lundi 10 septembre 2018

Science and Suit Work as Storms Capture Attention













ISS - Expedition 56 Mission patch.

September 10, 2018

The six Expedition 56 crew members started the workweek today with life science and spacesuit maintenance. Meanwhile, a typhoon and a hurricane captured the attention of mission managers and the crew alike.

Commander Drew Feustel and Flight Engineer Ricky Arnold examined mice onboard the International Space Station and them today for the Rodent Research-7 (RR-7) experiment. The duo checked the breathing and mass of the rodents before placing them back in their habitat and restocking their food. RR-7 is observing how microgravity impacts gut microbes and how it may affect astronaut health.


Image above: Astronaut Ricky Arnold captured this view of Hurricane Florence on Sept. 10 as it churned in the Atlantic headed for the U.S. east coast. Image Credit: @Astro_Ricky.

German astronaut Alexander Gerst of ESA (European Space Agency) wrapped up an experiment before finalizing spacesuit work in the U.S. Quest airlock. He stowed science gear in the morning that analyzed the exhaled air of astronauts to detect signs of airway inflammation. In the afternoon, Gerst completed the battery charging of the U.S. spacesuits then began regenerating metal oxide canisters in advance of a pair of spacewalks at the end of the month.

JAXA (Japan Aerospace Exploration Agency) officials are tracking Typhoon Mangkhut in the Pacific while the station crew sent down imagery of Hurricane Florence in the Atlantic. Mangkhut was moving on a course near a tracking site in Guam which JAXA uses to follow the progress of the Japanese HTV cargo craft after its launch. That launch was postponed from today to a later date. On the other side of the world, the station flew over Hurricane Florence as it neared the U.S. east coast enabling the crew to capture imagery to share with the world.

Hurricane Florence Views from Space Station

Dramatic Views of Hurricane Florence

Video above: Cameras outside the International Space Station captured dramatic views of rapidly strengthening Hurricane Florence at 8:10 a.m. EDT Sept. 10 as it moved in a westerly direction across the Atlantic, headed for a likely landfall along the eastern seaboard of the U.S. late Thursday or early Friday. Now a major hurricane with winds of 115 miles an hour and increasing, the National Hurricane Center says Florence’s forecast track will take the system over the southwestern Atlantic Ocean between Bermuda and the Bahamas Tuesday and Wednesday, and Florence will approach the coast of South Carolina or North Carolina on Thursday. The station was flying 255 miles over the storm at the time this video was captured. Video Credit: NASA.

ISS Sees Florence From Space

Top down look at Florence from the International Space Station. Image Credit: NASA
 
A few moments later, Isaac & the outer bands of Helene were also visible. Image Credit: NASA

Related links:

Expedition 56: https://www.nasa.gov/mission_pages/station/expeditions/expedition56/index.html

Rodent Research-7 (RR-7): https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7425

Airway inflammation: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1067

Spacewalks: https://www.nasa.gov/mission_pages/station/spacewalks

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

Best regards, Orbiter.ch

NASA Satellites Show Hurricane Florence Strengthening














NASA & JAXA - Global Precipitation Measurement (GPM) patch/ NASA - EOS Aqua Mission logo.

Sep. 10, 2018

NASA satellites are providing a lot of different kinds of data to forecasters at the National Hurricane Center to help them understand what’s happening Hurricane Florence. NASA’s Aqua satellite is providing visible, infrared and microwave imagery while the GPM core satellite is providing additional data like rain rates throughout the storm and cloud heights.


Image above: At 1:55 a.m. EDT (0555 UTC) on Sept. 10, the MODIS instrument aboard NASA’s Aqua satellite looked at Hurricane Florence in infrared light. MODIS found coldest cloud tops (red) had temperatures near minus 70 degrees Fahrenheit (minus 56.6 degrees Celsius) in the northern and western eyewall. Image Credits: NASA/NRL.

Last Friday, Sept. 7, Florence was a sheared tropical storm but on Saturday vertical shear lessened and Florence started to get better organized. Today, Sept. 10 Hurricane Florence was rapidly strengthening and became a major hurricane.

NOAA’s National Hurricane Center (NHC) said “Interests in the southeastern and mid-Atlantic states should monitor the progress of Florence. Storm Surge and Hurricane watches could be issued for portions of these areas by Tuesday morning”.

The Global Precipitation Measurement mission or GPM core observatory satellite had a fairly good look at Florence on Sunday, Sept. 9, 2018 at 2:13 p.m. EDT (1813 UTC). GPM is a joint satellite mission between NASA and the Japan Aerospace Exploration Agency called JAXA.


Image above: The GPM core observatory satellite had a fairly good look at Florence on Sunday, Sept. 9, 2018 at 2:13 p.m. EDT (1813 UTC). GPM estimated that precipitation was falling at a rate of greater than 44 mm (1.7 inches) per hour in a band of thunderstorms south of Florence’s center. Image Credits: NASA/JAXA, Hal Pierce.

When GPM observed Florence, the intensifying storm had maximum sustained winds of about 70 knots (81 mph) at that time and was still a tropical storm. At the time GPM observed Florence, GPM’s Microwave Imager (GMI) instruments revealed distinct rain bands wrapping around Florence’s southeastern side. Algorithms developed by NASA’s Precipitation Measurement Missions (PMM) team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland were used with GMI data and estimated that precipitation was falling at a rate of greater than 44 mm (1.7 inches) per hour in the rain band.

At NASA Goddard, a 3-D animation was created using data observed by GPM’s radar (DPR Ku Band), that showed the relative heights of storm tops within Florence. Those data were blended with estimates from geostationary satellite cloud top temperatures.

That heavy rainfall was confirmed in NASA infrared imagery the next day, Monday, Sept. 10. At 1:55 a.m. EDT (0555 UTC) on Sept. 10, from the Moderate Resolution Imaging Spectroradiometer or MODIS instrument aboard NASA’s Aqua satellite revealed strongest storms in Florence were in the northern and western part of the eyewall. In those areas, MODIS found coldest cloud tops had temperatures near minus 70 degrees Fahrenheit (minus 56.6 degrees Celsius). NASA research has found that cloud top temperatures that cold have the capability to generate heavy rainfall.

At 3:21 a.m. EDT (0721 UTC) the AIRS or Atmospheric Infrared Sounder instrument aboard Aqua provided another, wider infrared view of the storm that showed powerful thunderstorms with cloud tops as cold as or colder than minus 63 degrees Fahrenheit (minus 53 degrees Celsius) made up most of the storm. Temperatures that cold were also found in fragmented bands of storms south of Florence’s center.

Florence’s Status on Sept. 10 at 11 a.m. EDT

At 11 a.m. EDT (1500 UTC), the eye of Hurricane Florence was located near latitude 25.0 degrees north and longitude 60.0 degrees west. Florence is moving toward the west near 13 mph (20 kph).  A west-northwestward motion with an increase in forward speed is expected during the next couple of days.

GPM Flyby of Florence

Video above: The GPM core observatory satellite had a fairly good look at Florence on Sunday, Sept. 9, 2018 at 2:13 p.m. EDT (1813 UTC). GPM estimated that precipitation was falling at a rate of greater than 44 mm (1.7 inches) per hour in a band of thunderstorms south of Florence’s center. Video Credits: NASA/JAXA, Hal Pierce.

The NHC said, a turn toward the northwest is forecast to occur late Wednesday night.  On the forecast track, the center of Florence will move over the southwestern Atlantic Ocean between Bermuda and the Bahamas Tuesday and Wednesday, and approach the coast of South Carolina or North Carolina on Thursday.

Satellite data indicate that maximum sustained winds have increased to near 115 mph (185 kph) with higher gusts.  Florence is a category 3 hurricane on the Saffir-Simpson Hurricane Wind Scale. Further strengthening is anticipated, and Florence is expected to be an extremely dangerous major hurricane through Thursday.

Ocean swells generated by Florence are affecting Bermuda and portions of the U.S. East Coast.  These swells are likely to cause life-threatening surf and rip current conditions.

The NHC predicts that Florence’s winds will decrease slightly to 125 knots (144 mph) as the hurricane threatens the southeastern United States on Thursday September 13, 2018.

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

NASA’s Aqua satellite: https://aqua.nasa.gov/

NASA GPM satellite: https://www.nasa.gov/mission_pages/GPM/main/index.html

JAXA GPM satellite: http://global.jaxa.jp/projects/sat/gpm/

Images (mentioned), Video (mentioned), Text, Credits: NASA’ Goddard Space Flight Center, by Rob Gutro.

Greetings, Orbiter.ch

dimanche 9 septembre 2018

Japanese Cargo Mission Postponed













ISS - International Space Station logo.

September 9, 2018

As a result of adverse weather conditions, the Japan Aerospace Exploration Agency (JAXA) has postponed the scheduled launch of a Japanese cargo spacecraft from the Tanegashima Space Center in southern Japan.


Image above: Japan’s third resupply ship, the HTV-3, is pictured in September of 2012 attached to the International Space Station’s Harmony module. Image Credit: NASA.

The unpiloted H-II Transfer Vehicle-7 (HTV-7) is loaded with more than five tons of supplies, water, spare parts and experiments for the crew aboard the International Space Station.

A new launch date has not yet been determined.

JAXA Press Release:

Launch Postponed H-II Transfer Vehicle KOUNOTORI7 aboard the H-IIB Vehicle No. 7:
http://global.jaxa.jp/press/2018/09/20180909_h2bf7.html

Related links:

H-II Transfer Vehicle "KOUNOTORI" (HTV): http://global.jaxa.jp/projects/rockets/htv/

H-II Transfer Vehicle-7 (HTV-7): https://www.nasa.gov/mission_pages/station/structure/elements/htv.html

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

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

Greetings, Orbiter.ch

samedi 8 septembre 2018

Long March 2C launches Haiyang-1C













CASC - China Aerospace Science and Technology Corporation logo.

September 8, 2018

Haiyang-1C launched by Long March 2C

On September 7, 2018, China launched its third ocean survey satellite of the Haiyang-1 series on Friday, with the launch taking place from the Taiyuan Satellite Launching Center at 03:15 UTC. A Long March-2C (Chang Zheng-2C) rocket was used to loft the new satellite.

Haiyang-1C will be used to monitor and prevent oceanic pollution, resource investigation, construction of bayou and ports, and for the development of coastal areas, using the system to monitor ocean temperatures.

Haiyang-1C (HY-1C) launched by Long March-2C

Onboard HY-1C there are two instruments: The China Ocean Colour & Temperature Scanner (COCTS), a medium-resolution optical imager developed by SITP (Shanghai Institute of Technical Physics) of CAS (China Academy of Sciences), and the Coastal Zone Imager (CZI), a multispectral push broom CCD instrument developed by the Beijing Institute of Space Machines and Electricity, CAST.

Developed for measuring the ocean color and sea surface temperature, the 50 kg COCTS will be used for determining the Aerosol Optical Depth, Aerosol column burden, biomass, the Colour Dissolved Organic Matter (CDOM) and the Earth surface albedo.

Haiyang-1C satellite

The 15 kg CZI will be used to analyze the vegetation and coastal zone, determining the biomass, the Fraction of Absorbed PAR (FAPAR), Fraction of vegetated land, Land cover and the Leaf Area Index (LAI). The CZI used on Haiyang-1C was improved to 50 m resolution (from 250 m from the Haiyang-1B) and also has a wider image swath.

HY-1C is now able to image at up to 20 degrees pitch angles which would minimize problems from sun spots. The satellite lifetime is now five years (up from 3-5 years on HY-1B).

For more information about China Aerospace Science and Technology Corporation (CASC), visit: http://english.spacechina.com/n16421/index.html

Images, Video, Text, Credits: CASC/China Central Television (CCTV)/SciNews/NASA Spaceflight.com/Rui C. Barbosa.

Greetings, Orbiter.ch

vendredi 7 septembre 2018

The incredible lightness of the Higgs













CERN - European Organization for Nuclear Research logo.

7 Sep 2018

Why is the Higgs boson so light? That’s one of the questions that has been bothering particle physicists since the famous particle was discovered in 2012. This is because the theory of how the particle interacts with the most massive of all observed elementary particles, the top quark, involves corrections at a fundamental (quantum) level that could result in a Higgs mass much larger than the measured value of 125 GeV. How large? Perhaps as much as sixteen orders of magnitude larger than the measured Higgs mass. Since the Higgs mass is so light, this suggests more particles could exist that cancel the quantum corrections from the top quark (and other heavy particles).

In a paper posted online and submitted to the journal Physical Review Letters, the ATLAS collaboration reports results of a combination of searches for a new particle – dubbed a vector-like top quark – that could help keep the Higgs boson light.


Image above: View of the ATLAS detector. The ATLAS collaboration reports results of a combination of searches for a new particle – dubbed a vector-like top quark – that could be the culprit behind the Higgs lightness. (Image: Claudia Marcelloni/ATLAS CERN).

Various proposals attempt to cancel out the large quantum corrections to the Higgs boson mass. Many of them involve vector-like top quarks, which are hypothetical particles not predicted by the Standard Model of particle physics. Unlike the Standard Model top quark, which always decays to a bottom quark and a W boson, vector-like top quarks would decay in one of three different ways, if they decayed to Standard Model particles. Specifically, a vector-like top quark would decay to a bottom quark and a W boson, or to a Z boson and a top quark, or still to a Higgs boson and a top quark.

To maximise the chances of finding vector-like top quarks, the ATLAS collaboration conducted several different types of search using data from proton–proton collisions collected at the Large Hadron Collider (LHC) in 2015 and 2016 at an energy of 13 TeV; each individual search is sensitive to a particular set of particle decays. They then combined the results to increase the sensitivity to vector-like top quarks, yet found no sign of them.

Despite this, their analysis allowed them to expand the reach of individual searches and place the most stringent lower bounds on the mass of vector-like top quarks to date. The analysis excludes vector-like top quarks with masses below about 1300 GeV for any combination of the three top-quark decays into Standard Model particles. The previous best lower limit from an individual search was 1190 GeV.

It will now get more challenging: for masses heavier than 1300 GeV a single vector-like top quark is created more often than a pair. But with a wealth of data coming from the LHC, the search continues.

Note:

CERN, the European Organization for Nuclear Research, is one of the world’s largest and most respected centres for scientific research. Its business is fundamental physics, finding out what the Universe is made of and how it works. At CERN, the world’s largest and most complex scientific instruments are used to study the basic constituents of matter — the fundamental particles. By studying what happens when these particles collide, physicists learn about the laws of Nature.

The instruments used at CERN are particle accelerators and detectors. Accelerators boost beams of particles to high energies before they are made to collide with each other or with stationary targets. Detectors observe and record the results of these collisions.

Founded in 1954, the CERN Laboratory sits astride the Franco–Swiss border near Geneva. It was one of Europe’s first joint ventures and now has 22 Member States.

Related links:

Physical Review Letters: https://arxiv.org/abs/1808.02343

Higgs boson: https://home.cern/topics/higgs-boson

Standard Model of particle physics: https://home.cern/about/physics/standard-model

ATLAS: https://home.cern/about/experiments/atlas

Large Hadron Collider (LHC): https://home.cern/topics/large-hadron-collider

For more information about European Organization for Nuclear Research (CERN), Visit: https://home.cern/

Image (mentioned), Text, Credits: CERN/Ana Lopes.

Best regards, Orbiter.ch

Japan Is Go for Monday Cargo Launch to Station












ISS - Expedition 56 Mission patch.

September 7, 2018

Japan’s seventh cargo mission (HTV-7) to the International Space Station is in the final stages of preparation for launch on Monday at 7:32 p.m. EDT. Mission controllers are monitoring the weather at the Tanegashima Space Center launch site while the Expedition 56 crew is preparing for its arrival early Friday.

JAXA’s (Japan Aerospace Exploration Agency) HTV-7 is delivering a wide variety of science gear to support new research aboard the orbital lab. The new facilities will enable astronauts to observe physical processes at high temperatures, protein crystal growth and genetic alterations as well as a variety of other important space phenomena.


Image above: The Japanese HTV-6 cargo vehicle is seen during final approach to the International Space Station on Dec. 13, 2016. Image Credit: NASA:

HTV-7, also known as Kounotori, is also carrying six new lithium-ion batteries that robotics controllers will remove then install on the station’s port 4 truss structure. Astronauts Alexander Gerst, Drew Feustel and Ricky Arnold will complete the battery maintenance work over two spacewalks set for Sept. 20 and 26.

Feustel will lead the effort to capture Kounotori when he commands the Canadarm2 robotic arm to reach out and grapple it Friday at 7:40 a.m. He trained today with Flight Engineer Serena Auñón-Chancellor, who will back him up in the Cupola, practicing capture techniques on a computer.

International Space Station (ISS). Image Credit: NASA/STS-134

All six crew members got together at the end of the day for more eye checks. The sextet from the U.S., Russia and Germany used an ultrasound device, with assistance from doctors on the ground, and scanned each other’s eyes.

Related links:

Expedition 56: https://www.nasa.gov/mission_pages/station/expeditions/expedition56/index.html

JAXA’s (Japan Aerospace Exploration Agency) HTV-7: http://global.jaxa.jp/projects/iss_human/index.html

Spacewalks: https://www.nasa.gov/mission_pages/station/spacewalks

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/Mark Garcia.

Best regards, Orbiter.ch

The Legacy of NASA’s Dawn, Near End of Mission












NASA - Dawn Mission patch.

Sept. 7, 2018

Revealing Solar System Time Capsules, Breaking Engineering Barriers

NASA’s Dawn mission is drawing to a close after 11 years of breaking new ground in planetary science, gathering breathtaking imagery, and performing unprecedented feats of spacecraft engineering.

Dawn’s mission was extended several times as it explored Ceres and Vesta, which when combined, make up 45 percent of the mass of the main asteroid belt. Now, the spacecraft is about to run out of a key fuel, hydrazine. When that happens, most likely between September and October, Dawn will lose its ability to communicate with Earth. It will remain in a silent orbit around Ceres for decades.

“Although it will be sad to see Dawn’s departure from our mission family, we are intensely proud of its many accomplishments,” said Lori Glaze, acting director of the Planetary Science Division at Headquarters in Washington. “Not only did this spacecraft unlock scientific secrets at these two small but significant worlds, it was also the first spacecraft to visit and orbit bodies at two extraterrestrial destinations during its mission. Dawn’s science and engineering achievements will echo throughout history.”

Dusk for Dawn: NASA Mission to the Asteroid Belt

Video above: NASA’s Dawn spacecraft turned science fiction into science fact by using ion propulsion to explore the two largest bodies in the main asteroid belt, Vesta and Ceres. The mission will end this fall, when the spacecraft runs out of hydrazine, which keeps it oriented and in communication with Earth. Video Credit: JPL.

Dawn launched from Cape Canaveral Air Force Station in September 2007, strapped on a Delta II-Heavy rocket. From 2011 to 2012, the spacecraft swept over Vesta, capturing images of craters, canyons and even mountains of this planet-like world.

Then in 2015, Dawn’s cameras spotted a cryovolcano and mysterious bright spots on Ceres, which scientists later found might be salt deposits produced by the exposure of briny liquid from Ceres’ interior.

“Dawn’s legacy is that it explored two of the last uncharted worlds in the inner Solar System,” said Marc Rayman of NASA’s Jet Propulsion Laboratory, Pasadena California, who serves as Dawn’s mission director and chief engineer. “Dawn has shown us alien worlds that, for two centuries, were just pinpoints of light amidst the stars. And it has produced these richly detailed, intimate portraits and revealed exotic, mysterious landscapes unlike anything we’ve ever seen.”

Engineering Feats

Dawn is the only spacecraft to orbit a body in the asteroid belt. And it is the only spacecraft to orbit two extraterrestrial destinations. These feats were possible thanks to ion propulsion, a tremendously efficient propulsion system familiar to science-fiction fans and space enthusiasts. Dawn pushed the limits of the system’s capabilities and stamina, showing how useful it is for other missions that aim to visit multiple destinations.

Pushed by ion propulsion, Dawn reached Vesta in 2011 and investigated it from surface to core during 14 months in orbit. In 2012, engineers maneuvered Dawn out of orbit, and steered it though the asteroid belt for more than two years before inserting it into orbit around the dwarf planet Ceres, where it has been collecting data since 2015.

Artist's view of Dawn spacecraft. Image Credits: NASA/JPL

The mission targeted Ceres and Vesta because they function as time capsules, intact survivors of the earliest part of our history.

“Vesta and Ceres have each told their story of how and where they formed, and how they evolved -- a fiery magmatic history that led to rocky Vesta and a cooler, water-rich history that resulted in the ancient ocean world Ceres,” said Carol Raymond of JPL, principal investigator of the Dawn mission. “These treasure troves of information will continue to help us understand other bodies in the Solar System far into the future.”

Spectacular Ceres

On Ceres’s surface, scientists found the chemistry of an ancient ocean. “What we found was completely mind-blowing. Ceres’ history is just splayed all over its surface,” Raymond said.

Some of the bright spots turned out to be brilliant, salty deposits, made mainly of sodium carbonate that made its way to the surface in a slushy brine from within or below the crust.

The findings reinforce the idea that dwarf planets, not just icy moons like Enceladus and Europa, could have hosted oceans during their history -- and potentially still do. Analyses from Dawn data suggest there still may be liquid under Ceres’ surface and that some regions were geologically active relatively recently, feeding from a deep reservoir.

Bright Spots On Ceres

Image above: Bright surface features on the dwarf planet Ceres known as faculae were first discovered by NASA's Dawn spacecraft in 2015. This mosaic of one such feature, Cerealia Facula, combines images obtained from altitudes as low as 22 miles (35 km) above Ceres' surface. The mosaic is overlain on a topography model based on images obtained during Dawn's low altitude mapping orbit (240 miles or 385 km altitude). No vertical exaggeration was applied. The center of Cerealia Facula is located at 19.7 degrees north latitude and 239.6 degrees south longitude. During its mission of over a decade, the Dawn spacecraft has studied the asteroid Vesta and dwarf planet Ceres, celestial bodies believed to have formed early in the history of the solar system. The mission's goal is to characterize the early solar system and the processes that dominated its formation. Image Credit: NASA.

One of Dawn’s biggest reveals on Ceres lay in the region of Ernutet Crater. Organic molecules were found in abundance. Organics are among the building blocks of life, though Dawn’s data can’t determine if Ceres’ organics were formed from biological processes.

“There is growing evidence that the organics in Ernutet came from Ceres’ interior, in which case they could have existed for some time in the early, interior ocean,” said Julie Castillo-Rogez, Dawn’s project scientist and deputy principal investigator at JPL.

Vibrant Vesta

At Vesta, Dawn mapped the craters of this planet-like world and revealed that its northern hemisphere had experienced more large impacts than expected, suggesting there were more large objects in the asteroid belt early on than scientists thought.

In 1996, the Hubble space telescope relayed images of a mountain at the center of an enormous Vesta basin now called Rheasilvia. Dawn’s mapping showed it to be twice the height of Mt. Everest, and it revealed canyons that rival the Grand Canyon in size.

Dawn also confirmed Vesta as the source of a very common family of meteorites.

Nearing the End

Dawn has continued to gather high-resolution images, gamma ray and neutron spectra, infrared spectra and gravity data at Ceres. Nearly once a day, it will swoop over Ceres about 22 miles (35 kilometers) from its surface -- only about three times the altitude of a passenger jet -- gathering valuable data until it expends the last of the hydrazine that feeds thrusters controlling its orientation.

Because Ceres has conditions of interest to scientists who study chemistry that leads to the development of life, NASA follows strict planetary protection protocols for the disposal of the Dawn spacecraft. Unlike Cassini, which deliberately plunged into Saturn’s atmosphere to protect the system from contamination -- Dawn will remain in orbit around Ceres, which has no atmosphere.

Engineers designed Dawn’s final orbit to ensure it will not crash for at least 20 years -- and likely decades longer.

Rayman, who led the team that flew Dawn throughout the mission and into its final orbit, likes to think of Dawn’s end this way: as “an inert, celestial monument to human creativity and ingenuity.”

More on Dawn’s mission legacy is here: https://dawn.jpl.nasa.gov/mission/toolkit/

The Dawn mission is managed by JPL for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. JPL is responsible for overall Dawn mission science. Northrop Grumman in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, Max Planck Institute for Solar System Research, Italian Space Agency and Italian National Astrophysical Institute are international partners on the mission team.

For a complete list of mission participants, visit: https://dawn.jpl.nasa.gov/mission

More information about Dawn is available at the following sites:

https://www.nasa.gov/dawn

https://dawn.jpl.nasa.gov

Images (mentioned), Video (mentioned), Text, Credits: NASA/Dwayne Brown/JoAnna Wendel​/Tony Greicius/JPL/Gretchen McCartney.

Greetings, Orbiter.ch