jeudi 7 février 2019

2018 Fourth Warmest Year in Continued Warming Trend, According to NASA, NOAA













NASA logo.

Feb. 7, 2019

Earth's global surface temperatures in 2018 were the fourth warmest since 1880, according to independent analyses by NASA and the National Oceanic and Atmospheric Administration (NOAA).

Global temperatures in 2018 were 1.5 degrees Fahrenheit (0.83 degrees Celsius) warmer than the 1951 to 1980 mean, according to scientists at NASA’s Goddard Institute for Space Studies (GISS) in New York. Globally, 2018's temperatures rank behind those of 2016, 2017 and 2015. The past five years are, collectively, the warmest years in the modern record.

“2018 is yet again an extremely warm year on top of a long-term global warming trend,” said GISS Director Gavin Schmidt.

Since the 1880s, the average global surface temperature has risen about 2 degrees Fahrenheit (1 degree Celsius). This warming has been driven in large part by increased emissions into the atmosphere of carbon dioxide and other greenhouse gases caused by human activities, according to Schmidt.

2018 Was the Fourth Hottest Year on Record

Video above: Earth’s long-term warming trend can be seen in this visualization of NASA’s global temperature record, which shows how the planet’s temperatures are changing over time, compared to a baseline average from 1951 to 1980. The record is shown as a running five-year average. Video Credits: NASA’s Scientific Visualization Studio/Kathryn Mersmann.

Weather dynamics often affect regional temperatures, so not every region on Earth experienced similar amounts of warming. NOAA found the 2018 annual mean temperature for the contiguous 48 United States was the 14th warmest on record.

Warming trends are strongest in the Arctic region, where 2018 saw the continued loss of sea ice. In addition, mass loss from the Greenland and Antarctic ice sheets continued to contribute to sea level rise. Increasing temperatures can also contribute to longer fire seasons and some extreme weather events, according to Schmidt.

“The impacts of long-term global warming are already being felt — in coastal flooding, heat waves, intense precipitation and ecosystem change,” said Schmidt.

NASA’s temperature analyses incorporate surface temperature measurements from 6,300 weather stations, ship- and buoy-based observations of sea surface temperatures, and temperature measurements from Antarctic research stations.


Animation above: This line plot shows yearly temperature anomalies from 1880 to 2018, with respect to the 1951-1980 mean, as recorded by NASA, NOAA, the Japan Meteorological Agency, the Berkeley Earth research group, and the Met Office Hadley Centre (UK). Though there are minor variations from year to year, all five temperature records show peaks and valleys in sync with each other. All show rapid warming in the past few decades, and all show the past decade has been the warmest. Animation Credits: NASA’s Earth Observatory.

These raw measurements are analyzed using an algorithm that considers the varied spacing of temperature stations around the globe and urban heat island effects that could skew the conclusions. These calculations produce the global average temperature deviations from the baseline period of 1951 to 1980.

Because weather station locations and measurement practices change over time, the interpretation of specific year-to-year global mean temperature differences has some uncertainties. Taking this into account, NASA estimates that 2018’s global mean change is accurate to within 0.1 degree Fahrenheit, with a 95 percent certainty level.


Image above: Earth’s long-term warming trend can be seen in this visualization of NASA’s global temperature record. NASA’s Scientific Visualization Studio/Kathryn Mersmann.

NOAA scientists used much of the same raw temperature data, but with a different baseline period and different interpolation into the Earth’s polar and other data poor regions. NOAA’s analysis found 2018 global temperatures were 1.42 degrees Fahrenheit (0.79 degrees Celsius) above the 20th century average.

NASA’s full 2018 surface temperature data set — and the complete methodology used to make the temperature calculation — are available at: https://data.giss.nasa.gov/gistemp

GISS is a laboratory within the Earth Sciences Division of NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The laboratory is affiliated with Columbia University’s Earth Institute and School of Engineering and Applied Science in New York.

NASA uses the unique vantage point of space to better understand Earth as an interconnected system. The agency also uses airborne and ground-based monitoring, and develops new ways to observe and study Earth with long-term data records and computer analysis tools to better see how our planet is changing. NASA shares this knowledge with the global community and works with institutions in the United States and around the world that contribute to understanding and protecting our home planet.

For more information about NASA’s Earth science missions, visit: https://www.nasa.gov/earth

The slides for the Feb. 6 news conference are available at:
https://www.nasa.gov/sites/default/files/atoms/files/noaa-nasa_global_analysis-2018-final_feb6.pdf

NOAA’s Global Report is available at: http://bit.ly/Global201812

Climate: https://www.nasa.gov/subject/3127/climate

Animation (mentioned), Image (mentioned), Video (mentioned), Text, Credits: NASA/Sean Potter/Steve Cole.

Greetings, Orbiter.ch

Bubbles of Brand New Stars













ESO - European Southern Observatory logo.

7 February 2019

Bubbles of Brand New Stars

This dazzling region of newly-forming stars in the Large Magellanic Cloud (LMC) was captured by the Multi Unit Spectroscopic Explorer instrument (MUSE) on ESO’s Very Large Telescope. The relatively small amount of dust in the LMC and MUSE’s acute vision allowed intricate details of the region to be picked out in visible light.

Jumbo Jets

This region of the Large Magellanic Cloud (LMC) glows in striking colours in this image captured by the Multi Unit Spectroscopic Explorer (MUSE) instrument on ESO’s Very Large Telescope (VLT). The region, known as LHA 120-N 180B — N180 B for short — is a type of nebula known as an H II region (pronounced “H two”), and is a fertile source of new stars.

Digitized Sky Survey image around the HII region LHA 120-N 180B

The LMC is a satellite galaxy of the Milky Way, visible mainly from the Southern Hemisphere. At only around 160 000 light-years away from the Earth, it is practically on our doorstep. As well as being close to home, the LMC’s single spiral arm appears nearly face-on, allowing us to inspect regions such as N180 B with ease.

H II regions are interstellar clouds of ionised hydrogen — the bare nuclei of hydrogen atoms. These regions are stellar nurseries — and the newly formed massive stars are responsible for the ionisation of the surrounding gas, which makes for a spectacular sight. N180 B’s distinctive shape is made up of a gargantuan bubble of ionised hydrogen surrounded by four smaller bubbles.

The HII region LHA 120-N 180B in the constellation Mensa

Deep within this glowing cloud, MUSE has spotted a jet emitted by a fledgling star — a massive young stellar object with a mass 12 times greater than our Sun. The jet — named Herbig–Haro 1177, or HH 1177 for short — is shown in detail in this accompanying image. This is the first time such a jet has been observed in visible light outside the Milky Way, as they are usually obscured by their dusty surroundings. However, the relatively dust-free environment of the LMC allows HH 1177 to be observed at visible wavelengths. At nearly 33 light-years in length, it is one of the longest such jets ever observed.

Jet Infographic

HH 1177 tells us about the early lives of stars. The beam is highly collimated; it barely spreads out as it travels. Jets like this are associated with the accretion discs of their star, and can shed light on how fledgling stars gather matter. Astronomers have found that both high- and low-mass stars launch collimated jets like HH 1177 via similar mechanisms — hinting that massive stars can form in the same way as their low-mass counterparts.

Zooming in on the HII Region LHA 120-N 180B

MUSE has recently been vastly improved by the addition of the Adaptive Optics Facility , the Wide Field Mode of which saw first light in 2017. Adaptive optics is the process by which ESO’s telescopes compensate for the blurring effects of the atmosphere — turning twinkling stars into sharp, high-resolution images. Since obtaining these data, the addition of the Narrow Field Mode, has given MUSE vision nearly as sharp as that of the NASA/ESA Hubble Space Telescope — giving it the potential to explore the Universe in greater detail than ever before.

Panning across N180

More information

This research was presented in a paper entitled “An optical parsec-scale jet from a massive young star in the Large Magellanic Cloud” which appeared in the journal Nature.

The research team was composed of A. F. McLeod (who conducted this research while at the University of Canterbury, New Zealand and is now affiliated with the Department of Astronomy, University of California, Berkeley, and the Department of Physics and Astronomy, Texas Tech University, USA), M. Reiter (Department of Astronomy, University of Michigan, Ann Arbor, USA), R. Kuiper (Institute of Astronomy and Astrophysics, University of Tübingen, Germany), P. D. Klaassen (UK Astronomy Technology Centre, Royal Observatory Edinburgh, UK) and C. J, Evans (UK Astronomy Technology Centre, Royal Observatory Edinburgh, UK).

ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory by far. It has 16 Member States: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Ireland, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile and with Australia as a Strategic Partner. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope and its world-leading Very Large Telescope Interferometer as well as two survey telescopes, VISTA working in the infrared and the visible-light VLT Survey Telescope. ESO is also a major partner in two facilities on Chajnantor, APEX and ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre Extremely Large Telescope, the ELT, which will become “the world’s biggest eye on the sky”

Links:

ESOcast 193 Light: Bubbles of Brand New Stars: https://www.eso.org/public/videos/eso1903a/

Link to the research paper: https://www.nature.com/articles/nature25189

More information on MUSE: https://www.eso.org/public/teles-instr/paranal-observatory/vlt/vlt-instr/muse/

More information on the VLT: https://www.eso.org/public/teles-instr/paranal-observatory/vlt/

Adaptive Optics Facility: https://www.eso.org/public/teles-instr/technology/adaptive_optics/

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

Images, Text, Credits: ESO/Calum Turner/Texas Tech University & University of California Berkeley/A McLeod et al./Digitized Sky Survey 2. Acknowledgment: Davide De Martin/IAU and Sky & Telescope/Videos: ESO/Digitized Sky Survey 2/N. Risinger (skysurvey.org). Music: Astral Electronic.

Greetings, Orbiter.ch

ESA’s Mars rover has a name – Rosalind Franklin









ESA - ExoMars Mission logo.

7 February 2019

The ExoMars rover that will search for the building blocks of life on the Red Planet has a name: Rosalind Franklin. The prominent scientist behind the discovery of the structure of DNA will have her symbolic footprint on Mars in 2021. 

A panel of experts chose ‘Rosalind Franklin’ from over 36 000 entries submitted by citizens from all ESA Member States, following a competition launched by the UK Space Agency in July last year.

ExoMars rover

The ExoMars rover will be the first of its kind to combine the capability to roam around Mars and to study it at depth. The Red Planet has hosted water in the past, but has a dry surface exposed to harsh radiation today.

The rover bearing Rosalind Franklin’s name will drill down to two metres into the surface to sample the soil, analyse its composition and search for evidence of past – and perhaps even present – life buried underground.

The rover is part of the ExoMars programme, a joint endeavour between ESA and the Russian State Space Corporation, Roscosmos.

What’s in a name?

Rosalind Elsie Franklin was a British chemist and X-ray crystallographer who contributed to unravelling the double helix structure of our DNA. She also made enduring contributions to the study of coal, carbon and graphite. ESA has a long tradition of naming its missions for great scientists, including Newton, Planck and Euclid.

Rosalind Franklin

“This name reminds us that it is in the human genes to explore. Science is in our DNA, and in everything we do at ESA. Rosalind the rover captures this spirit and carries us all to the forefront of space exploration,” says ESA Director General Jan Woerner.

The name was revealed this morning in the ‘Mars Yard’ at Airbus Defence and Space in Stevenage, in the United Kingdom, where the rover is being built. ESA astronaut Tim Peake met the competition entrants who chose the winning name, and toured the facility with UK Science Minister Chris Skidmore.

“This rover will scout the martian surface equipped with next-generation instruments – a fully-fledged automated laboratory on Mars,” says Tim.

ExoMars rover name announced

“With it, we are building on our European heritage in robotic exploration, and at the same time devising new technologies.”

The rover will relay data to Earth through the Trace Gas Orbiter, a spacecraft searching for tiny amounts of gases in the martian atmosphere that might be linked to biological or geological activity since 2016.

Rosalind has already a proposed landing site. Last November a group of experts chose Oxia Planum near the martian equator to explore an ancient environment that was once water-rich and that could have been colonised by primitive life.

On our way to Mars, and back

Looking beyond ExoMars, bringing samples back from Mars is the logical next step for robotic exploration. ESA is already defining a concept for a sample return mission working in cooperation with NASA.

“Returning martian samples is a huge challenge that will require multiple missions, each one successively more complex than the one before,” says David Parker, ESA’s Director of Human and Robotic Exploration.

ExoMars Rover: from concept to reality

“We want to bring the Red Planet closer to home. We want to delve into its mysteries and bring back knowledge and benefits to people on Earth. Returned planetary samples are truly the gift that keeps on giving – scientific treasure for generations to come,” he adds.

Long-term planning is crucial to realise the missions that investigate fundamental science questions like could life ever have evolved beyond Earth?

ESA has been exploring Mars for more than 15 years, starting with Mars Express and continuing with the two ExoMars missions, keeping a European presence at the Red Planet into the next decade.

Related links:

ExoMars: http://www.esa.int/Our_Activities/Human_and_Robotic_Exploration/Exploration/ExoMars

Robotic exploration of Mars: http://exploration.esa.int/

ESA Member States: https://www.esa.int/About_Us/Welcome_to_ESA/New_Member_States

Mars Express: http://www.esa.int/Our_Activities/Space_Science/Mars_Express

Sample return mission: http://www.esa.int/Our_Activities/Human_and_Robotic_Exploration/Exploration/ESA_and_NASA_to_investigate_bringing_martian_soil_to_Earth

Images, Video, Text, Credits: ESA/S. Corvaja/ATG medialab/MRC Laboratory of Molecular Biology.

Best regards, Orbiter.ch

mercredi 6 février 2019

Transforming LHCb: What’s in store for the next two years?













CERN - European Organization for Nuclear Research logo.

6 February, 2019

The LHCb detector will undergo a metamorphosis during CERN’s second long shutdown (LS2) 

Opening of the LHCb detector in early December 2018 (Image: Maximilien Brice/CERN)

The LHCb experiment will undergo a metamorphosis over the coming two years, during CERN’s maintenance and upgrade period known as Long Shutdown 2 (LS2). When the Large Hadron Collider (LHC) restarts in 2021, the proton–proton collision rate at LHCb will be increased by a factor of five, and the collaboration is upgrading its detector to be ready for it.

The LHCb experiment is trying to solve the mystery of why nature prefers matter over antimatter: small asymmetries between the two could explain why matter emerged from the aftermath of the Big Bang while antimatter did not. In particular, LHCb is hunting for beauty or bottom (b) quarks, which were common at the infancy of the Universe and can be generated in their billions by the LHC, along with their antimatter counterparts, beauty antiquarks.

Forty is better than one

As every second of the LHC corresponds to several million proton–proton collisions, a detector’s trigger system needs to decide which data are important to keep and which can be discarded.

Within the LHC, bunches of protons travel in two beams, clockwise and anticlockwise, at almost the speed of light. The beams cross one another in a detector every 25 nanoseconds, corresponding to a frequency of 40 MHz (40 million times per second). In previous years, LHCb filtered down this “event rate” to 1 MHz, using fast electronics to select the most interesting events. Those events were then processed and sifted further. But from 2021 onwards, this will change radically: the whole detector will read at the full rate of 40 MHz to allow event selection to be done more precisely and flexibly by the software. For this reason, the electronics of essentially all the subdetectors will be modified and the computing power of the LHCb event selection system (trigger) will become more powerful.

Flowing at an immense rate of 4 terabytes per second, data will travel from the underground hall, straight from the detector electronics, via some 9000 300-metre-long optical fibres, into a new computer centre that is nearing completion. There, around 500 powerful custom-made boards will receive and transfer data to thousands of processing cores.

Highlights of the many LHCb upgrades taking place during LS2

A faster VELO

The vertex locator (VELO) – the subdetector that measures the distance between the collision point and the point where B hadrons (composite particles containing at least one b quark or antiquark) transform into other particles – is one of the key components being upgraded during LS2. The new VELO consists of pixel tracking layers, which offer improved hit resolution and simpler track reconstruction. It will also be closer to the beam axis: 5.1 mm as opposed to 8.4 mm. A new chip, the VELOPIX, capable of collecting signal hits from 256×256 pixels and sending data at a staggering rate of up to 20 Gb/s, was developed for this purpose.


Image above: Prototype vertex locator (VELO) pixel modules were developed last year ahead of the upgrade (Image: Julien Marius Ordan/CERN).

Mirror, mirror on the detector

The ring-imaging Cherenkov (RICH) detectors, which determine particles’ identities, will be equipped with a new mirror system. This is required to deflect, focus and detect cones of light emitted by travelling particles in an environment with much larger particle densities.

New silicon-microstrip sensors and SciFi tracking

Currently, the main tracking system reconstructs the path of charged particles in four tracking stations: one between RICH-1 and the LHCb dipole magnet, and three between the magnet and RICH-2. In the future, a new upstream tracker (UT) with innovative silicon-microstrip sensors will be installed in place of the station before the magnet. The three tracking stations after the magnet will be replaced by a new type of station based on scintillating fibres (SciFi), read out at one extremity by silicon photomultiplier (SiPM) arrays.

The SciFi tracker represents a major challenge for the collaboration, not only due to its complexity, but also because the technology has never been used for such a large area in such a radiation environment. Scientists ordered more than 11 000 km of fibre, which they meticulously verified and even cured of a few rare and local imperfections.


Image above: Removing the beam pipe of the LHCb experiment in early January 2019 (Image: Julien Marius Ordan/CERN).

With the planned higher luminosity and a greatly improved ability to pick the most interesting events, the transformed LHCb can look forward to unprecedented results in the future.

Read more in “LHCb’s momentous metamorphosis” in the latest CERN Courier, which also has LS2 highlights from ALICE, ATLAS and CMS: https://cerncourier.com/lhcbs-momentous-metamorphosis/

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:

LHCb experiment: https://home.cern/science/experiments/lhcb

Long Shutdown 2 (LS2): https://home.cern/tags/long-shutdown-2

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

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

Images (mentioned), Text, Credits: CERN, by Letizia Diamante.

Best regards, Orbiter.ch

Mind and Body Studies as Crew Finalizes Cygnus Packing













ISS - Expedition 58 Mission patch.

February 6, 2019

The astronauts onboard the International Space Station continued exploring today how living in space affects their minds and bodies. The Expedition 58 crew also researched fluid physics and prepared a resupply ship for its departure.

Anne McClain of NASA collected blood and urine samples this morning for the Repository physiology study. She spun the samples in a centrifuge then stowed them in a science freezer. She later took a cognition test in support of the Lighting Effects experiment that seeks to improve health and wellness.


Image above: Astronaut Anne McClain of NASA peers into a microscope and takes photographs for the Protein Crystal Growth-16 experiment that is exploring therapies for Parkinson’s disease. Image Credit: NASA.

Canadian Space Agency astronaut David Saint-Jacques along with McClain answered a pair of questionnaires in support of the Standard Measures and Behavioral Core Measures psychology studies. He also wrapped up a physics study observing the mechanics of fluids in hardware that represents a spacecraft fuel tank.

International Space Station (ISS). Animation Credit: NASA

McClain will be in the cupola Friday at 11:10 a.m. EST and release the U.S. Cygnus resupply ship from the Canadarm2 robotic arm. Saint-Jacques will back her up Friday and monitor the cargo vessel’s departure. The duo is finalizing packing, will install a small satellite deployer in Cygnus then close the hatches on Thursday.

Over in the station’s Russian segment, Commander Oleg Kononenko of Roscosmos worked on power supply and battery maintenance in the Zarya module. The long-serving cosmonaut also researched crew psychology and studied radiation exposure.

Related links:

Expedition 58: https://www.nasa.gov/mission_pages/station/expeditions/expedition58/index.html

Repository: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=954

Lighting Effects: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=2013

Standard Measures: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7711

Behavioral Core Measures: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7537

Mechanics of fluids: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=2043

Cupola: https://www.nasa.gov/mission_pages/station/structure/elements/cupola.html

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

Small satellite deployer: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=7847

Zarya module: https://www.nasa.gov/mission_pages/station/structure/elements/zarya-cargo-module

Radiation exposure: https://go.nasa.gov/2GcuT1J

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

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

Greetings, Orbiter.ch

Magnetic North rushes from Canada to Siberia













NOAA - National Oceanic and Atmospheric Administration logo.

February 6, 2019

An urgent update of the global magnetic model, essential for many navigation systems, was released this week.


Image above: very cool interactive tool for the current magnetic recession and historic location of the north magnetic pole.

Geographic North is not Magnetic North. The latter is currently traveling at a speed of 55 km per year. This discovery forced scientists to publish this week a new magnetic model, essential to many navigation systems.

The global magnetic model is used for aerial and naval navigation of armies, but also by phone compasses. It is updated every five years, but the latest model, dating back to 2015, was out of step with the observations made at the end of 2018.

NCEI has released an out-of-cycle World Magnetic Model to ensure safe navigation

The Earth's magnetic field is generated mainly by the movement of the liquid iron that makes up the majority of the Earth's core, 3000 km below the surface. This is what makes the magnetic poles derive. The model makes it possible to correct the direction indicated by the compass in order to find the geographic North, which is fixed. The discovery of magnetic north in northern Canada dates back to 1831.

From 15 km per year to 55 km per year

Scientists from US and British atmospheric agencies (NOAA and BGS) released an urgent update of the model on Monday, before a normal update in late 2019.

Concretely, if one compared the direction indicated by the needle of a compass of France between today and two centuries ago, there would be a difference of about twenty degrees, explains to AFP Arnaud Chulliat, geophysicist at the University of Colorado at Boulder and NOAA.

Position of the north magnetic pole since 1590

"It's a very slow movement, but it's very real. Over several decades, this can reach several degrees, "he says. This shift does not matter much in the most populated latitudes, but "near the magnetic pole, change is faster".

Magnetic North has, over the centuries, moved more or less unpredictably into the archipelagos of Canada's far north. Since the end of the 19th century, he has been heading for Siberia. Since the 1990s, the movement has accelerated, across the Arctic Ocean, from about 15 km/year (9.32 miles/year) to 55 km/year (34.17 miles/year) today.

NOAA / NCEI: World Magnetic Model Out-of-Cycle Release:
https://www.ncei.noaa.gov/news/world-magnetic-model-out-cycle-release

NOAA - National Centers for Environmental Information: https://www.ncei.noaa.gov/

Images, Text, Credits: ATS/NOAA/NCEI/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

Beyond Mars, the Mini MarCO Spacecraft Fall Silent













NASA - MarCO Mission patch.

February 6, 2019

Before the pair of briefcase-sized spacecraft known collectively as MarCO launched last year, their success was measured by survival: If they were able to operate in deep space at all, they would be pushing the limits of experimental technology.

Now well past Mars, the daring twins seem to have reached their limit. It's been over a month since engineers have heard from MarCO, which followed NASA's InSight to the Red Planet. At this time, the mission team considers it unlikely they'll be heard from again.


Animation above: MarCO-B, one of the experimental Mars Cube One (MarCO) CubeSats, took these images as it approached Mars. Animation Credits: NASA/JPL-Caltech.

MarCO, short for Mars Cube One, was the first interplanetary mission to use a class of mini-spacecraft called CubeSats. The MarCOs - nicknamed EVE and WALL-E, after characters from a Pixar film - served as communications relays during InSight's landing, beaming back data at each stage of its descent to the Martian surface in near-real time, along with InSight's first image. WALL-E sent back stunning images of Mars as well, while EVE performed some simple radio science.

All of this was achieved with experimental technology that cost a fraction of what most space missions do: $18.5 million provided by NASA's Jet Propulsion Laboratory in Pasadena, California, which built the CubeSats.

WALL-E was last heard from on Dec. 29; EVE, on Jan. 4. Based on trajectory calculations, WALL-E is currently more than 1 million miles (1.6 million kilometers) past Mars; EVE is farther, almost 2 million miles (3.2 million kilometers) past Mars.


Image above: Engineer Joel Steinkraus uses sunlight to test the solar arrays on one of the Mars Cube One (MarCO) spacecraft at NASA's Jet Propulsion Laboratory. Image Credits: NASA/JPL-Caltech.

The mission team has several theories for why they haven't been able to contact the pair. WALL-E has a leaky thruster. Attitude-control issues could be causing them to wobble and lose the ability to send and receive commands. The brightness sensors that allow the CubeSats to stay pointed at the Sun and recharge their batteries could be another factor. The MarCOs are in orbit around the Sun and will only get farther away as February wears on. The farther they are, the more precisely they need to point their antennas to communicate with Earth.

The MarCOs won't start moving toward the Sun again until this summer. The team will reattempt to contact the CubeSats at that time, though it's anyone's guess whether their batteries and other parts will last that long.

Even if they're never revived, the team considers MarCO a spectacular success.

"This mission was always about pushing the limits of miniaturized technology and seeing just how far it could take us," said Andy Klesh, the mission's chief engineer at JPL. "We've put a stake in the ground. Future CubeSats might go even farther."


Image above: An artist's rendering of the twin Mars Cube One (MarCO) spacecraft Cruise in Deep Space. Image Credits: NASA/JPL-Caltech.

A number of the critical spare parts for each MarCO will be used in other CubeSat missions. That includes their experimental radios, antennas and propulsion systems. Several of these systems were provided by commercial vendors, making it easier for other CubeSats to use them as well.

More small spacecraft are on the way. NASA is set to launch a variety of new CubeSats in coming years.

"There's big potential in these small packages," said John Baker, the MarCO program manager at JPL. "CubeSats - part of a larger group of spacecraft called SmallSats - are a new platform for space exploration that is affordable to more than just government agencies."

Related article & links:

NASA Hears MarCO CubeSats Loud and Clear from Mars
https://orbiterchspacenews.blogspot.com/2018/11/nasa-hears-marco-cubesats-loud-and.html

CubeSats: https://solarsystem.nasa.gov/news/834/10-things-cubesats-going-farther/

For more information, visit: https://www.jpl.nasa.gov/cubesat/missions/marco.php

Image (mentioned), Animation (mentioned), Text, Credits: NASA/JoAnna Wendel/JPL/Andrew Good.

Greetings, Orbiter.ch