mercredi 12 janvier 2022

Baby Stars in the Orion Constellation

 





NASA - WISE Mission patch.


Jan 12, 2022


Scores of baby stars shrouded by dust are revealed in this infrared image of the star-forming region NGC 2174, as seen by NASA’s Spitzer Space Telescope. Some of the clouds in the region resemble the face of a monkey in visible-light images, hence the nebula's nickname: the "Monkey Head." However, in infrared images such as this, the monkey disappears. That's because different clouds are highlighted in infrared and visible-light images.

Found in the northern reaches of the constellation Orion, NGC 2174 is located around 6,400 light-years away. Columns of dust, slightly to the right of center in the image, are being carved out of the dust by radiation and stellar winds from the hottest young stars recently born in the area.

Spitzer’s infrared view provides us with a preview of the next clusters of stars that will be born in the coming millennia. The reddish spots of light scattered through the darker filaments are infant stars swaddled by blankets of warm dust. The warm dust glows brightly at infrared wavelengths. Eventually, these stars will pop out of their dusty envelopes and their light will carve away at the dust clouds surrounding them.

In this image first published in 2015, infrared wavelengths have been assigned visible colors we see with our eyes. Light with a wavelength of 3.5 microns is shown in blue, 8.0 microns is green, and 24 microns in red. The greens show the organic molecules in the dust clouds, illuminated by starlight. Reds are caused by the thermal radiation emitted from the very hottest areas of dust.

Areas around the edges that were not observed by Spitzer have been filled in using infrared observations from NASA’s Wide Field Infrared Survey Explorer, or WISE.

Wide Field Infrared Survey Explorer (WISE): https://www.nasa.gov/mission_pages/WISE/main/index.html

Image Credits: NASA/JPL-Caltech/Text Credits: NASA/Yvette Smith.

Best regards, Orbiter.ch

mardi 11 janvier 2022

Dragon, Spacewalk Preps Amidst Space Botany and Biology Research

 







ISS - Expedition 66 Mission patch.


Jan 11, 2022

The International Space Station is gearing up for the departure of a U.S. resupply ship and a Russian spacewalk next week. Meanwhile, the Expedition 66 crew is maintaining its pace of research exploring how microgravity affects variety of biological phenomena.

The SpaceX Cargo Dragon vehicle has been docked to the Harmony module’s space-facing docking port since Dec. 22 when it delivered over 6,500 pounds of new science experiments, crew supplies, and station hardware. It is now being readied for departure on Jan. 21 its return to Earth a day later loaded with completed space research and old lab gear for analysis and inspection.


Image above: The station is pictured from the SpaceX Crew Dragon Endeavour during a fly around that took place on Nov. 8, 2021. Image Credit: NASA.

NASA Flight Engineers Kayla Barron and Raja Chari took turns Tuesday morning organizing and packing gear inside the Cargo Dragon. Chari then spent the afternoon swapping out science freezer components inside Dragon that will soon house research samples for examination by scientists on Earth.

Barron later collected root and shoot samples from Arabidopsis plants grown on petri plates readying them for stowage and analysis back on the ground. NASA astronaut Mark Vande Hei worked on another space botany investigation as he photographed and harvested cotton cultures grown on the station to understand how weightlessness affects plant genetics.

International Space Station (ISS). Animation Credit: ESA

NASA Flight Engineer Thomas Marshburn spent Tuesday on several human research and space biology tasks. He wrapped up blood pressure measurements for the Vascular Aging study, set up the Life Science Glovebox for an upcoming experiment, then took a robotics test for a behavioral investigation. Astronaut Matthias Maurer from ESA (European Space Agency) also worked on life science as he collected microbe samples for analysis, swapped particle samples inside the Mochii electron-scanning microscope, then took a cognition test.

Two cosmonauts, station Commander Anton Shkaplerov and Flight Engineer Pyotr Dubrov, continue getting ready for a spacewalk on Jan.19. Today, they configured a pair of Russian Orlan spacesuits that will be worn in the vacuum of space when they configure the station’s two newest modules, Nauka and Prichal.

Related links:

Expedition 66: https://www.nasa.gov/mission_pages/station/expeditions/expedition66/index.html

Harmony module: https://www.nasa.gov/mission_pages/station/structure/elements/harmony

Arabidopsis plants: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8297

Plant genetics: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8341

Vascular Aging: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7644

Life Science Glovebox: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=7676

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

Microbe samples: https://blogs.nasa.gov/spacestation/2022/01/11/dragon-spacewalk-preps-amidst-space-botany-and-biology-research/nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8333

Mochii: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=7657

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

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

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

Best regards, Orbiter.ch

NASA Prepares SLS Moon Rockets for First Crewed Artemis Missions

 







NASA - Space Launch System (SLS) logo.


Jan 11, 2022

As teams continue to prepare NASA’s Space Launch System (SLS) rocket for its debut flight with the launch of Artemis I, NASA and its partners across the country have made great progress building the rocket for Artemis II, the first crewed Artemis mission. The team is also manufacturing and testing major parts for Artemis missions III, IV and V.

“The Space Launch System team is not just building one rocket but manufacturing several rockets for exploration missions and future SLS flights beyond the initial Artemis launch,” said John Honeycutt, SLS program manager at NASA’s Marshall Space Flight Center in Huntsville, Alabama. “The Artemis I mission is the first in a series of increasingly complex missions that will extend our presence on the Moon. The SLS rocket’s unprecedented power and capabilities will send missions farther and faster throughout the solar system.”


Image above: Casting and assembly of solid rocket booster, shown her, for the Artemis IV mission is underway at Northrop Grumman’s factory in Promontory, Utah. The booster motors for Artemis II and Artemis III have completed casting and are ready to go to NASA’s Kennedy Space Center where they will be assembled with other booster hardware being prepared for the missions. Image Credit: NASA.

With its two solid rocket boosters and four RS-25 engines, SLS produces more than 8.8 million pounds of thrust to launch each Artemis mission beyond Earth’s orbit and onward to the Moon. The rocket features some of the largest, most advanced, and most reliable hardware elements ever built for space exploration.

To power the agency’s next-generation deep space missions, SLS delivers propulsion in phases. At liftoff, the core stage with its four RS-25 engines and the twin boosters fire to propel SLS off the launch pad into orbit. Once in orbit, the Interim Cryogenic Propulsion Stage (ICPS) provides the in-space propulsion to send NASA’s Orion spacecraft and its crew on a precise trajectory toward the Moon.

The first piece of rocket hardware – the ICPS – for Artemis II arrived in Florida July 28, 2021. It is undergoing final preparations at lead contractors Boeing and United Launch Alliance’s (ULA) facilities and will soon be delivered nearby to NASA’s Kennedy Space Center. The ICPS fires its RL10 engine, provided by Aerojet Rocketdyne, to send the Orion spacecraft toward the Moon. ULA is already building the Artemis III ICPS in its factory in Decatur, Alabama.


Image above: The Interim Cryogenic Propulsion Stage (ICPS) – for Artemis II arrived at the Space Coast on July 28, 2021. It is undergoing final preparations at prime contractors Boeing and United Launch Alliance’s (ULA) facilities and will soon be delivered to nearby Kennedy Space Center. The ICPS fires its RL10 engine, provided by Aerojet Rocketdyne, to send the Orion spacecraft toward the Moon. ULA is already building the Artemis III ICPS in its factory in Decatur, Alabama. Image Credit: ULA.

“The Space Launch System is a highly capable launch vehicle purposely designed and rigorously tested to safely transport people, large cargo, and flagship science missions to deep space destinations,” said John Blevins, SLS chief engineer at Marshall. “From the beginning, the SLS rocket was built to first safely send astronauts to space, and at the same time, to evolve to an even more powerful configuration that can support a variety of missions.”

Every NASA center and more than 1,000 different companies across America helped build the Artemis I SLS rocket as well as the SLS rockets that will launch future missions. The boosters and RS-25 engines – the main propulsion elements of the rocket -- for the Artemis II and Artemis III missions are in the final stages of assembly. In Utah, crews with Northrop Grumman, the lead contractor for the boosters, have completed casting all the booster motor segments for both Artemis II and Artemis III and began casting segments for Artemis IV. The five-segment solid rocket booster is the largest and most powerful booster ever built for spaceflight.

Aerojet Rocketdyne, the RS-25 lead contractor, is readying the RS-25 engines for the next three SLS flights after Artemis I. The engines have been tested and will be integrated with their respective core stages closer to final assembly. The engines for Artemis II are ready to go to NASA’s Michoud Assembly Facility in New Orleans, where they’ll be integrated with the SLS core stage. The Artemis III engines are being prepared for flight at Aerojet Rocketdyne’s facility at NASA’s Stennis Space Center near Bay St. Louis, Mississippi, and the company is already manufacturing engines for missions beyond Artemis IV.


Image above: NASA Administrator Bill Nelson and Deputy Administrator Pam Melroy get a look at the Space Launch System (SLS) core stage engine section that will be part of the Artemis IV Moon rocket. The core stage and its four RS-25 engines produce 2.2 million pounds of thrust to help launch mission. NASA and lead contractor Boeing are building core stages for three Artemis missions at the agency’s Michoud Assembly Facility in New Orleans. They also have started development work on the Exploration Upper Stage, a powerful rocket stage, that can send even more payload to the Moon than the rocket’s initial configuration for the first three missions. Image Credit: NASA.

Each 212-foot-tall core stage is produced by Boeing at Michoud. The factory’s 2.2-million-square-feet of manufacturing space and its cutting-edge manufacturing equipment allow teams to build multiple rocket stages at once. Currently, NASA and Boeing, the lead contractor for the SLS core stage, are building core stages for Artemis II, Artemis III, and Artemis IV at Michoud. In addition to the core stage, manufacturing at Michoud has started on test articles for the Exploration Upper Stage (EUS) that will power the Block IB configuration of the rocket starting with the Artemis IV mission.

“New tooling has been installed at Michoud to build the Exploration Upper Stage at the same time core stages are produced,” said Steve Wofford, NASA’s manager for the SLS Block IB effort. The EUS will send 83,000 pounds to the Moon, which is 40 percent more payload to orbit than the ICPS used on early Artemis missions, and 70 percent more than any existing rocket.”

Crews from Teledyne Brown Engineering in Huntsville, Alabama, and Marshall are manufacturing the cone-shaped launch vehicle stage adapters and Orion stage adapters for Artemis II and Artemis III. The adapters serve as vital connection points for the core and ICPS and Orion spacecraft. For missions beyond Artemis III, the universal stage adapter will connect the EUS to the Orion spacecraft and act as a payload storage compartment, accommodating large payloads, such as logistics modules or other exploration spacecraft. Engineers at RUAG Space USA completed panels for a universal stage adapter test article and delivered the panels to Dynetics in Huntsville, Alabama, the lead contractor for the adapter, that is assembling the test article in preparation for tests later in 2022.

With Artemis, NASA will land the first woman and the first person of color on the lunar surface and establish long-term exploration at the Moon in preparation for human missions to Mars. SLS and NASA’s Orion spacecraft, along with the human landing system and the Gateway in orbit around the Moon, are NASA’s foundation for deep space exploration.

For more on NASA’s SLS and additional photographs, visit: https://www.nasa.gov/sls

Images (mentioned), Text, Credits: NASA/Jennifer Harbaugh/Marshall Space Flight Center/Tracy McMahan/Ray Osorio.

Greetings, Orbiter.ch

NASA’s New IXPE Mission Begins Science Operations

 






NASA - IXPE Mission patch.


Jan 11, 2022

NASA’s newest X-ray eyes are open and ready for discovery!

Having spent just over a month in space, the Imaging X-ray Polarimetry Explorer (IXPE) is working and already zeroing in on some of the hottest, most energetic objects in the universe.

A joint effort between NASA and the Italian Space Agency, IXPE is the first space observatory dedicated to studying the polarization of X-rays coming from objects like exploded stars and black holes. Polarization describes how the X-ray light is oriented as it travels through space.

“The start of IXPE’s science observations marks a new chapter for X-ray astronomy,” said Martin Weisskopf, the mission’s principal investigator at NASA’s Marshall Space Flight Center in Huntsville, Alabama. “One thing is certain: we can expect the unexpected.”


Image above: Cassiopeia A supernova remnant. Image Credits: NASA/CXC/SAO.

IXPE launched Dec. 9 on a Falcon 9 rocket into orbit 370 miles (600 kilometers) above Earth’s equator. The observatory’s boom, which provides the distance needed to focus X-rays onto its detectors, was deployed successfully on Dec. 15. The IXPE team spent the next three weeks checking out the observatory’s maneuvering and pointing abilities and aligning the telescopes.

Over the course of these tests, the team pointed IXPE at two bright calibration targets: 1ES 1959+650, a black-hole-powered galaxy core with jets shooting into space; and SMC X-1, a spinning dead star, or pulsar. The brightness of these two sources made it easy for the IXPE team to see where X-rays are falling on IXPE’s polarization-sensitive detectors and make small adjustments to the telescopes’ alignment.

What’s Next for IXPE?

On Jan. 11, IXPE began observing its first official scientific target – Cassiopeia A, or Cas A – the remains of a massive star that blew itself apart in a supernova around 350 years ago in our own Milky Way galaxy. Supernovae are filled with magnetic energy and accelerate particles to near light-speed, making them laboratories for studying extreme physics in space.

IXPE will provide details about Cas A’s magnetic field structure that can’t be observed in other ways. By studying the X-ray polarization, scientists can work out the detailed structure of its magnetic field and the sites where these particles pick up speed.

Imaging X-ray Polarimetry Explorer (IXPE). Image Credit: NASA

IXPE’s observations of Cas A will last about three weeks.

“Measuring X-ray polarization is not easy,” said Weisskopf. “You have to collect a lot of light, and the unpolarized light acts like background noise. It can take a while to detect a polarized signal.”

More about the IXPE Mission

IXPE transmits scientific data several times a day to a ground station operated by the Italian Space Agency in Malindi, Kenya. The data flows from the Malindi station to IXPE’s Mission Operations Center at the University of Colorado Boulder’s Laboratory for Atmospheric and Space Physics (LASP) and then to IXPE’s Science Operations Center at NASA Marshall for processing and analysis. IXPE’s scientific data will be publicly available from the High Energy Astrophysics Science Research Center at the NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

The Marshall science operations team also coordinates with mission operations team at LASP to schedule science observations. The mission plans to observe more than 30 planned targets during its first year. The mission will study distant supermassive black holes with energetic particle jets that light up their host galaxies. IXPE will also probe the twisted space-time around stellar-mass black holes and measure their spin. Other planned targets include different types of neutron stars, such as pulsars and magnetars. The science team has also reserved about a month to observe other interesting objects that may appear in the sky or brighten unexpectedly.

IXPE is a collaboration between NASA and the Italian Space Agency with partners and science collaborators in 12 countries. Ball Aerospace, headquartered in Broomfield, Colorado, manages spacecraft operations.

Related link:

IXPE (Imaging X-ray Polarimetry Explorer): https://www.nasa.gov/ixpe

Images (mentioned), Text, Credits: NASA/Lee Mohon/Marshall Space Flight Center/Molly Porter.

Greetings, Orbiter.ch

NASA’s InSight Enters Safe Mode During Regional Mars Dust Storm

 






NASA - InSight Mission patch.


Jan 11, 2022

The lander has taken measures to conserve energy; engineers aim to return to normal operations next week.


Image above: This selfie of NASA’s InSight lander is a mosaic made up of 14 images taken on March 15 and April 11, 2019 – the 106th and 133rd Martian days, or sols, of the mission – by InSight’s Instrument Deployment Camera, located on its robotic arm. Image Credits: NASA/JPL-Caltech.

NASA’s InSight lander is stable and sending health data from Mars to Earth after going into safe mode Friday, Jan. 7, following a large, regional dust storm that reduced the sunlight reaching its solar panels. In safe mode, a spacecraft suspends all but its essential functions.

The mission’s team reestablished contact with InSight Jan. 10, finding that its power was holding steady and, while low, was unlikely to be draining the lander’s batteries. Drained batteries are believed to have caused the end of NASA’s Opportunity rover during an epic series of dust storms that blanketed the Red Planet in 2018.

Even before this recent dust storm, dust had been accumulating on InSight’s solar panels, reducing the lander’s power supply. Using a scoop on the lander’s robotic arm, InSight’s team came up with an innovative way to reduce the dust on one panel, and gained several boosts of energy during 2021, but these activities become increasingly difficult as available energy decreases.

Dust storms can affect solar panels in two ways: Dust reduces sunlight filtering through the atmosphere, and it can also accumulate on the panels. Whether this storm will leave an additional layer of dust on the solar panels remains to be determined.

The current dust storm was first detected by the Mars Color Imager (MARCI) camera aboard NASA’s Mars Reconnaissance Orbiter, which creates daily color maps of the entire planet. Those maps allow scientists to monitor dust storms and can serve as an early warning system for spacecraft on the Martian surface. InSight’s team received data indicating the regional storm is waning.

The whirlwinds and gusts of dust storms have helped to clear solar panels over time, as with the Spirit and Opportunity Mars rover missions. While InSight’s weather sensors have detected many passing whirlwinds, none have cleared any dust.

InSight’s engineers are hopeful they will be able to command the lander to exit safe mode next week. This will allow more flexibility in operating the lander, as communication, which requires a relatively large amount of energy, is limited in safe mode to conserve battery charge.

InSight landed on Mars on Nov. 26, 2018, to study the inner structure of the planet, including its crust, mantle and core. The spacecraft achieved its science objectives before its prime mission ended a year ago. NASA then extended the mission for up to two years, to December 2022, based on the recommendation of an independent review panel composed of experts with backgrounds in science, operations and mission management.

More About the Mission

JPL manages InSight for NASA’s Science Mission Directorate. InSight is part of NASA’s Discovery Program, managed by the agency's Marshall Space Flight Center in Huntsville, Alabama. Lockheed Martin Space in Denver built the InSight spacecraft, including its cruise stage and lander, and supports spacecraft operations for the mission.

InSight & mission logo animation. Animation Credits: NASA/JPL-Caltech

A number of European partners, including France’s Centre National d’Études Spatiales (CNES) and the German Aerospace Center (DLR), are supporting the InSight mission. CNES provided the Seismic Experiment for Interior Structure (SEIS) instrument to NASA, with the principal investigator at IPGP (Institut de Physique du Globe de Paris). Significant contributions for SEIS came from IPGP; the Max Planck Institute for Solar System Research (MPS) in Germany; the Swiss Federal Institute of Technology (ETH Zurich) in Switzerland; Imperial College London and Oxford University in the United Kingdom; and JPL. DLR provided the Heat Flow and Physical Properties Package (HP3) instrument, with significant contributions from the Space Research Center (CBK) of the Polish Academy of Sciences and Astronika in Poland. Spain’s Centro de Astrobiología (CAB) supplied the temperature and wind sensors.

Related link:

InSight Mars Lander: https://www.nasa.gov/mission_pages/insight/main/index.html

Image (mentioned), Animation (mentioned), Text, Credits: NASA/Tony Greicius/Karen Fox/Alana Johnson/JPL/Andrew Good.

Best regards, Orbiter.ch

The Milky Way's Supermassive Black Hole Has a Leak

 






NASA - Hubble Space Telescope patch.


Jan 11, 2022


Our Milky Way's central black hole has a leak. This supermassive black hole looks like it still has the vestiges of a blowtorch-like jet dating back several thousand years. NASA's Hubble Space Telescope hasn't photographed the phantom jet but has helped find circumstantial evidence that it is still pushing feebly into a huge hydrogen cloud and then splattering, like the narrow stream from a hose aimed into a pile of sand.

This composite image is of X-rays, molecular gas, and warm ionized gas near the galactic center. The orange-colored features are of glowing hydrogen gas. One such feature, at the top tip of the jet is interpreted as a hydrogen cloud that has been hit by the outflowing jet. The jet scatters off the cloud into tendrils that flow northward. Farther down near the black hole are X-ray observations of superheated gas colored blue and molecular gas in green. These data are evidence that the black hole occasionally accretes stars or gas clouds, and ejects some of the superheated material along its spin axis.

Hubble Space Telescope (HST)

For more information about Hubble, visit:

http://hubblesite.org/

http://www.nasa.gov/hubble

http://www.spacetelescope.org/

Image, Animation Credits: NASA, ESA, and Gerald Cecil (UNC-Chapel Hill); Image Processing: Joseph DePasquale (STScI)/Text Credits: NASA/Yvette Smith.

Greetings, Orbiter.ch

The Incredible ASIM: Distant galaxy edition

 







ISS / ESA - ASIM logo.


Jan 11, 2022

The Atmosphere–Space Interactions Monitor, or ASIM for short, is a first-of-its-kind complement of instruments on the International Space Station. Dubbed the ‘space storm hunter’, ASIM measures electric events in Earth’s upper atmosphere with cameras, photometers and X- and gamma-ray detectors.

ASIM on Columbus

Recently, ASIM unexpectedly detected a unique gamma-ray burst from outer space. This fortuitous observation was published in Nature magazine, less than a year after ASIM made a cover story.

It came from outer space

Mounted outside the Columbus module and designed to look downwards for electrical discharges born in stormy weather conditions in Earth’s upper atmosphere, ASIM recently detected another peculiar phenomenon: a burst of photon radiation coming from another galaxy.

The spurt turned out to be from an explosive flare from a magnetar located 10 million light-years away in a distant galaxy. Magnetars are a special type of neutron star – the collapsed core of what was once a supergiant star.

Illustration of a magnetar

Neutron stars spin very fast. The magnetic field of magnetars, however, is believed to be so powerful that it slows down the spin, tearing at the star’s crust and producing powerful bursts of radiation, x-ray and gamma-rays in particular.

Thanks to its design and performance, ASIM was able to record this gamma-ray photon outburst at extremely high speeds.

The measurements revealed unexpected, periodic “flickering” of the photon burst that will help to shed light on the physics of magnetars and the structure of neutron stars in general, one of the hottest topics in current research. The results were published in the December issue of Nature magazine.

https://www.nature.com/articles/s41586-021-04101-1?utm_medium=Social&utm_campaign=nature&utm_source=Twitter#Echobox=1640206807

Earth-bound and beyond

Since its launch in 2018, ASIM has been keeping researchers busy. From its vantage point outside the International Space Station, ASIM has provided tons of data on ‘transient luminous events’ sporting names like blue jets and red sprites taking place above thunderstorms in the upper atmosphere.

Aside from being a little-understood phenomenon and part of our world, these powerful electrical charges can reach into the stratosphere and above and change the chemical composition of the atmosphere with implications for the atmospheric radiation balance. The findings may help to make climate models more accurate.

Artist's impression of a terrestrial gamma-ray flash

Researchers are investigating the relationship between terrestrial gamma-ray bursts, lightning and high-altitude electric discharges across all seasons, across our world and at different times of day and night. Learn more about ASIM’s mission in this handy infographic.

This week ASIM was moved to another spot outside the Space Station to gracefully make place for an American technology demonstration payload. The move was carried out by the Station’s robotic arm.

From its new vantage point, just next to its current one, ASIM is pointing in a different direction, slightly more towards the horizon instead of straight down. This will help researchers work out how much our atmosphere influences the processes of electrical discharges. It’s like viewing a firework display from the side: one can enjoy the shapes more than if one is just below the display.

ASIM was built by Danish company Terma, Danish Technical University, University of Bergen in Norway and the University of Valencia in Spain for the European Space Agency.

Related link:

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

Images, Text, Credits: ESA/NASA.

Best regards, Orbiter.ch