vendredi 2 février 2018

CASC Long March 2D Launches CSES & MicroSatellites













CASC - China Seismo-Electromagnetic Satellite patch.


February 2, 2018

Long March 2D Launches CSES & MicroSatellites. Image Credit: CASC

China launched a Long March 2D rocket from the Jiuquan Satellite Launch Center on Friday, carrying a group of seven satellites from China, Italy, Argentina and Denmark including an innovative experiment to study the ionospheric precursors of Earthquakes to evaluate whether forecasting of strong Earthquakes will be possible from an orbital vantage point.

Friday’s launch occurred at 7:51 UTC from Jiuquan’s Launch Complex 43 and the two-stage rocket was headed to the south west toward a 500-Kilometer orbit from where its payloads will operate. Chinese state media declared the launch successful not long after the vehicle achieved orbit and the first payload teams confirmed signals from their satellites were being received.

Long March-2D launches China Seismo-Electromagnetic Satellite

Friday’s launch placed into orbit the China Seismo-Electromagnetic Satellite (CSES) “Zhangheng-1”, the next two satellites of the commercial Aleph-1 imaging constellation operated by Satellogic, the GOMX 4A and 4B duo experimenting with inter-satellite communications & stationkeeping, and the Chinese FengMaNiu 1 and Shaonian Xing CubeSats completing technology demonstration and outreach missions via amateur radio equipment.

Seismo-Electromagnetic Satellite (CSES). Image Credit: CAST

Zhangheng-1 is a 730-Kilogram, multi-instrument satellite named after Han Dynasty scholar Zhang Heng, setting out to complete a comprehensive study of the ionospheric precursors of Earthquakes using particle, magnetic & electric field and plasma sensors. The satellite, baselined for a five-year science mission, is based on the CAST2000 satellite platform and was developed by the China National Space Administration (CNSA), the China Earthquake Administration and the Italian Space Agency (ASI) which provided the High-Energy Particle Detector instrument.

The reliable prediction of Earthquakes brings the potential of saving hundreds if not thousands of lives every year, but so far only came with false starts and methodology based on flawed science. However, promising leads have been found in data from orbiting satellites that showed Earth’s crust may be giving hints before large tremors in the form of electromagnetic anomalies that will then percolate through Earth’s ionosphere up to altitudes of several hundred Kilometers where they can be detected between a few minutes to a few days before an Earthquake.

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

Images (mentioned), Video, Text, Credits: CASC/SpaceFlight101.com/SciNews.

Greetings, Orbiter.ch

Hubble’s Majestic Spiral in Pegasus











NASA - Hubble Space Telescope patch.

Feb. 2, 2018


This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (the Winged Horse). Facing us partially edge-on, the galaxy showcases its beautiful arms, which swirl like a whirlpool around its bright central region.

Astronomers took this image using Hubble’s Wide Field Camera 3 (WFC3), as they were observing an extraordinary exploding star — a supernova — near the galaxy’s central yellow core. Named SN 2014C, it rapidly evolved from a supernova containing very little hydrogen to one that is hydrogen-rich — in just one year. This rarely observed metamorphosis was luminous at high energies and provides unique insight into the poorly understood final phases of massive stars.

NGC 7331 is similar in size, shape and mass to the Milky Way. It also has a comparable star formation rate, hosts a similar number of stars, has a central supermassive black hole and comparable spiral arms. The primary difference between this galaxy and our own is that NGC 7331 is an unbarred spiral galaxy — it lacks a “bar” of stars, gas and dust cutting through its nucleus, as we see in the Milky Way. Its central bulge also displays a quirky and unusual rotation pattern, spinning in the opposite direction to the galactic disk itself.

Hubble Space Telescope (HST)

By studying similar galaxies we hold a scientific mirror up to our own, allowing us to build a better understanding of our galactic environment, which we cannot always observe, and of galactic behavior and evolution as a whole.

For more information about Hubble, visit:

http://hubblesite.org/
http://www.nasa.gov/hubble
http://www.spacetelescope.org/

Image, Animation, Credits: ESA/Hubble & NASA/D. Milisavljevic (Purdue University)/Text: European Space Agency/NASA/Karl Hille.

Best regards, Orbiter.ch

NASA’s Newly Rediscovered IMAGE Mission Provided Key Aurora Research












NASA - Magnetospheric Multiscale Satellites (MMS) patch.

Feb. 2, 2018

On Jan. 20, 2018, amateur astronomer Scott Tilley detected an unexpected signal coming from what he later postulated was NASA’s long-lost IMAGE satellite, which had not been in contact since 2005. On Jan. 30, NASA — along with help from a community of IMAGE scientists and engineers — confirmed that the signal was indeed from the IMAGE spacecraft. Whatever the next steps for IMAGE may be, the mission’s nearly six years in operation provided robust research about the space around Earth that continue to guide science to this day.

On March 25, 2000, NASA launched the Imager for Magnetopause-to-Aurora Global Exploration, or IMAGE, mission. It was the first mission to use neutral atom, photon and radio imaging techniques to produce large-scale, simultaneous measurements of the charged particles that exist in near-Earth space — namely in our magnetosphere, the magnetic fields that surround our planet, and its inner bubble of cold material called the plasmasphere.


Image above: IMAGE spacecraft is tested prior to its March 2000 launch. Image Credit: NASA.

“IMAGE was a discovery machine and a seminal mission that gave us a broader perspective on Earth’s environment and its ever-changing magnetosphere,” said Jim Green, director of planetary science at NASA Headquarters in Washington, who worked as a co-investigator and deputy project scientist for IMAGE. “Much of my career as a magnetospheric physicist was with IMAGE, and the science was transformative.”

Originally designed as a two-year mission, IMAGE was approved twice to continue its operations. But when the spacecraft unexpectedly failed to make contact on a routine pass on Dec.18, 2005, its promising tenure seemed to be cut short.

Investigations into possible causes of failure suggested that the transmitter controller power source was tripped, possibly by an incoming high-energy cosmic ray or radiation belt particle. It was hypothesized that passing through a dramatic change in energy — such as what happens when a spacecraft experiences total darkness during an eclipse — could potentially reset the spacecraft. But after a 2007 eclipse failed to induce a reboot, the mission was declared over.

What was the IMAGE mission?

Before that, however, IMAGE was a powerhouse. The data collected during its nearly five years of operation led to some 40 new discoveries about Earth’s magnetosphere and plasmasphere. Many of these discoveries had their basis in energetic neutral atom, or ENA, imaging, a novel technique pioneered by IMAGE to render the invisible visible.

The technique makes use of some fundamental space physics. Particles with an electric charge — like the ions that make up much of the plasma in the magnetosphere — are bound to Earth’s magnetic field lines, spinning around them like a yo-yo on a string. But when they crash into neutral particles, the charged particles can steal the neutral’s electrons in a process called charge exchange, becoming neutral themselves.

No longer magnetically bound, these energetic neutral atoms barrel off into space in whatever direction they were heading when the collision occurred. ENA instruments capture these neutral atoms and use them to build up large scale images of the surrounding plasma, similar to how ordinary cameras capture light rays to create pictures.


Image above: Earth's plasmasphere and plume as measured by IMAGE’s Extreme Ultraviolet Imager. Image Credits: Sandel, B. R., et al., Space Sci. Rev., 109, 25, 2003.

In combination with ENA instruments, IMAGE also used ultraviolet and radio imaging techniques that together led to many of IMAGE’s most notable accomplishments. Among them is the confirmation of the plasmaspheric plume, a region of plasma particles that flow backwards toward the Sun on Earth’s dayside. Such a backflow had been predicted by models, but never directly observed by spacecraft.

“It’s as if you’re driving in a convertible,” said Thomas Moore, the mission scientist for IMAGE, as well as the lead for the spacecraft’s Low Energy Neutral Atom (LENA) Imager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “The air is rushing against the car in one direction, but your hair will blow towards the windshield.”

IMAGE produced large-scale images every two minutes. The rapid cadence of imaging allowed scientists to knit the images together to create frame-by-frame movies that could show the vast scale of charged particle interactions in near-Earth space, including those that cause the aurora.


Animation above: IMAGE captured the South Pole aurora caused by a coronal mass ejection in the fall of 2003. Animation Credits: NASA’s Goddard Space Flight Center Scientific Visualization Studio/Tom Bridgman, lead animator.

The missions that had flown before IMAGE had only been able to gather measurements at a single point in time and space — catching the particles the spacecraft happened to fly through at the time, rather than capturing a wide panoramic view. But such point measurements are challenging to interpret.

“The trouble with a single point measurement is you’re always moving around and you’re never quite sure if the variation that you see is because you’ve moved to a different place or because something has changed globally in the system,” Moore said. “I used to liken space physics before IMAGE to trying to study severe storms by driving around with a rain gauge out your window.”

IMAGE drastically changed the playing field. “We suddenly had a camera that could see the whole system,” Moore added.


Image above: An oblique view of the plasmasphere, reconstructed from IMAGE data. Image Credits: NASA’s Goddard Space Flight Center Scientific Visualization Studio/Tom Bridgman, lead animator.

But IMAGE didn’t just make pretty pictures: It was also the first space science mission to formally include an education and public outreach program (POETRY) as part of its proposal to NASA, specifically setting aside a budget for such activities. Partnering with elementary, middle and high school teachers, IMAGE’s science findings were incorporated into lessons and classroom activities: https://image.gsfc.nasa.gov/poetry/activities.html

While IMAGE’s future continues to unfold, its legacy has already proven its worth: The information it gleaned with its wide-range view provides an important complement to missions looking at smaller scales of the magnetosphere, including the highly successful Magnetospheric Multiscale mission, or MMS, launched in March 2015 and currently in orbit.

NASA's Latest Updates on Contacting IMAGE

New data regarding IMAGE provides some additional — though not yet complete — information on how the spacecraft began to transmit signals again.

Read more: https://www.nasa.gov/feature/goddard/2018/nasa-image-confirmed

Related:

IMAGE mission homepage: https://image.gsfc.nasa.gov/

Magnetospheric Multiscale mission (MMS): https://mms.gsfc.nasa.gov/

Images (mentioned), Animation (mentioned), Text, Credits: NASA/Rob Garner/Goddard Space Flight Center, by Miles Hatfield.

Greetings, Orbiter.ch

Stellar winds behaving unexpectedly












ESA - XMM-Newton Mission patch.

2 February 2018

ESA’s XMM-Newton has spotted surprising changes in the powerful streams of gas from two massive stars, suggesting that colliding stellar winds don’t behave as expected.

Massive stars – several times larger than our Sun – lead turbulent lives, burning their nuclear fuel rapidly and pouring large amounts of material into their surroundings throughout their short but sparkling lives.

Stellar wind evolution

These fierce stellar winds can carry the equivalent of Earth’s mass in a month and travel at millions of kilometres per hour, so when two such winds collide they unleash enormous amounts of energy.

The cosmic clash heats the gas to millions of degrees, making it shine brightly in X-rays.

Normally, colliding winds change little because neither do the stars nor their orbits. However, some massive stars behave dramatically.

This is the case with HD 5980, a pairing of two huge stars each 60 times the mass of our Sun and only about 100 million kilometres apart – closer than we are to our star.

 One had a major outburst in 1994, reminiscent of the eruption that turned Eta Carinae into the second brightest star in the sky for about 18 years in the 19th century.

HD 5980 in the star-forming region NGC 346

While it is now too late to study Eta Carinae’s historic eruption, astronomers have been observing HD 5980 with X-ray telescopes to study the hot gas.

In 2007, Yaël Nazé of the University of Liège, Belgium, and her colleagues discovered the collision of winds from these stars using observations made by ESA’s XMM-Newton and NASA’s Chandra X-ray telescopes between 2000 and 2005.

Then they looked at it again with XMM-Newton in 2016.

“We expected HD 5980 to fade gently over the years as the erupting star settled back to normal – but to our surprise it did just the opposite,” says Yaël.

They found the pair was two and a half times brighter than a decade earlier, and its X-ray emission was even more energetic.

“We had never seen anything like that in a wind–wind collision.”

Deciphering Eta Carinae’s eruptive twin

With less material ejected but more light emitted, it was difficult to explain what was happening.

Finally, they found a theoretical study that offers a fitting scenario.

“When stellar winds collide, the shocked material releases plenty of X-rays. However, if the hot matter radiates too much light, it rapidly cools, the shock becomes unstable and the X-ray emission dims.

“This somewhat counterintuitive process is what we thought happened at the time of our first observations, more than 10 years ago. But by 2016, the shock had relaxed and the instabilities had diminished, allowing the X-ray emission to rise eventually.”

XMM-Newton spacecraft

These are the first observations that substantiate this previously hypothetical scenario. Yaël’s colleagues are now testing the new result in greater detail through computer simulations.

“Unique discoveries like this demonstrate how XMM-Newton keeps providing astronomers with fresh material to improve our understanding of the most energetic processes in the Universe,” says Norbert Schartel, XMM-Newton project scientist at ESA.

Notes for Editors:

The paper “A changing wind collision,” by Y. Nazé et al. is published in the Astrophysical Journal: http://iopscience.iop.org/article/10.3847/1538-4357/aaa29c/meta

Theoretical study: https://academic.oup.com/mnras/article/438/4/3557/1111976

XMM-Newton: http://sci.esa.int/xmm-newton/

XMM-Newton overview: http://www.esa.int/Our_Activities/Space_Science/XMM-Newton_overview

XMM-Newton image gallery: http://xmm.esac.esa.int/external/xmm_science/gallery/public/index.php

XMM-Newton in-depth: http://sci.esa.int/science-e/www/area/index.cfm?fareaid=23

Animation, Images, Text, Credits: ESA/Markus Bauer/Norbert Schartel/Université de Liège/Yaël Nazé/ESA/XMM-Newton; Y. Nazé et al. 2018/NASA, ESA, A. Nota (STScI/ESA).

Best regards, Orbiter.ch

jeudi 1 février 2018

Cosmonauts Complete Spacewalk Preps, More Eye Checks for Rest of Crew









ISS - Expedition 54 Mission patch.

February 1, 2018

A pair of cosmonauts have wrapped up preparations for Friday morning’s spacewalk to work on the Russian segment of the International Space Station. The other four Expedition 54 crew members continued more eye exams throughout the day on Thursday.

Commander Alexander Misurkin and Flight Engineer Anton Shkaplerov completed a spacewalk procedures review today, finished collecting tools and readied their Orlan spacesuits. The veteran cosmonauts will exit the Pirs airlock around 10:30 a.m. EST Friday for 6.5 hour spacewalk. NASA TV begins its live coverage of the second spacewalk of the year at 9:45 a.m.


Image above: The International Space Station orbits above the Falkland Islands off the coast of the southern-most portion of Argentina on the continent of South America. In the upper-right of the photograph is the docked Progress 68 cargo craft. Image Credit: NASA.

The duo will work outside the Zvezda service module to swap out a high gain communications antenna electronics system. If time permits the spacewalkers may also retrieve experiments, photograph the back of Zvezda, reposition a foot restraint and jettison old experiment gear.

The rest of the crew continued working with doctors in real time on the ground today to get a look at their eyes and understand how microgravity affects vision. Astronauts Mark Vande Hei, Scott Tingle and Joe Acaba participated in eye scans using an ultrasound device this morning. Tingle then partnered up with Japanese astronaut Norishige Kanai.

Related links:

NASA TV: https://www.nasa.gov/multimedia/nasatv/index.html

Expedition 54: https://www.nasa.gov/mission_pages/station/expeditions/expedition54/index.html

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), Text, Credits: NASA/Mark Garcia.

Best regards, Orbiter.ch

NASA Twins Study Confirms Preliminary Findings












ISS - The Twins Study patch.

Feb. 1, 2018

The Twin Study propelled NASA into the genomics era of space travel. It was a ground-breaking study comparing what happened to astronaut Scott Kelly, in space, to his identical twin brother, Mark, who remained on Earth. The perfect nature versus nurture study was born.

The Twins Study brought ten research teams from around the country together to accomplish one goal: discover what happens to the human body after spending one year in space. NASA has a grasp on what happens to the body after the standard-duration six-month missions aboard the International Space Station, but Scott Kelly’s one-year mission is a stepping stone to a three-year mission to Mars.


Image above: Identical twin astronauts, Scott and Mark Kelly, are subjects of NASA’s Twins Study. Scott (right) spent a year in space while Mark (left) stayed on Earth as a control subject. Researchers looked at the effects of space travel on the human body. Credit: NASA. Image Credit: NASA.

If the results of the Twins Study are like a play, Act 1 began at NASA’s Human Research Program (HRP) 2017 Investigators’ Workshop (IWS), where the ten teams presented their preliminary findings. Reports included data on what happened to Scott Kelly, physiologically and psychologically, while he was in space, and compared the data to Mark Kelly, as a control subject on Earth. The 2018 IWS is Act 2, where findings from 2017 were corroborated, with some additions. Researchers also presented what happened to Scott after he returned to Earth, again while making comparisons to Mark. Act 3 will be debuted later in 2018 when an integrated summary publication is expected to be released.

By measuring large numbers of metabolites, cytokines, and proteins, researchers learned that spaceflight is associated with oxygen deprivation stress, increased inflammation, and dramatic nutrient shifts that affect gene expression.

After returning to Earth, Scott started the process of readapting to Earth’s gravity. Most of the biological changes he experienced in space quickly returned to nearly his preflight status. Some changes returned to baseline within hours or days of landing, while a few persisted after six months.

Scott’s telomeres (endcaps of chromosomes that shorten as one ages) actually became significantly longer in space. While this finding was presented in 2017, the team verified this unexpected change with multiple assays and genomics testing. Additionally, a new finding is that the majority of those telomeres shortened within two days of Scott’s return to Earth.


Image above: The Twins Study Investigators came from around the country to meet and share their final research results at the annual Human Research Program Investigators’ Workshop held in Galveston, Texas. Image Credit: NASA.

Another interesting finding concerned what some call the “space gene”, which was alluded to in 2017. Researchers now know that 93% of Scott’s genes returned to normal after landing. However, the remaining 7% point to possible longer term changes in genes related to his immune system, DNA repair, bone formation networks, hypoxia, and hypercapnia.

Increasing mission duration from the typical six-month ISS mission to one year resulted in no significant decreases in Scott’s cognitive performance while inflight and relative to his twin brother Mark on the ground. However, a more pronounced decrease in speed and accuracy was reported postflight, possibly due to re-exposure and adjustment to Earth’s gravity, and the busy schedule that enveloped Scott after his mission.

For additional detail on preliminary findings, visit NASA Twins Study Investigators to Release Integrated Paper in 2018. All of these findings are being integrated and summarized by the research teams; researchers are also evaluating the possible impact that these findings will have on future space travel beyond low Earth orbit. The next step for Twins Study investigators is Act 3, as referenced above. An integrated summary paper will be published later this year. A series of smaller papers grouped by related research areas will also be released.


Image above: Graphic illustration of the path the individual Twins Study research takes from research to integration to one summary paper to several companion papers. Image Credit: NASA.

The Twins Study has benefited NASA by providing the first application of genomics to evaluate potential risks to the human body in space. The NASA Twins Study also presented a unique opportunity for investigators to collaborate, participating in a team approach to HRP research.

Observations guide development of future hypotheses. Research from the landmark Twins Study will inform NASA’s Human Research Program studies for years to come, as NASA continues to prioritize the health and safety of astronauts on spaceflight missions.

NASA's Human Research Program (HRP) is dedicated to discovering the best methods and technologies to support safe, productive human space travel. HRP enables space exploration by reducing the risks to astronaut health and performance using ground research facilities, the International Space Station, and analog environments. This leads to the development and delivery of an exploration biomedical program focused on: informing human health, performance, and habitability standards; the development of countermeasures and risk mitigation solutions; and advanced habitability and medical support technologies. HRP supports innovative, scientific human research by funding more than 300 research grants to respected universities, hospitals, and NASA centers to over 200 researchers in more than 30 states.

Related links:

Twins Study: https://www.nasa.gov/twins-study

NASA Twins Study Investigators to Release Integrated Paper in 2018: https://www.nasa.gov/feature/nasa-twins-study-investigators-to-release-integrated-paper-in-2018

Human Research Program: http://www.nasa.gov/hrp

Journey to Mars: https://www.nasa.gov/topics/journeytomars/index.html

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/Timothy Gushanas/Human Research Program/Monica Edwards/Laurie Abadie.

Best regards, Orbiter.ch

The Penguin and the Egg












NASA - Spitzer Space Telescope patch.

Feb. 1, 2018


This image of distant interacting galaxies, known collectively as Arp 142, bears an uncanny resemblance to a penguin guarding an egg. Data from NASA's Spitzer and Hubble space telescopes have been combined to show these dramatic galaxies in light that spans the visible and infrared parts of the spectrum.

This dramatic pairing shows two galaxies that couldn't look more different as their mutual gravitational attraction slowly drags them closer together.

The "penguin" part of the pair, NGC 2336, was probably once a relatively normal-looking spiral galaxy, flattened like a pancake with smoothly symmetric spiral arms. Rich with newly-formed hot stars, seen in visible light from Hubble as bluish filaments, its shape has now been twisted and distorted as it responds to the gravitational tugs of its neighbor. Strands of gas mixed with dust stand out as red filaments detected at longer wavelengths of infrared light seen by Spitzer.

The "egg" of the pair, NGC 2937, by contrast, is nearly featureless. The distinctly different greenish glow of starlight tells the story of a population of much older stars. The absence of glowing red dust features informs us that it has long since lost its reservoir of gas and dust from which new stars can form. While this galaxy is certainly reacting to the presence of its neighbor, its smooth distribution of stars obscures any obvious distortions of its shape.

Eventually these two galaxies will merge to form a single object, with their two populations of stars, gas and dust intermingling. This kind of merger was likely a significant step in the history of most large galaxies we see around us in the nearby universe, including our own Milky Way.

At a distance of about 23 million light-years, these two galaxies are roughly 10 times farther away than our nearest major galactic neighbor, the Andromeda galaxy. The blue streak at the top of the image is an unrelated background galaxy that is farther away than Arp 142.

Spitzer Space Telescope


Combining light from across the visible and infrared spectrums helps astronomers piece together the complex story of the life cycles of galaxies. While this image required data from both the Spitzer and Hubble telescopes to cover this range of light, NASA's upcoming James Webb Space Telescope will be able to see all of these wavelengths of light, and with dramatically better clarity.

The Hubble Space Telescope is a project of international cooperation between NASA and ESA (European Space Agency). NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, Inc., in Washington, D.C.

NASA's Jet Propulsion Laboratory, Pasadena, California, manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at Caltech in Pasadena, California. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA.

Spitzer Space Telescope: http://www.nasa.gov/mission_pages/spitzer/main/index.html

Hubble Space Telescope: https://www.nasa.gov/mission_pages/hubble/main/index.html

Images, Text, Credits: NASA/Tony Greicius/ESA/STScI/AURA/JPL-Caltech.

Greetings, Orbiter.ch