vendredi 3 avril 2020

Smart surfaces for space hygiene













ESA - Proxima Mission patch.

April 3, 2020

Matiss-2 experiment on the Space Station

While efforts continue to contain the spread of the novel coronavirus on Earth, a space-based experiment called Matiss has been investigating how ‘smart surfaces’ on the International Space Station could stop pathogens in their tracks.

The experiment examines the performance of five advanced materials in preventing illness-causing microorganisms from settling and growing in microgravity. Matiss (Microbial Aerosol Tethering on Innovative Surfaces in the international Space Station) is driven by the French space agency (CNES) and was commissioned in 2016 during ESA astronaut Thomas Pesquet’s Proxima mission.

Thomas Pesquet on the International Space Station

Materials sent to the Space Station were selected for their ability to respond to a given stimulus by repelling microorganisms, preventing their growth, or creating their own biofilms to provide a protective shield. They included a mix of advanced technology, from self-assembly monolayers and green polymers, to ceramic polymers and water-repellent hybrid silica.

Understanding the effectiveness and potential use of these materials will be essential to the design of future spacecraft, but could also lead to development and greater use of antimicrobial surfaces on elevator buttons and door handles, in bars, on public transport and in other high-traffic areas.

Reducing the risk

The confined environment of the International Space Station, where air and water are constantly recycled and waste is stored onboard, is the ideal environment for testing such surfaces.

Saturday cleaning day on Space Station

Astronauts already undertake a strict period of quarantine prior to launch and carry out regular, thorough cleaning once on Station to reduce the risk of illness and infection. However, surfaces that respond protectively to airborne bacteria would be easier to clean and more hygienic.

Evolution of an experiment

The first set of the Matiss experiment, known as Matiss-1, provided some baseline data points for researchers. Four sample holders – each containing the five materials to be tested plus a glass control surface – were set up in three different locations within the European Columbus laboratory, where they remained for six months. 

Once these samples were returned to Earth, researchers characterised the deposits formed on each surface and used the control material to establish a reference for the level and type of contamination expected over half a year.

Clean house

A continuation of the experiment, known as Matiss-2, saw four identical sample holders containing three different types of material installed in a single location in Columbus. This study aimed to better understand how contamination spreads across the hydrophobic and control surfaces.

Sample holders from Matiss-2 were returned to Earth on a SpaceX Dragon spacecraft in August 2019. At that time, NASA astronaut Andrew Morgan also installed a further set of two sample holders in Columbus, which aim to test new patterned hydrophobic (liquid-repelling) surfaces.

Related links:

Proxima: https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/Proxima

Human and Robotic Exploration: http://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration

Science & Exploration: http://www.esa.int/Science_Exploration

International Space Station (ISS): http://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/International_Space_Station

European Space Agency (ESA): http://www.esa.int/

Images, Video, Text, Credits: ESA/NASA/CNES/Emmanuel Grimault, 2016.

Best regards, Orbiter.ch

Choosing rocks on Mars to bring to Earth













NASA - Perseverance Mars Rover logo.

April 3, 2020

If you could bring something back from Mars to Earth, what would you choose? This question is becoming reality, as ESA opens a call for scientists to join a NASA team working to determine which martian samples should be collected and stored by the Perseverance rover set to launch this Summer.

Mars landscape

Perseverance is a standalone mission seeking signs of habitable conditions on our neighbour planet, but it is also part of the international Mars Sample Return campaign that ESA Member States agreed to finance last year during Space19+.

Perseverance rover

Traveling over 53 million km to Mars, landing, collecting samples and launching a vehicle to return to Earth is unprecedented. This campaign will span a decade and involve four launches, including three from Earth and the first launch from another planet.

Mars Sample Return overview infographic

Interplanetary geo-caching
 
Sample Fetch Rover for Mars Sample Return campaign

When Perseverance lands on Mars it will scout the area for over a year. One of its main tasks will be to collect samples in cigar-sized metal cylinders that it will leave on the surface for pickup at a later date.  As part of this international collaboration, ESA plans to provide a sophisticated Sample Fetch Rover to be operated during NASA’s Sample Retrieval Lander mission in the middle of this decade.

Earth Return Orbiter catching Mars sample capsule

The ESA rover will collect the samples that the Perseverance rover gathered and bring them to the lander, where they will be carefully stored in a Mars Ascent Vehicle (MAV). The MAV will launch the sample container from the martian surface, placing it in orbit around Mars.

Earth Return Orbiter leaving Mars orbit

Another important ESA contribution will be the biggest and most robust spacecraft flying to Mars – the Earth Return Orbiter that will rendezvous with the sample and bring it to Earth.

Packing for a return to Earth
 
Earth Return Orbiter releasing Mars sample capsule

Although the full campaign is in its early project phase, scientific experts must be selected now so they can begin training and operate alongside the Perseverance science team to enhance the value of the samples that will be collected. The selected scientists will also have to anticipate the needs of future investigators who may analyse these samples for a very diverse range of studies on Earth.

Martian soil

“We encourage applications from experts outside of the space field,” says ESA’s interim Mars Sample Return Programme Scientist Dr. Gerhard Kminek. “We need field geologists and laboratory experts who know how to pick the right samples based on information from the instruments that Perseverance has on-board.”

Mars Sample Return Earth Return Orbiter elements

ESA’s human spaceflight team leader adds, “experts selected through this call will receive training to form part of the international team of martian-geologists-at-a-distance. These are exciting times and we are looking forward to receiving the best proposals Europe has to offer.”

Uncovering the secrets of our Solar System

Studying Mars samples on Earth will allow scientists to use instruments more powerful than anything that could be flown on robotic missions.  The chance to learn and share resources, including sending samples to the best laboratories around the world, offers incredible opportunities for new discoveries.

Mars Express view of Terra Sabaea and Arabia Terra

Samples may be analysed again and again, enabling new information to be extracted – much like with lunar samples brought to Earth in the 1960s and 1970s, which continue to reveal new discoveries to this day.

Gerhard concludes, “There are many reasons to study Mars, but one of the most pressing is that, while life arose and evolved on Earth, we still don’t know if life had a chance on Mars. Planetary scientists can study rocks, sediments and soils for clues to uncover the geological and potential biological history of Mars. Then, by comparing those findings with Earth we also learn more about our own planet.”

Apply for this opportunity to contribute to ground-breaking science through ESA’s Announcement of Opportunity page for Human and Robotic Exploration research: https://www.esa.int/spaceflightAO

Related links:

Perseverance: https://mars.nasa.gov/mars2020/

Mars Sample Return campaign: https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/Exploration/Mars_sample_return

Mars Express: http://www.esa.int/ESA_Multimedia/Missions/Mars_Express

Human and Robotic Exploration: http://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration

Images, Videos, Text, Credits: ESA/NASA/JPL-Caltech/ATG medialab.

Greetings, Orbiter.ch

jeudi 2 avril 2020

NASA Outlines Lunar Surface Sustainability Concept











NASA - Artemis Program logo.

April 2, 2020

When NASA sends astronauts to the surface of the Moon in 2024, it will be the first time outside of watching historical footage most people witness humans walking on another planetary body. Building on these footsteps, future robotic and human explorers will put in place infrastructure for a long-term sustainable presence on the Moon.


Image above: Infographic showing the evolution of lunar activities on the surface and in orbit. Image Credit: NASA. 

NASA recently proposed a plan to go from limited, short-term Apollo-era exploration of the 1960s, to a 21st Century plan in a report to the National Space Council. With the Artemis program, we will explore more of the Moon than ever before to make the next giant leap – sending astronauts to Mars.

“After 20 years of continuously living in low-Earth orbit, we’re now ready for the next great challenge of space exploration – the development of a sustained presence on and around the Moon,” said NASA Administrator Jim Bridenstine. “For years to come, Artemis will serve as our North Star as we continue to work toward even greater exploration of the Moon, where we will demonstrate key elements needed for the first human mission to Mars.”

On the surface, the core elements for a sustained presence would include an emphasis on mobility to allow astronauts to explore more of the Moon and conduct more science:

- A lunar terrain vehicle or LTV, would transport crew around the landing zone


Image above: Concept image showing the view of a crew Lunar Terrain Vehicle. Image Credit: NASA.

- The habitable mobility platform would enable crews to take trips across the Moon lasting up to 45 days

- A lunar foundation surface habitat would house as many as four crew members on shorter surface stays

Astronauts working on the lunar surface also could test advanced robotics, as well as a wide set of new technologies identified in the Lunar Surface Innovation Initiative, focusing on tech development in the areas such as of in-situ resource utilization (ISRU) and power systems. Rovers will carry a variety of instruments including ISRU experiments that will generate information on the availability and extraction of usable resources (e.g., oxygen and water). Advancing these technologies could enable the production of fuel, water, and/or oxygen from local materials, enabling sustainable surface operations with decreasing supply needs from Earth.

Another key difference from Apollo and Artemis will be use of the Gateway in lunar orbit, built with commercial and international partners. The lunar outpost will serve as a command and control module for surface expeditions and an office and home for astronauts away from Earth. Operating autonomously when crew is not present, it also will be a platform for new science and technology demonstrations around the Moon.

Over time, NASA and its partners will enhance the lunar Gateway’s habitation capabilities and related life support systems. Adding a large-volume deep space habitation element would allow astronauts to test capabilities around the Moon for long-duration deep space missions.

While the goal of Apollo was to land the first humans on the Moon, the Artemis program will use the Moon as a testbed for crewed exploration farther into the solar system, beginning with Mars. This is America’s Moon to Mars space exploration approach. A proposed multi-month split-crew operation at the Gateway and on the lunar surface would test the agency’s concept for a human mission to the Red Planet.

For such a mission, NASA envisions a four-person crew traveling to the Gateway and living aboard the outpost for a multi-month stay to simulate the outbound trip to Mars. Later, two crew members would travel to the lunar surface and explore with the habitable mobility platform, while the remaining two astronauts stay aboard Gateway. The four crew members are later reunited aboard the lunar outpost for another multi-month stay, simulating the return trip to Earth. This mission would be the longest duration human deep space mission in history and would be the first operational test of the readiness of our deep-space systems.

The report also highlights a robotic return to the surface beginning next year for scientific discovery. The Moon is a natural laboratory to study planetary processes and evolution, and a platform from which to observe the universe. NASA will send dozens of new science instruments and technology demonstrations to the Moon with its Commercial Lunar Payload Services initiative. Some of these robotic precursors, including the Volatiles Investigating Polar Exploration Rover or VIPER, will study the terrain, and metal and ice resources at the lunar South Pole.


Image above: An artist's concept of NASA’s Volatiles Investigating Polar Exploration Rover, or VIPER. VIPER is a mobile robot that will roam around the Moon’s south pole looking for water ice. The VIPER mission will give us surface-level detail of where the water is and how much is available for us to use. This will bring us a significant step closer towards NASA’s ultimate goal of a sustainable, long-term presence on the Moon – making it possible to eventually explore Mars and beyond. Image Credits: NASA Ames/Daniel Rutter.

The Space Launch System rocket, Orion spacecraft, human landing systems and modern spacesuits will round out the agency’s deep space systems. As part of the Artemis III mission, the first human expedition back on the Moon will last approximately seven days. NASA plans to send Artemis Generation astronauts on increasingly longer missions about once per year thereafter.

With strong support in NASA, America and its partners will test new technologies and reduce exploration costs over time. Supporting infrastructure including power, radiation shielding, a landing pad, as well as waste disposal and storage could be built up in the coming decades, too.

“The U.S. is still the only nation to have successfully landed humans on the Moon and spacecraft on the surface of Mars,” the report states. “As other nations increasingly move out into space, American leadership is now called for to lead the next phase of humanity’s quest to open up the future to endless discovery and growth.”

Read the full report (PDF):

NASA's Plan for Sustained Lunar Exploration and Development
https://www.nasa.gov/sites/default/files/atoms/files/a_sustained_lunar_presence_nspc_report4220final.pdf

Related links:

Lunar terrain vehicle (LTV): https://www.nasa.gov/feature/nasa-to-industry-send-ideas-for-lunar-rovers

Lunar Surface Innovation Initiative: https://www.nasa.gov/directorates/spacetech/Lunar_Surface_Innovation_Initiative

Gateway: https://www.nasa.gov/topics/moon-to-mars/lunar-gateway

Moon to Mars: http://www.nasa.gov/moontomars

Commercial Lunar Payload Services: http://www.nasa.gov/clps

VIPER: http://www.nasa.gov/viper

Artemis: https://www.nasa.gov/artemisprogram

Images (mentioned), Text, Credits: NASA/Cheryl Warner.

Best regards, Orbiter.ch

Science Expands on Station, Dragon Departs on Monday













ISS - Expedition 62 Mission patch.

April 2, 2020

International Space Station (ISS). Animation Credit: NASA

The International Space Station expanded its research capabilities overnight after robotics controllers installed a new external science platform. Meanwhile, the Expedition 62 crew is packing cargo for return to Earth while getting ready for its own departure.

Europe’s latest contribution to the orbiting lab, Bartolomeo, was attached to the outside of the Columbus laboratory module early Thursday morning. Robotic engineers remotely commanded the Canadarm2 robotic arm and the Dextre robotic hand and completed the fine-tuned installation work over two days. Bartolomeo, delivered last month aboard the SpaceX Dragon cargo craft, gives private and institutional researchers the ability to command and control science payloads outside the space station.


Image above: NASA astronaut Jessica Meir strikes a superhero pose in the weightless environment of the International Space Station. Image Credit: NASA.

Commander Oleg Skripochka with NASA Flight Engineers Jessica Meir and Andrew Morgan are preparing to end their mission in space on April 17. They checked their Sokol launch and entry suits they will wear when they parachute to Earth inside the Soyuz MS-15 crew ship for leaks today. The crew is also gathering personal items for stowage inside the Soyuz spaceship.

Before they leave, the SpaceX Dragon space freighter will return to Earth after being released from the Canadarm2 on Monday at 9:52 a.m. EDT. Meir and Morgan will finish loading over 4,000 pounds of station hardware and research samples, including live mice and plant cells, late Sunday. NASA TV will begin its live coverage of Dragon’s departure on Monday at 9:30 a.m.


Image above: SpaceX's Dragon resupply ship slowly approaches the orbiting lab as both spacecraft were orbiting 258 miles above the Mediterranean Sea Dec. 9, 2019. Filled with more than 4,000 pounds of valuable scientific experiments and other cargo, Dragon is now set to leave the International Space Station Monday, April 6. Image Credit: NASA.

The station boosted its orbit again today raising it to the correct altitude enabling the new Expedition 63 crew to launch and dock on April 9 inside the Soyuz MS-16 crew ship. NASA astronaut Chris Cassidy and Roscosmos cosmonauts Anatoly Ivanishin and Ivan Vagner will take a six-hour ride to their new home in space and begin a 195-day mission aboard the orbital lab.

Related links:

Expedition 62: https://www.nasa.gov/mission_pages/station/expeditions/expedition62/index.html

Expedition 63: https://www.nasa.gov/mission_pages/station/expeditions/expedition63/index.html

Bartolomeo: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=7799

Columbus laboratory module: https://www.nasa.gov/mission_pages/station/structure/elements/europe-columbus-laboratory

Canadarm2: https://www.nasa.gov/mission_pages/station/structure/elements/mobile-servicing-system.html

Dextre: https://www.nasa.gov/mission_pages/station/structure/elements/special-purpose-dextrous-manipulator

Live mice: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8150

Plant cells: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8223

NASA TV live coverage: https://www.nasa.gov/press-release/nasa-tv-to-air-us-cargo-ship-departure-from-space-station-1

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Images (mentioned), Animation (mentioned), Text, Credits: NASA/Mark Garcia.

Best regards, Orbiter.ch

New NASA Radar Looks to Monitor Volcanoes and Earthquakes from Space











NASA - ISRO SAR Mission logo.

April 2, 2020

Instead of looking up to the sky for bright bursts of fiery color, a research team spent Fourth of July 2018 peering down at fiery globs of molten lava from a sky-diving airplane. Bolted to their plane was a new NASA instrument designed to detect each time the volcano took a breath, as its caldera swelled and deflated.

The team flew multiple flights above the Kīlauea Volcano in Hawaii Volcanoes National Park from July 3 to 5, 2018, to demonstrate how a new instrument could pave the way for a future constellation of small satellites dedicated to monitoring impacts from volcanic activity, earthquakes and changes in land surfaces, said Lauren Wye, the principal investigator who led and recently concluded the instrument’s development at SRI International in Menlo Park, California.

A global map detailing land elevation changes over time can help scientists pinpoint ground motion before, during and following earthquakes and volcanic eruptions, and help identify impacts from floods and groundwater pumping. “The CubeSat Imaging Radar for Earth Sciences, or CIRES, can help decision-makers and emergency managers obtain observations sooner after a hazardous event so that they are better prepared to deal with disaster relief,” Wye said.


Image above: The ash plume from the Kilauea volcano on the big island of Hawaii was pictured May 12, 2018, from the International Space Station. Image Credit: NASA.

Although Kīlauea’s eruption impacted over 50 square miles of land, ground deformation, or a change in land elevation, is not always perceptible to the human eye. Highly specialized technology like Wye’s new instrument can pinpoint and record these changes.

CIRES is equipped with an S-band Interferometric Synthetic Aperture Radar (InSAR). The S-band radar is able to penetrate through vegetation and reach the ground. CIRES takes two radar images of a specific area from approximately the same position in space at two different times and then processes the two images to determine the difference between them.

The National Academies of Sciences, Engineering and Medicine’s 2017 Decadal Survey, “Thriving on Our Changing Planet: A Decadal Strategy for Earth Observations from Space,” recommends that NASA use InSAR measurements to help address the dynamics of earthquakes, volcanoes, landslides, glaciers, groundwater and Earth’s interior.

A constellation of small InSAR satellites could work in tandem with the NASA-ISRO SAR Mission (NISAR), which is NASA’s first dedicated InSAR satellite currently in development. Multiple small satellites could collect frequent data over rapidly evolving processes, like volcanic eruptions, earthquakes and landslides, adding to NISAR’s systematic global data.

Once upon a radar

Traditionally, researchers monitor ground deformation with on-the-ground sensors and the Global Positioning System (GPS). InSAR measurements are complementary to ground measurements and can often guide how ground sensors are installed. “InSAR data have revolutionized how we look at earthquakes and volcanoes,” Kyle Anderson, a geophysicist at the U.S. Geological Survey, said.

In orbit, a series of small InSAR satellites could peer down and record changes in ground deformation. “Volcanoes will often inflate with magma before they erupt,” Anderson said. Anderson worked with the CIRES team at Kīlauea. “Although it’s difficult to predict how big or how long the eruption will be, we can say, this volcano started inflating and there’s a higher probability of it erupting.”

The CIRES project began in January 2015 at SRI International with funding from NASA’s Earth Science Technology Office to develop the instrument’s radar electronics hardware over two years. It then received an additional three years of funding to prepare the radar for space, demonstrate the imaging capabilities via aircraft, including both on-board and remotely piloted aircraft, and advance a space-deployable antenna to complete the instrument.

“InSAR has been particularly useful for better understanding volcanoes in remote areas,” Anderson said. For example, the technology helped scientists notice deformation near the Three Sisters cluster of volcanoes in central Oregon from 1997 to 2001. InSAR pinpointed deformation in an area that last saw an eruption 1,500 years ago. Because of the observed changes, the USGS installed seismometers, GPS stations and gas-monitoring equipment to check for other signs of activity. In 2004, those instruments detected a swarm of 300 small earthquakes.


Image above: Three Sisters Volcano in Central Oregon. Image Credit: USGS.

“InSAR allows you to get wide areas of coverage and see how one part of the volcano’s caldera is changing relative to another part,” Patrick Rennich, the CIRES signal processing and experiment design lead, said. Typically, researchers place a limited number of GPS sensors on specific parts of the volcano to monitor any movement. “CIRES should be able to cover the entire caldera,” Rennich said.

Steps to space

During development, “the team ran into a lot of hiccups,” Wye said. However, with each hiccup, like a delayed test flight, the team got innovative. “It led to a lot of fun exercises,” Wye said.

One of those exercises saw the team strapping the instrument to a moving car. They drove the car, which they dubbed “CarSAR,” along elevated roads in the Bay Area of Northern California in early 2018 to see how CIRES would pick up information in a valley below. “But we really needed to get higher to test our data,” Wye said.

When the Kīlauea Volcano started erupting in May 2018, they saw their opportunity. On July 4, 2018, lava was flowing and the volcano’s caldera was collapsing. CIRES successfully obtained SAR, or snapshot imagery, but wasn’t able to obtain InSAR, or comparison images, over Kīlauea, in part because, “It was difficult to fly on the exact same path every day,” Rennich said.

The flights over Kīlauea, among other field tests, helped the team learn what worked and didn’t work as they developed the instrument. They were able to optimize CIRES to improve its power management, size, sensor capabilities and ability to withstand heat.

In December 2019, the team again strapped CIRES, with updated hardware and software, to an airplane usually reserved for commercial skydiving and flew 10,000 feet above an army training facility in Indiana. “It turns out that skydiving operators are very comfortable flying with an open door,” Rennich said.

The team flew CIRES above a simulated flooded village at the Muscatatuck Urban Training Center to better understand radar signatures in a flooded urban environment. The flight also produced data that could improve algorithms that quantify the extent of flooding and related damage. NASA’s Earth Science Technology Office and Disasters Program helped fund the flights and analysis of the CIRES data.


Image above: The CubeSat Imaging Radar for Earth Sciences (CIRES) is loaded on an aircraft before validation tests in Indiana in December 2019. Image Credit: Michael Huff.

“By mounting CIRES on an airplane, we could fly at different angles and see how different building orientations affect how they appear in radar images due to flooding,” Sang-Ho Yun, a geophysicist and coinvestigator of this project at NASA’s Jet Propulsion Laboratory in Pasadena, California, said. “Flooding is like a ghost,” Yun said; its ephemeral nature makes it difficult to assess the accuracy of flood mapping techniques.

The team also performed an experiment where they controlled motion on the ground to test CIRES. During the Indiana flight, “One of our colleagues on the ground would raise silvery metal reflectors by half a centimeter to a centimeter to show that we can detect that level of change,” Rennich said. This helped prove that CIRES collected accurate InSAR data.

The flights were successful in part because the team was able to fly CIRES along the same path multiple times in a row, which they weren’t able to do in Hawaii. “We implemented a better pilot navigation system,” Rennich said, which allowed the team to fly within a few feet of where they had flown the previous day. In Hawaii, the they flew approximately 500 feet from the previous day’s course.

“When you’re in space, trajectory is much more repeatable,” Rennich said, because each satellite is on a predictable, traceable course.

For the team to make CIRES, or a CIRES-like instrument work in space, they would need to significantly extend its antenna, from two feet across to 10 feet across, Rennich said. “Everything else pretty much stays the same,” he said.

“Small satellites, similar in scope to CIRES, can be a dream system from a rapid disaster response point of view,” Yun said. Although small satellites, like CIRES, won’t be able to obtain the same accuracy as larger systems, they could obtain data more frequently when a disaster hits. “With small satellites, we can cost effectively achieve that goal,” Yun said.

For more information about NASA’s Earth Science Technology Office (ESTO), visit: https://slack-redir.net/link?url=http%3A%2F%2Festo.nasa.gov

NISAR (NASA-ISRO Synthetic Aperture Radar): https://www.nasa.gov/subject/6533/nisar

Images (mentioned), Text, Credits: NASA/Sara Blumberg/Earth Science Technology Office/Elizabeth Goldbaum.

Best regards, Orbiter.ch

Rosette Nebula Gives Birth to Stars











ESA & NASA - Herschel Mission patch.

April 2, 2020


This 2010 image from the Herschel Space Observatory shows dust clouds associated with the Rosette Nebula, a stellar nursery about 5,000 light-years from Earth in the Monoceros, or Unicorn, constellation. Herschel collected the infrared light given out by dust. The bright smudges are dusty cocoons containing massive embryonic stars, which will grow up to 10 times the mass of our Sun. The small spots near the center of the image are lower mass stellar embryos. The nebula itself is located to the right of the picture, along with its massive cluster of stars.

 Herschel Space Observatory

Editor note:

The Herschel space observatory operated between 2009 and 2013.

Related links:

NASA's Herschel Space Observatory: https://www.nasa.gov/mission_pages/herschel/index.html

ESA's Herschel Space Observatory: https://www.esa.int/Science_Exploration/Space_Science/Herschel

Images, Text, Credits: ESA and the PACS, SPIRE & HSC consortia, F. Motte (AIM Saclay,CEA/IRFU - CNRS/INSU - U.ParisDidedrot) for the HOBYS key programme/NASA/Yvette Smith.

Greetings, Orbiter.ch

WFIRST Will Use Warped Space-time to Help Find Exoplanets












NASA - Wide Field Infrared Survey Telescope (WFIRST) patch.

April 2, 2020

The NASA mission will identify planets with large orbits, similar to our solar system's far-flung giants, Uranus and Neptune.


Image above: WFIRST will make its microlensing observations in the direction of the center of the Milky Way galaxy. The higher density of stars will yield more exoplanet detections. Image Credits: NASA's Goddard Space Flight Center/CI Lab.

NASA's Wide Field Infrared Survey Telescope (WFIRST) will search for planets outside our solar system toward the center of our Milky Way galaxy, where most stars are. Studying the properties of exoplanet worlds will help us understand what planetary systems throughout the galaxy are like and how planets form and evolve.

Combining WFIRST's findings with results from NASA's Kepler and Transiting Exoplanet Survey Satellite (TESS) missions will complete the first planet census that is sensitive to a wide range of planet masses and orbits, bringing us a step closer to discovering habitable Earth-like worlds beyond our own.

To date, astronomers have found most planets when they pass in front of their host star in events called transits, which temporarily dim the star's light. WFIRST data can spot transits, too, but the mission will primarily watch for the opposite effect - little surges of radiance produced by a light-bending phenomenon called microlensing. These events are much less common than transits because they rely on the chance alignment of two widely separated and unrelated stars drifting through space.

"Microlensing signals from small planets are rare and brief, but they're stronger than the signals from other methods," said David Bennett, who leads the gravitational microlensing group at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "Since it's a one-in-a-million event, the key to WFIRST finding low-mass planets is to search hundreds of millions of stars."

In addition, microlensing is better at finding planets in and beyond the habitable zone - the orbital distances where planets might have liquid water on their surfaces.

Microlensing 101

This effect occurs when light passes near a massive object. Anything with mass warps the fabric of space-time, sort of like the dent a bowling ball makes when set on a trampoline. Light travels in a straight line, but if space-time is bent - which happens near something massive, like a star - light follows the curve.

Any time two stars align closely from our vantage point, light from the more distant star curves as it travels through the warped space-time of the nearer star. This phenomenon, one of the predictions of Einstein's general theory of relativity, was famously confirmed by British physicist Sir Arthur Eddington during a total solar eclipse in 1919. If the alignment is especially close, the nearer star acts like a natural cosmic lens, focusing and intensifying light from the background star.

Planets orbiting the foreground star may also modify the lensed light, acting as their own tiny lenses. The distortion they create allows astronomers to measure the planet's mass and distance from its host star. This is how WFIRST will use microlensing to discover new worlds.

Familiar and Exotic Worlds

"Trying to interpret planet populations today is like trying to interpret a picture with half of it covered," said Matthew Penny, an assistant professor of physics and astronomy at Louisiana State University in Baton Rouge who led a study to predict WFIRST's microlensing survey capabilities. "To fully understand how planetary systems form we need to find planets of all masses at all distances. No one technique can do this, but WFIRST's microlensing survey, combined with the results from Kepler and TESS, will reveal far more of the picture."

More than 4,000 confirmed exoplanets have been discovered so far, but only 86 were found via microlensing. The techniques commonly used to find other worlds are biased toward planets that tend to be very different from those in our solar system. The transit method, for example, is best at finding sub-Neptune-like planets that have orbits much smaller than Mercury's. For a solar system like our own, transit studies could miss every planet.

Wide Field Infrared Survey Telescope or WFIRST. Animation Credit: NASA

WFIRST's microlensing survey will help us find analogs to every planet in our solar system except Mercury, whose small orbit and low mass combine to put it beyond the mission's reach. WFIRST will find planets that are the mass of Earth and even smaller - perhaps even large moons, like Jupiter's moon Ganymede.

WFIRST will find planets in other poorly studied categories, too. Microlensing is best suited to finding worlds from the habitable zone of their star and farther out. This includes ice giants, like Uranus and Neptune in our solar system, and even rogue planets - worlds freely roaming the galaxy unbound to any stars.

While ice giants are a minority in our solar system, a 2016 study indicated that they may be the most common kind of planet throughout the galaxy. WFIRST will put that theory to the test and help us get a better understanding of which planetary characteristics are most prevalent.

Hidden Gems in the Galactic Core

WFIRST will explore regions of the galaxy that haven't yet been systematically scoured for exoplanets due to the different goals of previous missions. Kepler, for example, searched a modest-sized region of about 100 square degrees with 100,000 stars at typical distances of around a thousand light-years. TESS scans the entire sky and tracks 200,000 stars; however their typical distances are around 100 light-years. WFIRST will search roughly 3 square degrees, but will follow 200 million stars at distances of around 10,000 light-years.

Since WFIRST is an infrared telescope, it will see right through the clouds of dust that block other telescopes from studying planets in the crowded central region of our galaxy. Most ground-based microlensing observations to date have been in visible light, making the center of the galaxy largely uncharted exoplanet territory. A microlensing survey conducted since 2015 using the United Kingdom Infrared Telescope (UKIRT) in Hawaii is smoothing the way for WFIRST's exoplanet census by mapping the region.

The UKIRT survey is providing the first measurements of the rate of microlensing events toward the galaxy's core, where stars are most densely concentrated. The results will help astronomers select the final observing strategy for WFIRST's microlensing effort.

WFIRST telescope operation description. Animation Credit: NASA

The UKIRT team's most recent goal is detecting microlensing events using machine learning, which will be vital for WFIRST. The mission will produce such a vast amount of data that combing through it solely by eye will be impractical. Streamlining the search will require automated processes.

Additional UKIRT results point to an observing strategy that will reveal the most microlensing events possible while avoiding the thickest dust clouds that can block even infrared light.

"Our current survey with UKIRT is laying the groundwork so that WFIRST can implement the first space-based dedicated microlensing survey," said Savannah Jacklin, an astronomer at Vanderbilt University in Nashville, Tennessee, who has led several UKIRT studies. "Previous exoplanet missions expanded our knowledge of planetary systems, and WFIRST will move us a giant step closer to truly understanding how planets - particularly those within the habitable zones of their host stars - form and evolve."

From Brown Dwarfs to Black Holes

The same microlensing survey that will reveal thousands of planets will also detect hundreds of other bizarre and interesting cosmic objects. Scientists will be able to study free-floating bodies with masses ranging from that of Mars to 100 times the Sun's.

The low end of the mass range includes planets that were ejected from their host stars and now roam the galaxy as rogue planets. Next are brown dwarfs, which are too massive to be characterized as planets but not quite massive enough to ignite as stars. Brown dwarfs don't shine visibly like stars, but WFIRST will be able to study them in infrared light through the heat left over from their formation.

Objects at the higher end include stellar corpses - neutron stars and black holes - left behind when massive stars exhaust their fuel. Studying them and measuring their masses will help scientists understand more about stars' death throes while providing a census of stellar-mass black holes.

"WFIRST's microlensing survey will not only advance our understanding of planetary systems," said Penny, "it will also enable a whole host of other studies of the variability of 200 million stars, the structure and formation of the inner Milky Way, and the population of black holes and other dark, compact objects that are hard or impossible to study in any other way."

The FY2020 Consolidated Appropriations Act funds the WFIRST program through September 2020. The FY2021 budget request proposes to terminate funding for the WFIRST mission and focus on the completion of the James Webb Space Telescope, now planned for launch in March 2021. The Administration is not ready to proceed with another multi-billion-dollar telescope until Webb has been successfully launched and deployed.

WFIRST is managed at Goddard, with participation by NASA's Jet Propulsion Laboratory and Caltech/IPAC in Pasadena, the Space Telescope Science Institute in Baltimore, and a science team comprising scientists from research institutions across the United States.

Related links:

2016 study: https://www.nasa.gov/feature/goddard/2016/most-common-outer-planets-likely-neptune-mass

United Kingdom Infrared Telescope (UKIRT): http://www.ukirt.hawaii.edu/

Microlensing survey: https://exoplanetarchive.ipac.caltech.edu/docs/UKIRTMission.html

For more information about WFIRST, visit:

https://www.nasa.gov/content/goddard/wfirst-wide-field-infrared-survey-telescope

Image (mentioned), Animations (mentioned), Text, Credits: NASA/JPL/Calla Cofield/Goddard Space Flight Center/Claire Andreoli/Written by Ashley Balzer.

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