mardi 10 septembre 2019

JAXA - H-IIB F8/HTV-8 launch-pad in fire













JAXA - H-IIB Launch Vehicle No. 8 (H-IIB F8) Mission patch.

Sept. 10, 2019

H-IIB F8/HTV-8 launch-pad in fire

A Japanese H-2B rocket will launch the eighth H-2 Transfer Vehicle. The HTV serves as an automated cargo vehicle to deliver equipment and supplies to the International Space Station.

H-IIB F8/HTV-8 launchpad fire

JAXA’s H-IIB Launch Vehicle No. 8 (H-IIB F8) launch with the H-II Transfer Vehicle “KOUNOTORI8” (HTV-8) from the Yoshinobu Launch Complex, at JAXA’s Tanegashima Space Center, was canceled on 10 September 2019 due to a fire on the launchpad. The fire was extinguished, the causes are under investigation.

Related articles:


JAXA Spacecraft Carries Science, Technology to the Space Station
https://orbiterchspacenews.blogspot.com/2019/09/jaxa-spacecraft-carries-science.html

JAXA and Sony CSL to Conduct In-Orbit Demonstrations of Long-Distance Laser Communication
https://orbiterchspacenews.blogspot.com/2019/08/jaxa-and-sony-csl-to-conduct-in-orbit.html

Related links:

H-II Transfer Vehicle-8 (HTV-8): https://www.nasa.gov/mission_pages/station/structure/elements/htv.html

Japan Aerospace Exploration Agency (JAXA): https://global.jaxa.jp/

Image, Video, Text, Credits: JAXA/NECOVIDEO VISUAL SOLUTIONS/SciNews/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch

Studying flames in microgravity is helping make combustion on Earth cleaner, and space safer













ISS - International Space Station logo.

Sept. 10, 2019

Understanding how fire spreads and behaves in space is crucial for the safety of future astronauts and for understanding and controlling fire here on Earth.

Microgravity is also crucial for combustion researchers to test some of the core principles of the field. “If you look at any textbook on combustion, almost all of the theories that are developed ignore the influence of gravity,” says NASA’s Glenn Research Center scientist Daniel Dietrich.


Image above: This flame was one of many ignited as part of the Flame Design investigation inside of CIR to investigate the amount of soot that is produced in different conditions. The yellow spots are soot clusters that glow yellow when hot. These clusters grow larger in microgravity than on Earth because the soot remains within the flame longer. Image Credit: NASA.

The primary focus of microgravity combustion experiments has been related to either fire safety in space or better understanding of practical combustion on Earth and in space. The reduced gravity creates flames that look a lot different from the ones seen here on Earth: with the near absence of gravity on the space station, flames tend to be spherical. On Earth, hot gasses from the flame rise while gravity pulls cooler, denser air to the bottom of the flame. This creates both the shape of the flame, as well as a flickering effect. In microgravity, this flow doesn’t occur. This reduces the variables in combustion experiments, making them simpler and creating spherical shaped flames.

Learning to make cleaner or more efficient flames can have an impact on many areas of our lives. “Most of our electricity in the U.S. is generated by combustion,” says Glenn project scientist Dennis Stocker. “In regards to power transportation, where would we be without combustion? So combustion is a big part of our modern lives.”


Image above: NASA astronaut and Expedition 59 Flight Engineer Christina Koch works inside the U.S. Destiny laboratory module's Combustion Integrated Rack. She was replacing hardware for a series of experiments collectively known as Advanced Combustion via Microgravity Experiments (ACME). Image Credit: NASA.

As with other space station research, experiments with combustion are developed to be safely conducted without risk to the spacecraft or its crew. That is why the Combustion Integrated Rack (CIR) was created and launched to the International Space Station in 2008. The CIR, along with facilities such as the Microgravity Science Glovebox, created a secure and safe environment in which to study combustion without putting the crew in danger. The CIR provides general-purpose hardware to support a wide range of combustion experiments. Researchers also have provided additional hardware needed to conduct a variety of flame experiments.

“One of the biggest discoveries, not only in the microgravity program, but in probably the past 20 – 30 years of combustion research has been during the FLEX experiments on the space station,” says Dietrich. The FLame Extinguishment Experiment (FLEX) was analyzing the effectiveness of fire suppressants by studying burning fuel droplets in the CIR, when researchers accidentally made a surprising discovery related to cool flames, or apparent continued "burning" after flame extinction under certain conditions.

“It's not only important from a nerdy theoretical combustion point of view, but also from a practical point of view,” says Dietrich. “The low temperature chemical reactions that we can study on facilities like the space station are very important in real combustion systems like engines.”

However, the CIR is not the only way to perform combustion experiments using the space station. A set of notable exceptions are the Saffire experiments that occurred aboard an uncrewed Cygnus spacecraft after they detached from the station. Since these experiments occurred away from the space station, they could study topics such as fire spread and oxygen use in larger flames in microgravity.


Image above: Astronaut Michael Fincke, Expedition 18 commander, works on the Multi-User Droplet Combustion Apparatus (MDCA) Chamber Insert Assembly (CIA) in the Harmony node of the International Space Station. Image Credit: NASA.

Currently scientists are conducting a set of experiments known as the Advanced Combustion via Microgravity Experiments (ACME) on the orbiting laboratory. These tests are grouped together because they use the same modular set of hardware on the station. Together they will yield data that could help improve fuel efficiency and reduce pollutant production in practical combustion on Earth.

One of these ACME investigations, known as Flame Design, focuses on soot, the carbon residue left behind when organic matter (or other carbon-containing material) does not fully burn. Soot causes environmental and health issues, but also can be helpful in various ways; for example, by enhancing radiant heat. Radiant heat is the reason you feel warmer standing in direct sunlight than when you stand in the shade.

Normally, most flames on Earth burn in air. Inert gas is introduced at the same time as oxygen for combustion on Earth. This investigation instead introduces the inert gas with the fuel, rather than with the oxygen. “It turns out, it has a big impact on the flame,” says principal investigator Richard Axelbaum. “In this case, even though the temperatures of the flames may be the same whether you introduce the inert with the oxidizer or the fuel, the impact for soot formation or flame strength is substantially different.”

The Flame Design investigation is studying the quantity of soot produced under different flame conditions. Each test produces a flame and may produce soot clusters that glow yellow when hot. These clusters grow larger in microgravity than on Earth because the soot remains within the flame longer.

Designing Flames Aboard the International Space Station

This experiment’s results could enable the design of flames that are more sooty or soot-free, depending on the need of a specific application. “When you're completely finished with the combustion process, in general you want to have complete burnout of all the soot. That’s true when you're producing power,” says Axelbaum. “There are some other cases where your goal is to produce carbon black which is a form of soot.” For the most part though, these results may help create more efficient and less polluting burner designs.

The knowledge gained from these combustion experiments aboard the orbiting laboratory is helping us better understand fire here on Earth, but it will be crucial when preparing for future missions beyond low Earth orbit. “Part of the future is looking at partial gravity,” says Stocker. “Understanding that will be important for fire safety on other worlds, like the Moon or Mars.”

Related links:

FLame Extinguishment Experiment (FLEX): http://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=655

Saffire experiments: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1543

Advanced Combustion via Microgravity Experiments (ACME): http://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1651

Flame Design: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=2059

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), Video (NASA), Text, Credits: NASA/Michael Johnson/JSC/International Space Station Program Science Office/Erin Winick.

Greetings, Orbiter.ch

A burst of asteroid activity in Europe









ESA - European Space Agency patch.

10 September 2019

Hera approaches the impact scene

The next few days will see a rare convergence of asteroid-related activity in Europe, as planetary defence and other experts meet in three locations to coordinate humanity's efforts to defend ourselves from hazardous space rocks.

Such intense levels of international scientific collaboration are driven in part by the fact that an asteroid impact could cause devastating effects on Earth. But this is also a testament to the fact that we are at a point in human history where we can do something about risky asteroids.

Infographic: asteroid danger explained

According to recent ESA estimates, there are 878 asteroids in the ‘risk list’. This ESA catalogue brings together all asteroids we know of that have a ‘non-zero’ chance of impacting Earth in the next 100 years – meaning that an impact, however unlikely, cannot be ruled out.

An impact by even a small asteroid could cause serious destruction to inhabited areas. This is why ESA, together with international partners, is taking action to search for asteroids, develop technology that could deflect them in future and collaborate at the international level to support mitigation measures.

The flurry of upcoming meetings will cover vital topics in planetary defence, including the planned, first-ever test of asteroid deflection, coordination and communication of asteroid warnings and how to ensure the most effective emergency response on the ground. With all the work being done, the planet has never been so prepared for the unlikely but very real threat of an asteroid impact.

11-13 September, AIDA workshop, Rome

The ESA/NASA “AIDA” collaboration (for Asteroid Impact Deflection Assessment) will see NASA’s DART spacecraft crash into and deflect the 160-m asteroid Didymos-B (also known as Didymoon, the smaller of the Didymos dual asteroid system).

Later, ESA’s Hera mission will survey the crash site and gather the maximum possible data on the effects of this collision.

Hera: ESA’s planetary defence mission

The AIDA workshop brings together asteroid researchers and spacecraft engineers from the US, Europe and around the world to discuss the latest in this first-ever test of asteroid deflection, planned for 2022.

Astronomers from both sides of the Atlantic will also be reporting on the latest observation campaigns to gather additional data on the Didymos asteroid system, helping with the planning of both missions.

12-13 September, IAWN/SNPAG meeting, Munich

The International Asteroid Warning Network, currently led by NASA, and the ESA-chaired Space Mission Planning Advisory Group regularly meet to discuss all things asteroid.

Both groups have mandates from the UN to coordinate, at the international level, different aspects of any future responses to any asteroid risks.

The un-detection of asteroid 2006 QV89

The latest meetings will be hosted by the European Southern Observatory in Garching, Munich.

The organisations will discuss the recent ‘non-detection’ of asteroid 2006 QV89, the latest news from the Minor Planet Center and how asteroid warnings are communicated to the public and media.

16-17 September, ESA's third emergency response workshop, ESOC

Representatives of civil protection agencies from six countries including Germany, Switzerland and the US, as well as from the United Nations Office for Outer Space Affairs, will join ESA’s Planetary Defence Office at the Agency’s operations centre in Darmstadt, Germany.

This will be the third in a series of emergency response workshops with the purpose of establishing a link between ESA and national civil protection authorities, ensuring national agencies understand the asteroid threat and how ESA can support them in their work to protect life and infrastructure on the ground.

Chelyabinsk sky rendering

These three meetings illustrate the breadth of activity currently taking place across the globe to mitigate the risk of an asteroid impact, to ensure early warnings of such a threat, and to prepare on Earth in the unlikely event of a strike – planetary defence is heating up!

Find out more about ESA’s Planetary Defence activities, here: http://www.esa.int/Our_Activities/Space_Safety/Risky_asteroids

Related links:

AIDA: http://www.esa.int/Our_Activities/Space_Safety/Hera/AIDA

DART: https://www.nasa.gov/planetarydefense/dart

Hera: http://www.esa.int/Our_Activities/Space_Safety/Hera

International Asteroid Warning Network: http://iawn.net/

Space Mission Planning Advisory Group: https://www.cosmos.esa.int/web/smpag

European Southern Observatory (ESO): https://www.eso.org/

Minor Planet Center: https://minorplanetcenter.net/iau/mpc.html

United Nations Office for Outer Space Affairs: http://www.unoosa.org/

Space Safety: http://www.esa.int/Our_Activities/Space_Safety

Animation, Images, Video, Text, Credits: ESA CC BY-SA 3.0 IGO/ESO/ O. Hainaut/Sandia Labs CC BY-NC-ND 2.0.

Greetings, Orbiter.ch

Hubble Explores the Formation and Evolution of Star Clusters in the Large Magellanic Cloud













ESA - Hubble Space Telescope logo.

10 September 2019

Globular Cluster NGC 1466

Just as people of the same age can vary greatly in appearance and shape, so do collections of stars or stellar aggregates. New observations from the NASA/ESA Hubble Space Telescope suggest that chronological age alone does not tell the complete story when it comes to the evolution of star clusters.

Previous research on the formation and evolution of star clusters has suggested that these systems tend to be compact and dense when they form, before expanding with time to become clusters of both small and large sizes. New Hubble observations in the Large Magellanic Cloud (LMC) galaxy have increased our understanding of how the size of star clusters in the LMC changes with time[1].

Star clusters are aggregates of many (up to one million) stars. They are active systems in which the mutual gravitational interactions among the stars change their structure over time (known to astronomers as "dynamical evolution"). Because of such interactions, heavy stars tend to progressively sink towards the central region of a star cluster, while low-mass stars can escape from the system. This causes a progressive contraction of the cluster core over different timescales and means that star clusters with the same chronological age can vary greatly in appearance and shape because of their different “dynamical ages”.

Artist’s Impression of Blue Stragglers

Located nearly 160 000 light-years from Earth, the LMC is a satellite galaxy of the Milky Way which hosts star clusters covering a wide range of ages. This differs from our own Milky Way galaxy which primarily contains older star clusters. The distribution of sizes as a function of age observed for star clusters in the LMC is very puzzling, as the young clusters are all compact, while the oldest systems have both small and large sizes.

All star clusters, including those in the LMC, have been found to host a special type of re-invigorated stars called blue stragglers [2]. Under certain circumstances, stars receive extra fuel that bulks them up and substantially brightens them. This can happen if one star pulls matter off a neighbour, or if they collide.

As a result of dynamical aging, heavier stars sink towards the centre of a cluster as the cluster ages, in a process similar to sedimentation, called “central segregation”.  Blue stragglers are bright, making them relatively easy to observe, and they have high masses, which means that they are affected by central segregation and can be used to estimate the dynamical age of a star cluster [3].

The formation of blue stragglers

Francesco Ferraro of the University of Bologna in Italy and his team used the Hubble Space Telescope to observe blue stragglers in five (coeval) old  LMC star clusters with different sizes and succeeded in ranking them in terms of their dynamical age.

“We demonstrated that different structures of star clusters are due to different levels of dynamical ageing: they are in different physical shape despite the fact that they were born at the same cosmic time. This is the first time that the effect of dynamical ageing has been measured in the LMC clusters” says Ferraro.

Animation of Blue Stragglers

“These findings present intriguing areas for further research, since they reveal a novel and valuable way of reading the observed patterns of LMC star clusters, providing new hints about the cluster formation history in the LMC galaxy,” adds co-author Barbara Lanzoni.

Notes:

[1] The observations were achieved from a set of long exposures acquired with the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 (WFC3) and Advanced Camera for Surveys (ACS) for five old star clusters in the Large Magellanic Cloud galaxy, secured under proposal 14164 (PI: Sarajedini).  http://archive.stsci.edu/proposal_search.php?mission=hst&id=14164

[2] Blue stragglers are so called because of their blue colour, and the fact that their evolution lags behind that of their neighbours.

[3] Blue stragglers combine being relatively bright and having high mass by the standards of globular cluster stars, but they are not the only stars within these clusters that are either bright or massive.

Hubble Space Telescope (HST)

More information:

The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

The team’s paper will appear in Nature Astronomy.

The international team of astronomers in this study consists of F. Ferraro (University of Bologna, Italy and INAF, Italy), B. Lanzoni (University of Bologna, Italy and INAF, Italy), E. Dalessandro (INAF, Italy), M. Cadelano (University of Bologna, Italy and INAF, Italy), S. Raso (University of Bologna, Italy and INAF, Italy), A. Mucciarelli (University of Bologna, Italy and INAF, Italy), G. Beccari (European Southern Observatory, Germany), C. Pallanca (University of Bologna, Italy and INAF, Italy). More information about the paper can be found here:
http://www.cosmic-lab.eu/Cosmic-Lab/LMC_dynamicalage.html

Links:

Hubble Space Telescope (HST): http://www.spacetelescope.org/

Images of Hubble: http://www.spacetelescope.org/images/archive/category/spacecraft/

Hubblesite release: https://hubblesite.org/contents/news-releases/2019/news-2019-42

Science paper: http://www.spacetelescope.org/static/archives/releases/science_papers/heic1915/heic1915a.pdf

Images, Animation, Video, Text, Credits: ESA/Hubble & NASA/L. Calçada/M. Kornmesser.

Best regards, Orbiter.ch

lundi 9 septembre 2019

Day Before HTV-8 Launch, Crew Studies Effects of Microgravity on Space-faring Humans













ISS - Expedition 60 Mission patch.

September 9, 2019

The International Space Station is abuzz as preparations heat up for the launch of the Japan Aerospace Exploration Agency HTV-8 “Kounotori” cargo craft from the Tanegashima Space Center tomorrow, Sept. 10. Launch is slated for 5:33 p.m. EDT, and can be seen live on NASA Television. 

NASA astronauts Christina Koch and Andrew Morgan spent more time practicing 30-meter approach and capture runs, followed by their own evaluations, in preparation for HTV-8’s arrival days later on Saturday, Sept. 14. The vehicle will be loaded with more than four tons of supplies, spare parts and experiment hardware for the space station residents.


Image above: At the Gagarin Cosmonaut Training Center in Star City, Russia, spaceflight participant Hazzaa Ali Almansoori of the United Arab Emirates (left), Oleg Skripochka of Roscosmos (center) and Jessica Meir of NASA (right) pose for pictures Sept. 5 as part of a pre-flight news conference. They will launch Sept. 25 from the Baikonur Cosmodrome in Kazakhstan on the Soyuz MS-15 spacecraft for a mission on the International Space Station. Image Credit: Gagarin Cosmonaut Training Center.

In the Kibo module, Morgan spoke to media out of Morgantown, West Virginia, referencing not only of NASA’s future with the Artemis program, but also the work currently underway that will benefit life on Earth and expand humanity’s reach into the solar system. Morgan referenced his early morning tasks with Fluid Shifts and his first spacewalk just weeks before, when he and NASA astronaut Nick Hague installed International Docking Adapter to usher in a new era of commercial visiting vehicles that will launch from American soil. 

Science investigations that will help develop countermeasures for humans exploring deep space, and for longer durations, rounded out the busy Monday. Commander Alexey Ovchinin of Roscosmos and crewmates Koch and Hague conducted eye exams aboard the orbiting laboratory. Since it is known that living and working in microgravity can induce vascular changes, as well as head and eye pressure, these measurements will help medical experts and scientists on the ground track crew health as Expedition 60 continues. Furthering research for Fluid Shifts, all other crewmates, with the exception of Koch and ESA (European Space Agency) astronaut Luca Parmitano, conducted venous ultrasounds in support of ongoing studies into vascular and fluid movement within space-faring human bodies.


Image above: Expedition 60 crew members Drew Morgan and Nick Hague pose with the spacesuits they wore during a recent spacewalk to install equipment that will accommodate the future arrivals of commercial crew spacecraft. Image Credit: NASA.

Parmitano, meanwhile, worked to close out Space Moss, an experiment that helps decode how microgravity affects the growth, development, gene expression and photosynthetic activity of tiny, rootless moss plants growing within the Cell Biology Experiment Facility incubator on the orbiting laboratory. 

Back on Earth, cosmonaut Oleg Skripochka, NASA astronaut Jessica Meir and spaceflight participant Hazzaa Ali Almansoori are set to depart for the Baikonur Cosmodrome in Kazakhstan tomorrow after spending the week prior taking part in ceremonial activities and mission briefings leading up to their mission start on Sept. 25, when they launch into space aboard a Soyuz MS-15 spacecraft.

Related links:

Expedition 60: https://www.nasa.gov/mission_pages/station/expeditions/expedition60/index.html

Japan Aerospace Exploration Agency HTV-8: https://www.nasa.gov/press-release/nasa-television-to-air-launch-capture-of-cargo-ship-to-space-station

Kibo module: https://www.nasa.gov/mission_pages/station/structure/elements/japan-kibo-laboratory

Fluid Shifts: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1126

NASA Television: https://www.nasa.gov/nasalive/

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

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), Text, Credits: NASA/Catherine Williams.

Best regards, Orbiter.ch

NASA Estimates Hurricane Dorian’s Massive Rainfall Track













NASA & JAXA - Global Precipitation Measurement (GPM) patch.

Sep. 09, 2019

Dorian – Atlantic Ocean

On Monday morning, September 9, Hurricane Dorian was a post-tropical storm after a mid-latitude weather front and cold seas had altered its tropical characteristics over the weekend. NASA compiled data on Hurricane Dorian and created a map that showed the heavy rainfall totals it left in its wake from the Bahamas to Canada.


Image above: At one-day intervals, the image shows the distance that tropical-storm force (39 mph) winds extended from Hurricane Dorian’s low-pressure center, as estimated by the National Hurricane Center. The Saffir-Simpson hurricane-intensity category is the number following the “H” in the label on the image. “TS” or “PT” indicate times when the storm was either at tropical storm strength or when the storm was categorized as post-tropical. Red circles over North Carolina indicate preliminary reports of tornadoes on Sept. 5. Image Credits: NASA Goddard.

On Saturday and Sunday, Sept. 7 and 8, Hurricane Dorian struck eastern Canada, causing wind damage and bringing heavy rainfall.  According to the Associated Press, a peak of 400,000 people were without power in Nova Scotia, Canada, because of Dorian.

At NASA’s Goddard Space Flight Center in Greenbelt, Maryland, a graphic was produced that shows precipitation that fell during the almost two-week period from August 27 to the early hours of Sept. 9. The near-real-time rain estimates come from the NASA’s IMERG algorithm, which combines observations from a fleet of satellites, in near real time, to provide near-global estimates of precipitation every 30 minutes.

his year, NASA began running an improved version of the IMERG algorithm that does a better job estimating precipitation at high latitudes, specifically north of 60 degrees North latitude. The post-tropical remnants of Hurricane Dorian were approaching this cold region at the end of the analysis period. While the IMERG algorithm is still unable to estimate precipitation falling over ice-covered surfaces (such as Greenland), IMERG can now give a more complete picture of the water cycle in places such as Canada, which is, for the most part, free of snow cover at this time of year.

In addition to rainfall totals, the map includes preliminary reports of tornadoes from 4:50 AM to 5:00 PM EDT on September 5 in North Carolina as provided by NOAA’s Storm Prediction Center.

IMERG showed largest rainfall amounts of more than 36 inches over the Bahamas and in an area off the coast of northeastern Florida. A large area of rainfall between 16 and 24 inches fell in many areas off the U.S. East Coast. Areas include those from South Carolina to the Bahamas, another off the North Carolina coast, a third area off the coasts of southern New Jersey, Delaware and Maryland, and the New England states.

By combining NASA precipitation estimates with other data sources, we can gain a greater understanding of major storms that affect our planet.

Global Precipitation Measurement (GPM) satellite. Image Credits: NASA/JAXA

On Monday, Sept. 9 at 0300 UTC (Sept. 8 a t 11 p.m. EDT), NOAA’s National Hurricane Center (NHC) issued the final advisory on Dorian. At that time, Dorian had moved into the Labrador Sea and its impacts on Newfoundland were beginning to subside. Post-tropical cyclone Dorian had maximum sustained winds near 50 knots (57 mph/93 kph). It was centered near 52.1 degrees north latitude and 53.4 degrees west longitude. That puts the center about 375 miles north of Cape Race, Newfoundland, Canada. Dorian was speeding to the east-northeast at 21 knots. Minimum central pressure was 980 millibars.

On Sept. 9, additional rainfall totals expected from Dorian in far eastern Quebec, Newfoundland and Labrador are expected to be less than 1 inch. Meanwhile, life-threatening rip tide and surf conditions are expected to affect mid-Atlantic and New England coasts of the U.S., as well as the coast of Atlantic Canada.

The NHC said the cyclone will continue into the open Atlantic, where it will dissipate south of Greenland.

Related articles:

NASA Finds Dorian Transitioning to an Extra-Tropical Cyclone
https://orbiterchspacenews.blogspot.com/2019/09/nasa-finds-dorian-transitioning-to.html

NASA Measures Dorian’s Heavy Rainfall from Bahamas to Carolinas
https://orbiterchspacenews.blogspot.com/2019/09/nasa-measures-dorians-heavy-rainfall.html

For updated forecasts, visit: http://www.nhc.noaa.gov/

Global Precipitation Measurement (GPM): https://www.nasa.gov/mission_pages/GPM/main/index.html

For more about NASA’s IMERG, visit: https://pmm.nasa.gov/gpm/imerg-global-image

Images (mentioned), Text, Credits: NASA’s Goddard Space Flight Center, by Owen Kelley/Rob Gutro.

Greetings, Orbiter.ch

New Models Suggest Titan Lakes Are Explosion Craters













NASA & ESA - Cassini Mission to Saturn & Titan patch.

Sept. 9, 2019

Using radar data from NASA's Cassini spacecraft, recently published research presents a new scenario to explain why some methane-filled lakes on Saturn's moon Titan are surrounded by steep rims that reach hundreds of feet high. The models suggests that explosions of warming nitrogen created basins in the moon's crust.

Titan is the only planetary body in our solar system other than Earth known to have stable liquid on its surface. But instead of water raining down from clouds and filling lakes and seas as on Earth, on Titan it's methane and ethane — hydrocarbons that we think of as gases but that behave as liquids in Titan's frigid climate.


Image above: This artist's concept of a lake at the north pole of Saturn's moon Titan illustrates raised rims and rampartlike features such as those seen by NASA's Cassini spacecraft around the moon's Winnipeg Lacus. Image Credits: NASA/JPL-Caltech.

Most existing models that lay out the origin of Titan's lakes show liquid methane dissolving the moon's bedrock of ice and solid organic compounds, carving reservoirs that fill with the liquid. This may be the origin of a type of lake on Titan that has sharp boundaries. On Earth, bodies of water that formed similarly, by dissolving surrounding limestone, are known as karstic lakes.

The new, alternative models for some of the smaller lakes (tens of miles across) turns that theory upside down: It proposes pockets of liquid nitrogen in Titan's crust warmed, turning into explosive gas that blew out craters, which then filled with liquid methane. The new theory explains why some of the smaller lakes near Titan's north pole, like Winnipeg Lacus, appear in radar imaging to have very steep rims that tower above sea level — rims difficult to explain with the karstic model.

The radar data were gathered by the Cassini Saturn Orbiter — a mission managed by NASA's Jet Propulsion Laboratory in Pasadena, California — during its last close flyby of Titan, as the spacecraft prepared for its final plunge into Saturn's atmosphere two years ago. An international team of scientists led by Giuseppe Mitri of Italy's G. d'Annunzio University became convinced that the karstic model didn't jibe with what they saw in these new images.

"The rim goes up, and the karst process works in the opposite way," Mitri said. "We were not finding any explanation that fit with a karstic lake basin. In reality, the morphology was more consistent with an explosion crater, where the rim is formed by the ejected material from the crater interior. It's totally a different process."

The work, published Sept. 9 in Nature Geosciences, meshes with other Titan climate models showing the moon may be warm compared to how it was in earlier Titan "ice ages."

Over the last half-billion or billion years on Titan, methane in its atmosphere has acted as a greenhouse gas, keeping the moon relatively warm — although still cold by Earth standards. Scientists have long believed that the moon has gone through epochs of cooling and warming, as methane is depleted by solar-driven chemistry and then resupplied.

Artist^s view of Cassini Titan flyby's. Image Credit: NASA/JPL

In the colder periods, nitrogen dominated the atmosphere, raining down and cycling through the icy crust to collect in pools just below the surface, said Cassini scientist and study co-author Jonathan Lunine of Cornell University in Ithaca, New York.

"These lakes with steep edges, ramparts and raised rims would be a signpost of periods in Titan's history when there was liquid nitrogen on the surface and in the crust," he noted. Even localized warming would have been enough to turn the liquid nitrogen into vapor, cause it to expand quickly and blow out a crater.

"This is a completely different explanation for the steep rims around those small lakes, which has been a tremendous puzzle," said Cassini Project Scientist Linda Spilker of JPL. "As scientists continue to mine the treasure trove of Cassini data, we'll keep putting more and more pieces of the puzzle together. Over the next decades, we will come to understand the Saturn system better and better."

The Cassini-Huygens mission is a cooperative project of NASA, ESA (the European Space Agency) and the Italian Space Agency. JPL, a division of Caltech in Pasadena, manages the mission for NASA's Science Mission Directorate in Washington. JPL designed, developed and assembled the Cassini orbiter. The radar instrument was built by JPL and the Italian Space Agency, working with team members from the U.S. and several European countries.

Titan's lakes: https://www.jpl.nasa.gov/news/news.php?feature=7378

More information about Cassini can be found here: https://solarsystem.nasa.gov/cassini

Images (mentioned), Text, Credits: NASA/Jon Nelson/Alana Johnson/JPL/Gretchen McCartney.

Best regards, Orbiter.ch