ERIK MARTIN WILLÈN: March 2024

Saturday, March 30, 2024

ESA, NASA Solar Observatory Discovers Its 5,000th Comet - UNIVERSE

On March 25, 2024, a citizen scientist in the Czech Republic spotted a comet in an image from the Solar and Heliospheric Observatory (SOHO) spacecraft, which has now been confirmed to be the 5,000^th comet discovered using SOHO data. SOHO has achieved this milestone over 28 years in space, even though it was never designed to be a comet hunter.

The 5,000^th comet discovered with the Solar and Heliospheric Observatory (SOHO) spacecraft is noted by a small white box in the upper left portion of this image. A zoomed-in inset shows the comet as a faint dot between the white vertical lines. The image was taken on March 25, 2024, by SOHO’s Large Angle and Spectrometric Coronagraph (LASCO), which uses a disk to block the bright Sun and reveal faint features around it. NASA/ESA/SOHO

The comet is a small body made of ice and rock that takes only a few years to orbit the Sun. It belongs to the “Marsden group” of comets. This group is thought to be related to comet 96P/Machholz (which SOHO observes when Machholz passes near the Sun every 5.3 years) and is named for the late scientist Brian Marsden who first recognized the group using SOHO observations. Only about 75 of the 5,000 comets discovered with SOHO belong to the Marsden group.

A joint mission of ESA (European Space Agency) and NASA, SOHO launched in December 1995 to study the Sun and the dynamics in its outer atmosphere, called the corona. A science instrument on SOHO, called the Large Angle and Spectrometric Coronagraph (LASCO), uses an artificial disk to block the blinding light of the Sun so scientists can study the corona and environment immediately around the Sun.

This also allows SOHO to do something many other spacecraft cannot – see comets flying close to the Sun, known as “sungrazing” comets or “sungrazers.” Many of these comets only brighten when they’re too close to the Sun for other observatories to see and would otherwise go undetected, lost in the bright glare of our star. While scientists expected SOHO to serendipitously find some comets during its mission, the spacecraft’s ability to spot them has made it the most prolific comet-finder in history – discovering more than half of the comets known today.

In fact, soon after SOHO launched, people around the world began spotting so many comets in its images that mission scientists needed a way to keep track of them all. In the early 2000s, they launched the NASA-funded Sungrazer Project that allows anyone to report comets they find in SOHO images.

This animation shows the Solar and Heliospheric Observatory’s 5,000th comet (circled) moving across the field relative to background stars. The images in this sequence were taken with the spacecraft’s Large Angle and Spectrometric Coronagraph (LASCO) instrument. NASA/ESA/SOHO

SOHO’s 5,000^th comet was found by Hanjie Tan, a Sungrazer Project participant who is originally from Guangzhou, China, and is currently pursuing a doctoral degree in astronomy in Prague, Czech Republic. Tan has been participating in the Sungrazer Project since he was 13 years old and is one of the project’s youngest comet discoverers.

“Since 2009, I've discovered over 200 comets,” Tan said. “I got into the Sungrazer Project because I love looking for comets. It's really exciting to be the first to see comets get bright near the Sun after they've been traveling through space for thousands of years.”

Most of the 5,000 comets discovered using SOHO have been found with the help of an international cadre of volunteer comet hunters – many with no formal scientific training – participating in the Sungrazer Project.

“Prior to the launch of the SOHO mission and the Sungrazer Project, there were only a couple dozen sungrazing comets on record – that’s all we knew existed,” said Karl Battams, a space scientist at the U.S. Naval Research Lab in Washington, D.C., and the principal investigator for the Sungrazer Project. “The fact that we’ve finally reached this milestone – 5,000 comets – is just unbelievable to me.”

SOHO's 5,000th comet was discovered with the help of volunteers participating in the NASA-funded Sungrazer Project. Credit: NASA's Goddard Space Flight Center

The vast number of comets discovered using SOHO has allowed scientists to learn more about sungrazing comets and groups of comets that orbit the Sun. Comets discovered by the Sungrazer Project have also helped scientists learn more about the Sun, by watching the comets plunge through our star’s atmosphere like small solar probes.

“The statistics of 5,000 comets, and looking at their orbits and trajectories through space, is a super unique dataset – it’s really valuable science,” Battams said. “It’s a testament to the countless hours the project participants have put into this. We absolutely would never had reached this milestone if it wasn’t for what the project volunteers have done.”

The Sungrazer Project is one of many opportunities that anyone can get involved with to help make discoveries with NASA during the Heliophysics Big Year, which extends through the end of 2024. Learn more about SOHO, the Sungrazer Project, and other NASA science projects you can participate in:

by Vanessa Thomas
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Source: ESA, NASA Solar Observatory Discovers Its 5,000th Comet

Early Adopters of NASA’s PACE Data to Study Air Quality, Ocean Health - EARTH

From the atmosphere down to the surface of the ocean, data from NASA’s PACE (Plankton, Aerosol, Cloud, ocean Ecosystem) satellite benefits ecosystems, human health, and underrepresented communities.

Years before the launch in February 2024, mission leaders from NASA teamed with dozens of applied scientists and environmental professionals to prepare for the many practical uses that could be informed by PACE data. PACE’s Early Adopter program integrates science data into business, environmental management, and decision-making activities to benefit society.

A SpaceX Falcon 9 rocket with NASA’s PACE (Plankton, Aerosol, Cloud, ocean Ecosystem) spacecraft stands vertical at Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida on Feb. 5, 2024. PACE is NASA’s newest Earth-observing satellite that will help increase our understanding of Earth’s oceans, atmosphere, and climate by delivering hyperspectral observations of microscopic marine organisms called phytoplankton as well new data on clouds and aerosols. SpaceX

The researchers specialize in a wide range of topics including water resources, fisheries and aquaculture, air quality and health, climate, and agriculture. These early adopters of the science provide a bridge between the PACE team and local communities and decision-makers who need accessible products for public use. Such work can help connect the new frontier of PACE’s hyperspectral and multi-angular polarimetric data to real-world problems – and find new ways to address challenges.

Helping Coastal Communities Keep Fisheries Safe

In coastal communities, knowing the quality of the water is essential for ecosystem health, safe and sustainable seafood, and recreation – not to mention human livelihoods that depend on fisheries.

Phytoplankton are microscopic organisms that live in watery environments. When conditions are right, phytoplankton undergo explosive population growth, creating blooms visible from space. Such a bloom occurred in the North Atlantic Ocean, off the coast of Newfoundland in early August 2010. The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite captured this natural-color image on Aug. 9, 2010. The paisley pattern of peacock blue owes its color to phytoplankton. Credit: NASA/Goddard/Jeff Schmaltz/MODIS Land Rapid Response Team

Marina Marrari, executive director of the Costa Rican Fishing Federation in San José is one of PACE’s early adopters. Marrari and her colleagues developed a mobile app that will pull in data from PACE’s Ocean Color Instrument to help inform the public about harmful algal blooms. Known as pezCA, the app distributes near real-time data about ocean temperature, chlorophyll concentration, and currents as measured by other NASA satellites. Once PACE data is available, the app will be updated to include a product on specific types of harmful algal blooms that can have toxic effects on people and animals.

Bringing Air Quality Alerts to the Midwest

Information on air quality and airborne particles (aerosols) is typically available for dense urban areas like Los Angeles, Atlanta, and New York. Marcela Loría-Salazar, assistant professor at the University of Oklahoma in Norman, plans to use data from PACE’s polarimeters and OCI to study air quality in locations in the middle of the United States, where there tend to be fewer ground-based monitors.

Urban pollution emissions, desert dust, and smoke from wildfires can travel from distant places – across continents or even oceans. (Think of the wildfire smoke that can blow from Alaska and Canada into the central U.S.) PACE gathers global data on this dust and smoke in Earth’s atmosphere every one to two days, and that data is open access – meaning it is available for anyone to find and download free from the Internet.

Smoke from Canadian wildfires drifts slowly south over the United States’ Midwest. The drifting smoke can be seen in this Terra satellite image taken in December 2017 over Lake Michigan, as well as parts of Minnesota, Wisconsin, Indiana, and Ohio. NASA MODIS Rapid Response Team / Jeff Schmaltz

Loría-Salazar and her team can use this information to track aerosols, studying how they change as they move over land, change altitude, and interact with other atmospheric particles. Her goal is to better understand how these aerosols affect human health when they’re inhaled. Her team works with the Oklahoma state government to develop solutions to improve air quality decision-making.

She also works with tribal nations to help inform air quality decisions in their communities. For example, setting prescribed fires is a traditional activity to preserve ecosystems, but the fires do put smoke into the air. By using satellite data, tribal managers can make better-informed decisions about the potential risk of acute smoke exposure on a given day.

Tracking Health of Marine Mammal Ecosystems

Phytoplankton are the center of the marine food web. These microscopic organisms are food for bigger animals like zooplankton, fish, and shellfish – and ultimately whales and dolphins. While PACE can’t directly detect fish or mammals below the surface of the ocean, it can view communities of phytoplankton, which can inform scientists about the ocean ecosystem in which fish and mammals live.

Liz Ferguson on the coast of the oceans where she studies marine mammals. Courtesy of Liz Ferguson

By examining phytoplankton, scientists can gain valuable insights into changes occurring within marine habitats, as these microorganisms often serve as early indicators of regional ecosystem health. Liz Ferguson, CEO and marine ecologist for Ocean Science Analytics, studies marine mammals off the Pacific Coast of North America.

Monitoring plankton communities enhances scientists’ ability to perceive the intricate dynamics within marine ecosystems. By closely monitoring shifts in environmental variables and the behavior of indicator species such as marine mammals, Ferguson can study the impact of climate change on the California current's ecosystems.

Doubling Up Satellite Data

Some species of phytoplankton produce toxins that can be dangerous for humans, pets, and livestock. When these phytoplankton multiply to large numbers, it’s called a harmful algal bloom.

Richard Stumpf and Michelle Tomlinson, oceanographers with the National Oceanic and Atmospheric Administration (NOAA), use satellite data to study these blooms and help inform communities about their risks. They have been using data from the Ocean and Land Color Instrument on the European Space Agency's Sentinel-3 satellite, which captures Earth data by measuring certain wavelengths of light. PACE’s Ocean Color Instrument sensor does the same, but as a hyperspectral instrument, it can detect more than 200 wavelengths – more than five times the number observed by Sentinel-3 and other current instruments.

Richard Stumpf examines water from plankton net tows in Lake Erie taken in early summer 2023. A net tow concentrates plankton from the water making it easier to identify what is present, particularly when a bloom is developing. The middle jar is the unfiltered lake water, the top one is from an area that has mostly zooplankton (microscopic animals), and the bottom (greenish) one has cyanobacteria. Courtesy of Richard Stumpf

PACE data can help Stumpf and Tomlinson continue their research on how the color of harmful algal blooms change over time and space. Choosing specific wavelengths of data from PACE can also help verify the data from Sentinel-3 and extend the long-term data record.

The hyperspectral capabilities of PACE can allow scientists and environmental managers to not only spot emerging blooms, but also identify the specific communities of phytoplankton that make up the bloom. Detecting these details helps scientists better inform local water managers about the location, timing, and type of harmful algal blooms, which can help mitigate risks to the public.

Source: Early Adopters of NASA’s PACE Data to Study Air Quality, Ocean Health

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Friday, March 29, 2024

Stunning Echo of 800-year-old Explosion - UNIVERSE

X-ray: (Chandra) NASA/CXC/U. Manitoba/C. Treturik, (XMM-Newton) ESA/C. Treturik; Optical: (Pan-STARRS) NOIRLab/MDM/Dartmouth/R. Fesen; Infrared: (WISE) NASA/JPL/Caltech/; Image Processing: Univ. of Manitoba/Gilles Ferrand and Jayanne English

In the year 1181 a rare supernova explosion appeared in the night sky, staying visible for 185 consecutive days. Historical records show that the supernova looked like a temporary ‘star’ in the constellation Cassiopeia shining as bright as Saturn.

Ever since, scientists have tried to find the supernova’s remnant. At first it was thought that this could be the nebula around the pulsar — the dense core of a collapse star — named 3C 58. However closer investigations revealed that the pulsar is older than supernova 1181.

In the last decade, another contender was discovered; Pa 30 is a nearly circular nebula with a central star in the constellation Cassiopeia. It is pictured here combining images from several telescopes. This composite image uses data across the electromagnetic spectrum and shows a spectacular new view of the supernova remnant. This allows us to marvel at the same object that appeared in our ancestors’ night sky more than 800 years ago.

X-ray observations by ESA’s XMM-Newton (blue) show the full extent of the nebula and NASA’s Chandra X-ray Observatory (cyan) pinpoints its central source. The nebula is barely visible in optical light but shines bright in infrared light, collected by NASA’s Wide-field Infrared Space Explorer (red and pink). Interestingly, the radial structure in the image consists of heated sulfur that glows in visible light, observed with the ground-based Hiltner 2.4 m telescope at the MDM Observatory (green) in Arizona, USA, as do the stars in the background by Pan-STARRS (white) in Hawaii, USA.

Studies of the composition of the different parts of the remnant have led scientists to believe that it was formed in a thermonuclear explosion, and more precisely a special kind of supernova called a sub-luminous Type Iax event. During this event two white dwarf stars merged, and typically no remnant is expected for this kind of explosion. But incomplete explosions can leave a kind of ‘zombie’ star, such as the massive white dwarf star in this system. This very hot star, one of the hottest stars in the Milky Way (about 200 000 degrees Celsius), has a fast stellar wind with speeds up to 16,000 km/h. The combination of the star and the nebula makes it a unique opportunity for studying such rare explosions.

The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.

For more Chandra images, multimedia and related materials, visit:

https://www.nasa.gov/mission/chandra-x-ray-observatory/

Visual Description:

This is a composite image of SNR 1181, the remains of an explosion hundreds of years ago caused by the merger of two stars.

A bright, multi-colored, spherical nebula sits in the middle of the canvas surrounded by a field of stars that appear as white dots. In the center of the nebula is a small point of aqua-colored light. This is the hot white dwarf star that was left behind after the likely merger of two smaller white dwarfs caused an explosion. From this single point of aqua light, several spectacular rays expand outward, resembling a single firework bursting in celebration in the night sky.

Source: Stunning Echo of 800-year-old Explosion - NASA

NASA Sees Progress on Blue Origin’s Orbital Reef Life Support System - Commercial Low Earth Orbit Development Program

A digital rendering of Blue Origin’s free-flying station named Orbital Reef, which continues to be developed as part of a Space Act Agreement with NASA. Blue Origin

A NASA-funded commercial space station, Blue Origin’s Orbital Reef, recently completed testing milestones for its critical life support system as part of the agency’s efforts for new destinations in low Earth orbit.

The four milestones are part of a NASA Space Act Agreement originally awarded to Blue Origin in 2021 and focused on the materials and designs for systems to clean, reclaim, and store the air and water critical for human spaceflight.

NASA is working closely with commercial companies to develop new space stations capable of providing services to NASA and others, which will ensure that the U.S. maintains a continuous human presence in low Earth orbit and provides direct benefits for people on Earth.

“These milestones are critical to ensuring that a commercial destination can support human life so NASA astronauts can continue to have access to low Earth orbit to conduct important scientific research in the unique microgravity environment,” said Angela Hart, manager of NASA’s Commercial Low Earth Orbit Development Program. “Additionally, each milestone that is completed allows NASA to gain insight into our partner’s progress on station design and development.”

Humans living and working in space do so in a closed environment that must be monitored and controlled. On the International Space Station, components for the environmental control and life support system maintain clean air and water for astronauts. The regenerative system recycles and reclaims most of the water and oxygen produced by normal human activities. This significantly reduces the amount of mass that would have to be launched to the orbiting laboratory for these functions.

Orbital Reef will have a similar system in place. All four milestones tested different parts of the system, including a trace contaminant control test, water contaminant oxidation test, urine water recovery test, and water tank test.

The trace contaminant control test screened materials to remove harmful impurities from the air. The water containment oxidation test, urine water recovery test, and water tank test all focused on potential cleaning, reclaiming, and storing technologies.

NASA is supporting the design and development of multiple commercial space stations, including Blue Origin’s Orbital Reef, through funded and unfunded agreements. The current design and development phase will be followed by the procurement of services from one or more companies, where NASA aims to be one of many customers for low Earth orbit destinations.

NASA’s commercial strategy for low Earth orbit will provide the government with reliable and safe services at a lower cost and enable the agency to focus on Artemis missions to the Moon in preparation for Mars, while also continuing to use low Earth orbit as a training and proving ground for those deep space missions.

For more information about NASA’s commercial space strategy, visit: https://www.nasa.gov/humans-in-space/commercial-space/

Source: NASA Sees Progress on Blue Origin’s Orbital Reef Life Support System - NASA