied exploration research are not mutually exclusive, and advances in one area often enable advancements in the other. NASA’s Space Life and Physical Sciences Research Applications division has identified the highest research priorities for long-term use of low-Earth orbit: in life sciences, the priorities are studies of plants, model organisms, and of the microbiome of the built environment; and in physical sciences, the priorities are studies into combustion and phase change-associated energy transfer.

For more than 18 years, humans have lived and worked aboard the International Space Station, conducting thousands of experiments in areas such as human research, biology, and physical science, as well as advanced technology development. Many of these experiments, conducted via the ISS National Lab, have been research and development with commercial objectives. New opportunities are needed to move beyond research and development, and the station will play an essential role in enabling those opportunities for new commercial markets needed to build a sustainable ecosystem in low-Earth orbit.

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Maxar Technologies Awarded Artemis Lunar Gateway Power and Propulsion Contract by NASA

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

The power and propulsion element of NASA's
Gateway is a high-power, 50-kilowatt solar electric
propulsion spacecraft – three times more powerful
than current capabilities. Credits: NASA

In one of the first steps of the agency’s Artemis lunar exploration plans, NASA announced on Thursday the selection of Maxar Technologies, formerly SSL, in Westminster, Colorado, to develop and demonstrate power, propulsion and communications capabilities for NASA’s lunar Gateway.

“The power and propulsion element is the foundation of Gateway and a fine example of how partnerships with U.S. companies can help expedite NASA’s return to the Moon with the first woman and next man by 2024,” said NASA Administrator Jim Bridenstine. “It will be the key component upon which we will build our lunar Gateway outpost, the cornerstone of NASA’s sustainable and reusable Artemis exploration architecture on and around the Moon.”

The power and propulsion element is a high-power, 50-kilowatt solar electric propulsion spacecraft – three times more powerful than current capabilities. As a mobile command and service module, the Gateway provides a communications relay for human and robotic expeditions to the lunar surface, starting at the Moon’s South Pole.

This firm-fixed price award includes an indefinite-delivery/indefinite-quantity portion and carries a maximum total value of $375 million. The contract begins with a 12-month base period of performance and is followed by a 26-month option, a 14-month option and two 12-month options.

The power and propulsion element provides a
communications relay capability for NASA's
Gateway, enabling it to serve as a mobile command
and service module for human and robotic
expeditions to the lunar surface. Credits: NASA

Spacecraft design will be completed during the base period, after which the exercise of options will provide for the development, launch, and in-space flight demonstration. The flight demonstration will last as long as one year, during which the spacecraft will be fully owned and operated by Maxar. Following a successful demonstration, NASA will have the option to acquire the spacecraft for use as the first element of the Gateway. NASA is targeting launch of the power and propulsion element on a commercial rocket in late 2022.

“We’re excited to demonstrate our newest technology on the power and propulsion element. Solar electric propulsion is extremely efficient, making it perfect for the Gateway,” said Mike Barrett, power and propulsion element project manager at NASA’s Glenn Research Center in Cleveland. “This system requires much less propellant than traditional chemical systems, which will allow the Gateway to move more mass around the Moon, like a human landing system and large modules for living and working in orbit.”

Charged with returning to the Moon within five years, NASA’s lunar exploration plans are based on a two-phase approach: the first is focused on speed – landing on the Moon by 2024 – while the second will establish a sustained human presence on and around the Moon by 2028. We then will use what we learn on the Moon to prepare to send astronauts to Mars.

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Massive Martian Ice Deposit Discovered Under Red Planet's North Pole

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

An exaggerated view of Mars' north polar cap.
Researchers with The University of Texas at Austin
and the University of Arizona estimate that if melted,
the massive ice deposits discovered in this region
would cover the planet in 1.5 meters (5 feet) of water.
Image: SA/DLR/FU Berlin; NASA MGS MOLA

Newly discovered layers of ice buried a mile beneath Mars' north pole are the remnants of ancient polar ice sheets and could be one of the largest water reservoirs on the planet, according to scientists at The University of Texas at Austin and the University of Arizona.

The team made the discovery using measurements gathered by the Shallow Radar (SHARAD) on NASA's Mars Reconnaissance Orbiter (MRO). SHARAD emits radar waves that can penetrate up to a mile and a half beneath the surface of Mars.

The findings, published May 22 in Geophysical Research Letters, are important because the layers of ice are a record of past climate on Mars in much the same way that tree rings are a record of past climate on Earth. Studying the geometry and composition of these layers could tell scientists whether climate conditions were previously favorable for life, researchers said. The team found layers of sand and ice that were as much as 90% water in some places.

If melted, the newly discovered polar ice would be equivalent to a global layer of water around Mars at least 1.5 meters (5 feet) deep.

"We didn't expect to find this much water ice here," said lead author Stefano Nerozzi, a graduate research assistant at the University of Texas Institute for Geophysics (UTIG) who is completing his Ph.D. at the Jackson School of Geosciences. "That likely makes it the third largest water reservoir on Mars after the polar ice caps."

The findings were corroborated by an independent study using gravity data instead of radar, led by researchers at Johns Hopkins University. Nerozzi was a co-author. The papers have been published simultaneously in Geophysical Research Letters.

The authors think that the layers formed when ice accumulated at the poles during past ice ages on Mars. Each time the planet warmed, a remnant of the ice caps became covered by sand, which protected the ice from solar radiation and prevented it from dissipating into the atmosphere.

Scientists have long known about glacial events on Mars, which are driven by variations in the planet's orbit and tilt. Over periods of about 50,000 years, Mars leans toward the sun before gradually returning to an upright position, like a wobbling spinning top. When the planet spins upright, the equator faces the sun, allowing the polar ice caps to grow. As the planet tilts, the ice caps retreat, perhaps vanishing entirely.

Until now, scientists thought that the ancient ice caps were lost. The paper shows that in fact significant ice sheet remnants have survived under the planet's surface, trapped in alternating bands of ice and sand, like layers on a cake.

Co-author Jack Holt, a professor at the Lunar & Planetary Laboratory of the University of Arizona, said that the study provides new, important insights into the exchange of water ice between the poles and the midlatitudes, where his research group previously confirmed the presence of widespread glaciers, also using the SHARAD instrument.

"Surprisingly, the total volume of water locked up in these buried polar deposits is roughly the same as all the water ice known to exist in glaciers and buried ice layers at lower latitudes on Mars, and they are approximately the same age," he said.

Holt, who was a UTIG scientist and research professor for 19 years before joining the University of Arizona in 2018, has been a co-investigator with SHARAD since the spacecraft arrived at Mars in 2006.

Nerozzi said that studying this record of past polar glaciation could help determine whether Mars was ever habitable.

"Understanding how much water was available globally versus what's trapped in the poles is important if you're going to have liquid water on Mars," Nerozzi said. "You can have all the right conditions for life, but if most of the water is locked up at the poles, then it becomes difficult to have sufficient amounts of liquid water near the equator."

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Spinning Black Hole Sprays Light-Speed Plasma Clouds into Space

Avi Cohen  -   
S y d n e y ,   A u s t r a l i a - 

Artist’s impression of V404 Cygni seen close up.
The binary star system consists of a normal star in
orbit with a black hole. Material from the star falls
towards the black hole and spirals inwards in an
accretion disk, with powerful jets being launched
from the inner regions close to the black hole.
Credit: ICRAR

Astronomers have discovered rapidly swinging jets coming from a black hole almost 8000 light-years from Earth.

Published today in the journal Nature, the research shows jets from V404 Cygni’s black hole behaving in a way never seen before on such short timescales. The jets appear to be rapidly rotating with high-speed clouds of plasma—potentially just minutes apart—shooting out of the black hole in different directions.

Lead author Associate Professor James Miller-Jones, from the Curtin University node of the International Centre for Radio Astronomy Research (ICRAR), said black holes are some of the most extreme objects in the Universe.

“This is one of the most extraordinary black hole systems I’ve ever come across,” Associate Professor Miller-Jones said.

“Like many black holes, it’s feeding on a nearby star, pulling gas away from the star and forming a disk of material that encircles the black hole and spirals towards it under gravity.

“What’s different in V404 Cygni is that we think the disk of material and the black hole are misaligned.

“This appears to be causing the inner part of the disk to wobble like a spinning top and fire jets out in different directions as it changes orientation.”

V404 Cygni was first identified as a black hole in 1989 when it released a big outburst of jets and radiation. Astronomers looking at archival photographic plates then found previous outbursts in observations from 1938 and 1956.

Associate Professor Miller-Jones said that when V404 Cygni experienced another very bright outburst in 2015, lasting for two weeks, telescopes around the world tuned in to study what was going on.

“Everybody jumped on the outburst with whatever telescopes they could throw at it,” he said.

“So we have this amazing observational coverage.”

When Associate Professor Miller-Jones and his team studied the black hole, they saw its jets behaving in a way never seen before. Where jets are usually thought to shoot straight out from the poles of black holes, these jets were shooting out in different directions at different times. They were changing direction very quickly—over no more than a couple of hours.

Associate Professor Miller-Jones said the change in the movement of the jets was because of the accretion disk—the rotating disk of matter around a black hole. He said V404 Cygni’s accretion disk is 10 million kilometres wide, and the inner few thousand kilometres was puffed up and wobbling during the bright outburst.

Artist’s impression of jet ejections in V404 Cygni.
With our radio telescopes, we see individual bright
clouds of plasma that have been ejected from the
innermost regions, and redirected by the puffed-up
inner accretion disk. Credit: ICRAR

“The inner part of the accretion disk was precessing and effectively pulling the jets around with it,” Associate Professor Miller-Jones said.

“You can think of it like the wobble of a spinning top as it slows down—only in this case, the wobble is caused by Einstein’s theory of general relativity.”

The research used observations from the Very Long Baseline Array, a continent-sized radio telescope made up of 10 dishes across the United States, from the Virgin Islands in the Caribbean to Hawaii.

Co-author Alex Tetarenko—a recent PhD graduate from the University of Alberta and currently an East Asian Observatory Fellow working in Hawaii—said the speed the jets were changing direction meant the scientists had to use a very different approach to most radio observations.

“Typically, radio telescopes produce a single image from several hours of observation,” she said.

“But these jets were changing so fast that in a four-hour image we just saw a blur.

“It was like trying to take a picture of a waterfall with a one-second shutter speed.”

Instead, the researchers produced 103 individual images, each about 70 seconds long, and joined them together into a movie.

“It was only by doing this that we were able to see these changes over a very short time period,” Dr Tetarenko said.

Study co-author Dr Gemma Anderson, who is also based at ICRAR’s Curtin University node, said the wobble of the inner accretion disk could happen in other extreme events in the Universe too.

“Anytime you get a misalignment between the spin of a black hole and the material falling in, you would expect to see this when a black hole starts feeding very rapidly,” Dr Anderson said.

“That could include a whole bunch of other bright, explosive events in the Universe, such as supermassive black holes feeding very quickly or tidal disruption events, when a black hole shreds a star.”

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Astronomers Capture First Image of a Black Hole

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

Credit: Event Horizon Telescope Collaboration

An international collaboration presents paradigm-shifting observations of the gargantuan black hole at the heart of distant galaxy Messier 87.

The Event Horizon Telescope (EHT) — a planet-scale array of eight ground-based radio telescopes forged through international collaboration — was designed to capture images of a black hole. Today, in coordinated press conferences across the globe, EHT researchers reveal that they have succeeded, unveiling the first direct visual evidence of a supermassive black hole and its shadow.

Scientists have obtained the first image of a black hole, using Event Horizon Telescope observations of the center of the galaxy M87. The image [above] shows a bright ring formed as light bends in the intense gravity around a black hole that is 6.5 billion times more massive than the Sun. This long-sought image provides the strongest evidence to date for the existence of supermassive black holes and opens a new window onto the study of black holes, their event horizons, and gravity.

This breakthrough was announced today in a series of six papers published in a special issue of The Astrophysical Journal Letters. The image reveals the black hole at the center of Messier 87, a massive galaxy in the nearby Virgo galaxy cluster. This black hole resides 55 million light-years from Earth and has a mass 6.5 billion times that of the Sun.

The EHT links telescopes around the globe to form an Earth-sized virtual telescope with unprecedented sensitivity and resolution. The EHT is the result of years of international collaboration, and offers scientists a new way to study the most extreme objects in the Universe predicted by Einstein’s general relativity during the centennial year of the historic experiment that first confirmed the theory.

“We have taken the first picture of a black hole," said EHT project director Sheperd S. Doeleman of the Center for Astrophysics | Harvard & Smithsonian. “This is an extraordinary scientific feat accomplished by a team of more than 200 researchers."

Black holes are extraordinary cosmic objects with enormous masses but extremely compact sizes. The presence of these objects affects their environment in extreme ways, warping spacetime and super-heating any surrounding material.

“If immersed in a bright region, like a disc of glowing gas, we expect a black hole to create a dark region similar to a shadow — something predicted by Einstein’s general relativity that we’ve never seen before, explained chair of the EHT Science Council Heino Falcke of Radboud University, the Netherlands. "This shadow, caused by the gravitational bending and capture of light by the event horizon, reveals a lot about the nature of these fascinating objects and allowed us to measure the enormous mass of M87’s black hole."

Multiple calibration and imaging methods have revealed a ring-like structure with a dark central region — the black hole’s shadow — that persisted over multiple independent EHT observations.

“Once we were sure we had imaged the shadow, we could compare our observations to extensive computer models that include the physics of warped space, superheated matter and strong magnetic fields. Many of the features of the observed image match our theoretical understanding surprisingly well," remarks Paul T.P. Ho, EHT Board member and Director of the East Asian Observatory. “This makes us confident about the interpretation of our observations, including our estimation of the black hole’s mass."

Creating the EHT was a formidable challenge which required upgrading and connecting a worldwide network of eight pre-existing telescopes deployed at a variety of challenging high-altitude sites. These locations included volcanoes in Hawai`i and Mexico, mountains in Arizona and the Spanish Sierra Nevada, the Chilean Atacama Desert, and Antarctica.

The EHT observations use a technique called very-long-baseline interferometry (VLBI) which synchronises telescope facilities around the world and exploits the rotation of our planet to form one huge, Earth-size telescope observing at a wavelength of 1.3 mm. VLBI allows the EHT to achieve an angular resolution of 20 micro-arcseconds — enough to read a newspaper in New York from a sidewalk café in Paris.

The telescopes contributing to this result were ALMA, APEX, the IRAM 30-meter telescope, the James Clerk Maxwell Telescope, the Large Millimeter Telescope Alfonso Serrano, the Submillimeter Array, the Submillimeter Telescope, and the South Pole Telescope. Petabytes of raw data from the telescopes were combined by highly specialised supercomputers hosted by the Max Planck Institute for Radio Astronomy and MIT Haystack Observatory.

The construction of the EHT and the observations announced today represent the culmination of decades of observational, technical, and theoretical work. This example of global teamwork required close collaboration by researchers from around the world. Thirteen partner institutions worked together to create the EHT, using both pre-existing infrastructure and support from a variety of agencies. Key funding was provided by the US National Science Foundation (NSF), the EU's European Research Council (ERC), and funding agencies in East Asia.

“We have achieved something presumed to be impossible just a generation ago," concluded Doeleman. “Breakthroughs in technology, connections between the world's best radio observatories, and innovative algorithms all came together to open an entirely new window on black holes and the event horizon."

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NASA Administrator Statement on Return to Moon in Five Years

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

Vice President Mike Pence speaks about NASA’s
mandate to return American astronauts to the Moon
and on to Mars. Credits: NASA

The following is a statement from NASA Administrator Jim Bridenstine on Tuesday’s announcement by Vice President Mike Pence, at the fifth meeting of the National Space Council, about putting American astronauts back on the Moon in the next five years.

“Today, I joined leaders from across the country as Vice President Mike Pence chaired the fifth meeting of the National Space Council. Vice President Pence lauded President Donald J. Trump’s bold vision for space exploration and spoke to NASA’s progress on key elements to accomplish the President’s Space Policy Directives.

“Among the many topics discussed during our meeting at the U.S. Space and Rocket Center in Huntsville, Alabama, was to accelerate our return to the Moon:

• NASA is charged to get American astronauts to the Moon in the next five years.
• We are tasked with landing on the Moon’s South Pole by 2024.
• Stay on schedule for flying Exploration Mission-1 with Orion on the Space Launch System (SLS) rocket next year, and for sending the first crewed mission to the lunar vicinity by 2022.
• NASA will continue to ‘use all means necessary’ to ensure mission success in moving us forward to the Moon.

“It is the right time for this challenge, and I assured the Vice President that we, the people of NASA, are up to the challenge.

“We will take action in the days and weeks ahead to accomplish these goals. We have laid out a clear plan for NASA’s exploration campaign that cuts across three strategic areas: low-Earth orbit, the Moon, and Mars and deeper into space.

“I have already directed a new alignment within NASA to ensure we effectively support this effort, which includes establishing a new mission directorate to focus on the formulation and execution of exploration development activities. We are calling it the Moon to Mars Mission Directorate.

“Earlier today I was also at Marshall Space Flight Center for an all-hands to reinforce our commitment to SLS with the workforce. We discussed my recent announcement that NASA would consider all options to fly Orion around the Moon on schedule. I shared the analysis we conducted to assess flying the Orion on different commercial options. While some of these alternative vehicles could work, none was capable of achieving our goals to orbit around the Moon for Exploration Mission-1 within our timeline and on budget. The results of this two-week study reaffirmed our commitment to the SLS. More details will be released in the future.

“There’s a lot of excitement about our plans and also a lot of hard work and challenges ahead, but I know the NASA workforce and our partners are up to it. We are now looking at creative approaches to advance SLS manufacturing and testing to ensure Exploration Mission-1 launches in 2020. We will work to ensure we have a safe and reliable launch system that keeps its promise to the American people.

“I know NASA is ready for the challenge of moving forward to the Moon, this time to stay.”

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NASA Selects Mission to Study Space Weather from Space Station

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

An image taken from the International Space Station
shows orange swaths of airglow hovering in Earth’s
atmosphere. NASA’s new Atmospheric Waves
Experiment will observe this airglow from a perch
on the space station to help scientists understand,
and ultimately improve forecasts of, space weather
changes in the upper atmosphere.
Credits: NASA

NASA has selected a new mission that will help scientists understand and, ultimately, forecast the vast space weather system around our planet. Space weather is important because it can have profound impacts – affecting technology and astronauts in space, disrupting radio communications and, at its most severe, overwhelming power grids.

The new experiment will, for the first time, obtain global observations of an important driver of space weather in a dynamic region of Earth’s upper atmosphere that can cause interference with radio and GPS communications.

The Atmospheric Waves Experiment (AWE) mission will cost $42 million and is planned to launch in August 2022, attached to the exterior of the Earth-orbiting International Space Station. From its space station perch, AWE will focus on colorful bands of light in Earth’s atmosphere, called airglow, to determine what combination of forces drive space weather in the upper atmosphere.

Researchers once thought that only the Sun’s constant outflow of ultraviolet light and particles, the solar wind, could affect the region. However, recently they have learned that solar variability is not enough to drive the changes observed, and Earth’s weather also must be having an effect. To help unravel that connection, AWE will investigate how waves in the lower atmosphere, caused by variations in the densities of different packets of air, impact the upper atmosphere.

AWE is a Mission of Opportunity under NASA’s Heliophysics Explorers Program, which conducts focused scientific research and develops instrumentation to fill the scientific gaps between the agency’s larger missions. Since the 1958 launch of NASA’s first satellite Explorer 1, which discovered Earth’s radiation belts, the Explorers Program has supported more than 90 missions. The Uhuru and Cosmic Background Explorer (COBE) missions led to Nobel prizes for their investigators.

“The Explorers Program seeks innovative ideas for small and cost-constrained missions that can help unravel the mysteries of the universe and explore our place in it,” said Paul Hertz, NASA’s Director of Astrophysics. “This mission absolutely meets that standard with a creative and cost-effective mission to solve mysteries about Earth’s upper atmosphere.”

AWE was selected for development based on its potential science value and the feasibility of its development plans. The mission is led by Michael Taylor at Utah State University in Logan and it is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

NASA also has selected the Sun Radio Interferometer Space Experiment (SunRISE) for a seven-month, $100,000 extended formulation study. SunRISE would be an array of six CubeSats operating like one large radio telescope. This proposed mission would investigate how giant space weather storms from the Sun, called solar particle storms, are accelerated and released into planetary space.

While SunRISE has not yet demonstrated its readiness for the next phase of mission development, the proposed concept represents a compelling use of new NASA-developed technology. SunRISE is led by Justin Kasper at the University of Michigan in Ann Arbor and managed by NASA’s Jet Propulsion Laboratory in Pasadena, California.

The Explorers Program, the oldest continuous NASA program, is designed to provide frequent, low-cost access to space using principal investigator-led space science investigations relevant to the work of NASA’s Science Mission Directorate in astrophysics and heliophysics.

The program is managed by Goddard for the Science Mission Directorate, which conducts a wide variety of research and scientific exploration programs for Earth studies, space weather, the solar system and universe.

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NASA's Record-Setting Opportunity Rover Mission on Mars Comes to End

Shantel Harris -
W a s h i n g t o n ,   D C ,   U S A - 

The dramatic image of NASA's Mars Exploration
Rover Opportunity's shadow was taken on sol 180
(July 26, 2004) by the rover's front hazard-avoidance
camera as the rover moved farther into Endurance
Crater in the Meridiani Planum region of Mars.
Credits: NASA/JPL-Caltech

One of the most successful and enduring feats of interplanetary exploration, NASA's Opportunity rover mission is at an end after almost 15 years exploring the surface of Mars and helping lay the groundwork for NASA’s return to the Red Planet.

The Opportunity rover stopped communicating with Earth when a severe Mars-wide dust storm blanketed its location in June 2018. After more than a thousand commands to restore contact, engineers in the Space Flight Operations Facility at NASA's Jet Propulsion Laboratory (JPL) made their last attempt to revive Opportunity Tuesday, to no avail. The solar-powered rover's final communication was received June 10.

“It is because of trailblazing missions such as Opportunity that there will come a day when our brave astronauts walk on the surface of Mars," said NASA Administrator Jim Bridenstine. “And when that day arrives, some portion of that first footprint will be owned by the men and women of Opportunity, and a little rover that defied the odds and did so much in the name of exploration."

Designed to last just 90 Martian days and travel 1,100 yards (1,000 meters), Opportunity vastly surpassed all expectations in its endurance, scientific value and longevity. In addition to exceeding its life expectancy by 60 times, the rover traveled more than 28 miles (45 kilometers) by the time it reached its most appropriate final resting spot on Mars – Perseverance Valley.

“For more than a decade, Opportunity has been an icon in the field of planetary exploration, teaching us about Mars' ancient past as a wet, potentially habitable planet, and revealing uncharted Martian landscapes," said Thomas Zurbuchen, associate administrator for NASA's Science Mission Directorate. “Whatever loss we feel now must be tempered with the knowledge that the legacy of Opportunity continues – both on the surface of Mars with the Curiosity rover and InSight lander – and in the clean rooms of JPL, where the upcoming Mars 2020 rover is taking shape."

The final transmission, sent via the 70-meter Mars Station antenna at NASA's Goldstone Deep Space Complex in California, ended a multifaceted, eight-month recovery strategy in an attempt to compel the rover to communicate.

“We have made every reasonable engineering effort to try to recover Opportunity and have determined that the likelihood of receiving a signal is far too low to continue recovery efforts," said John Callas, manager of the Mars Exploration Rover (MER) project at JPL.

Opportunity landed in the Meridiani Planum region of Mars on Jan. 24, 2004, seven months after its launch from Cape Canaveral Air Force Station in Florida. Its twin rover, Spirit, landed 20 days earlier in the 103-mile-wide (166-kilometer-wide) Gusev Crater on the other side of Mars. Spirit logged almost 5 miles (8 kilometers) before its mission wrapped up in May 2011.

From the day Opportunity landed, a team of mission engineers, rover drivers and scientists on Earth collaborated to overcome challenges and get the rover from one geologic site on Mars to the next. They plotted workable avenues over rugged terrain so that the 384-pound (174-kilogram) Martian explorer could maneuver around and, at times, over rocks and boulders, climb gravel-strewn slopes as steep as 32-degrees (an off-Earth record), probe crater floors, summit hills and traverse possible dry riverbeds. Its final venture brought it to the western limb of Perseverance Valley.

“I cannot think of a more appropriate place for Opportunity to endure on the surface of Mars than one called Perseverance Valley," said Michael Watkins, director of JPL. “The records, discoveries and sheer tenacity of this intrepid little rover is testament to the ingenuity, dedication, and perseverance of the people who built and guided her."

Drive along with the NASA’s Opportunity Mars rover and hear the voices of scientists and engineers behind the mission. Designed to run for 90 days, the exploration spanned more than 15 years from 2004 to 2019. Along the way, it discovered definitive proof of liquid water on ancient Mars and set the off-world driving record.

Credits: NASA/JPL-Caltech

More Opportunity Achievements:

• Set a one-day Mars driving record March 20, 2005, when it traveled 721 feet (220 meters).
• Returned more than 217,000 images, including 15 360-degree color panoramas.
• Exposed the surfaces of 52 rocks to reveal fresh mineral surfaces for analysis and cleared 72 additional targets with a brush to prepare them for inspection with spectrometers and a microscopic imager.
• Found hematite, a mineral that forms in water, at its landing site.
• Discovered strong indications at Endeavour Crater of the action of ancient water similar to the drinkable water of a pond or lake on Earth.

All of the off-roading and on-location scientific analyses were in service of the Mars Exploration Rovers’ primary objective: To seek out historical evidence of the Red Planet's climate and water at sites where conditions may once have been favorable for life. Because liquid water is required for life, as we know it, Opportunity's discoveries implied that conditions at Meridiani Planum may have been habitable for some period of time in Martian history.

“From the get-go, Opportunity delivered on our search for evidence regarding water," said Steve Squyres, principal investigator of the rovers' science payload at Cornell University. “And when you combine the discoveries of Opportunity and Spirit, they showed us that ancient Mars was a very different place from Mars today, which is a cold, dry, desolate world. But if you look to its ancient past, you find compelling evidence for liquid water below the surface and liquid water at the surface."

All those accomplishments were not without the occasional extraterrestrial impediment. In 2005 alone, Opportunity lost steering to one of its front wheels, a stuck heater threatened to severely limit the rover's available power, and a Martian sand ripple almost trapped it for good. Two years later, a two-month dust storm imperiled the rover before relenting. In 2015, Opportunity lost use of its 256-megabyte flash memory and, in 2017, it lost steering to its other front wheel.

Each time the rover faced an obstacle, Opportunity's team on Earth found and implemented a solution that enabled the rover to bounce back. However, the massive dust storm that took shape in the summer of 2018 proved too much for history's most senior Mars explorer.

“When I think of Opportunity, I will recall that place on Mars where our intrepid rover far exceeded everyone's expectations," Callas said. “But what I suppose I'll cherish most is the impact Opportunity had on us here on Earth. It's the accomplished exploration and phenomenal discoveries. It’s the generation of young scientists and engineers who became space explorers with this mission. It's the public that followed along with our every step. And it's the technical legacy of the Mars Exploration Rovers, which is carried aboard Curiosity and the upcoming Mars 2020 mission. Farewell, Opportunity, and well done."

Mars exploration continues unabated. NASA's InSight lander, which touched down on Nov. 26, is just beginning its scientific investigations. The Curiosity rover has been exploring Gale Crater for more than six years. And, NASA's Mars 2020 rover and the European Space Agency’s ExoMars rover both will launch in July 2020, becoming the first rover missions designed to seek signs of past microbial life on the Red Planet.

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