Tag Archives: National Science Foundation

Astronomers Find Rare Star System That Will Trigger a Kilonova

An artist’s rendition of the binary stay system, called CPD-29 2176.
Illustration: Noir Lab

The universe has no shortage of oddities, and researchers at the National Science Foundation’s NOIRLab have observed another one in the form of a particular binary star system. The system, called CPD-29 2176, will eventually trigger a kilonova, a celestial event in which two neutron stars collide in a massive explosion that forms heavy elements, including gold and platinum.

CPD-29 2176 is located around 11,400 light-years from Earth and was found by researchers using NASA’s Neil Gehrels Swift Observatory. Astronomers then conducted more observations at NOIRLab’s Cerro Tololo Inter-American Observatory in Chile. CPD-29 2176 is home to one neutron star and one massive star that is in the process of going supernova, only to become a second neutron star in the future. Eventually, the two neutron stars will collide, producing a kilonova, an explosion that is thought to produce bursts of gamma rays and large amounts of gold and platinum. The paper documenting the research team’s find is published today in Nature.

“We know that the Milky Way contains at least 100 billion stars and likely hundreds of billions more. This remarkable binary system is essentially a one-in-ten-billion system,” said André-Nicolas Chené in a NOIRLab press release. Chené is a NOIRLab astronomer and an author on the study. “Prior to our study, the estimate was that only one or two such systems should exist in a spiral galaxy like the Milky Way.”

While many stars implode was a powerful supernova when they die, the dying star in CPD-29 2176 is becoming an ultra-stripped supernova. An ultra-stripped supernova lacks the vast amount of force that a typical supernova has, since the dying star has had much of its mass stripped by its companion. The researchers think that the neutron star in the system was also formed with an ultra-stripped supernova and argue that this is the reason that CPD-29 2176 is able to remain as a binary—a typical supernova would have enough power to kick a companion star out of its orbit.

“The current neutron star would have to form without ejecting its companion from the system. An ultra-stripped supernova is the best explanation for why these companion stars are in such a tight orbit,” said lead author Noel D. Richardson, a physics and astronomy professor at Embry-Riddle Aeronautical University, in the NOIRLab release. “To one day create a kilonova, the other star would also need to explode as an ultra-stripped supernova so the two neutron stars could eventually collide and merge.”

It will take around one million years for the star undergoing ultra-stripped supernova to turn into a neutron star. It is then when the two stars will begin to spiral into each other, eventually resulting in the metal-producing kilonova, according to the research. In these dramatic cosmic endings, we can look forward to the creation of the same elements that make life possible.  

More: Watch Four Planets Spin Around a Star 130 Million Light-Years Away

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Large Satellite Could Be Bad for Astronomers Observing Skies

A huge satellite is about to take flight, spreading its giant antenna array to potentially block astronomers’ views of the cosmos. AST SpaceMobile’s BlueWalker 3 is scheduled for launch on Saturday to test the company’s broadband network technology, but the prototype satellite is extremely bright and could interfere with celestial observations.

BlueWalker is scheduled to ride to low Earth orbit aboard SpaceX’s Falcon 9 rocket at 7:51 p.m. ET from the Kennedy Space Center in Florida. Once in low Earth orbit, the satellite will test out the Texas-based company’s ability to directly beam internet connectivity from space to people’s cellphones. The Chairman and CEO of AST SpaceMobile Abel Avellan recently boasted on Twitter, “Made in TX— size matters!” when referring to the satellite. And indeed it does, as this bad boy sports a 693 square foot array of antennas (64 square meters) that will unfold in space. With its antenna fully unfurled, the satellite is expected to be among the brightest objects in the night sky, according to Sky and Telescope.

As it points towards Earth, the satellite’s giant array will reflect sunlight back to our planet, potentially causing bright streaks across astronomical images and interfering with scientific data. Even worse is that if the test satellite succeeds in its mission, the company could send more than 100 of its satellites to orbit by the end of 2024 to build out a full internet constellation. The operational satellites, which are to be named BlueBirds, could cause even more interference as they are expected to be of similar size to BlueWalker 3.

Astronomers have expressed concern over the satellite’s brightness as it joins the hoards of commercial satellite constellations currently being built in low Earth orbit. From the location of Rubin Observatory on Cerro Pachon in Chile, the BlueWalker satellite will be as bright as the star Vega near zenith in twilight, according to Connie Walker, an astronomer at the National Science Foundation’s (NSF) NOIRLab. “These new satellites are expected to saturate Rubin observations,” Walker told Gizmodo in an email.

In an effort to understand the extent of this threat, NSF’s NOIRLab and the International Astronomical Union’s (IAU) Centre for the Protection of the Dark and Quiet Sky from Satellite Constellation Interference have called on astronomers from around the world to take brightness observations of the satellite once it’s in orbit. “[Low Earth orbit satellites] disproportionately affect science programs that require twilight observations, such as searches for Earth-threatening asteroids and comets, outer Solar System objects, and visible-light counterparts of fleeting gravitational-wave sources,” NSF wrote in a report.

BlueWalker is launching to space along with 60 of SpaceX’s Starlink satellites, which have already caused disruption of astronomical observations. Elon Musk’s private space company is seeking to launch a whopping 42,000 satellites to low Earth orbit to build a broadband internet megaconstellation. Although SpaceX has only received approval for 12,000 satellites by the Federal Communications Commission thus far. But the company has been in talks with IAU to figure out ways to dim the brightness of their satellites so that they don’t interfere with images of the cosmos.

The advancement in technology brings on an exciting era for our connectivity, so hopefully it doesn’t come at the cost of our ability to stare at celestial objects and gather valuable data about the universe.

More: SpaceX Launches 3,000th Starlink Satellite as Elon’s Internet Constellation Continues to Grow



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Signs of Water Seen in Massive Galaxy of the Early Universe

Scientists studying the most massive known galaxy in the early universe have found evidence of water in it, an intriguing observation that sheds light on how the universe has evolved.

This massive galaxy is actually a pair of galaxies, which are known together as SPT0311-58. First discovered in 2017, the galactic duo is seen as they were when the universe was a mere 780 million years old (it’s now encroaching on its 14 billionth birthday). Finding water there makes it the most distant detection of the stuff in a regular star-forming galaxy. The team’s research was accepted for publication in The Astrophysical Journal.

“This galaxy is the most massive galaxy currently known at high redshift, or the time when the Universe was still very young,” said Sreevani Jarugula, an astronomer at the University of Illinois and a co-author of the recent paper, in a National Radio Astronomy Observatory press release. “It has more gas and dust compared to other galaxies in the early Universe, which gives us plenty of potential opportunities to observe abundant molecules and to better understand how these life-creating elements impacted the development of the early Universe.”

It may look like a couple magenta smudges, but that distant galaxy is essentially a repository of information about the universe shortly after the Big Bang. SPT0311-58 was found by researchers using the Atacama Large Millimeter/submillimeter Array, or ALMA, one of the best telescope arrays around for looking at the beginnings of the universe.

ALMA is located high in Chile’s Atacama Desert, giving it terrifically sharp and unpolluted views of the night sky. The array also drove the recent finding, which comes from a study of the galaxy’s gas content. Besides water molecules, the researchers also found carbon monoxide.

Part of the ALMA telescope in Chile’s Atacama Desert.
Photo: MARTIN BERNETTI/AFP (Getty Images)

“This exciting result, which shows the power of ALMA, adds to a growing collection of observations of the early Universe,” said Joe Pesce, an astrophysicist and ALMA Program Director at the National Science Foundation, in the same release. “These molecules, important to life on Earth, are forming as soon as they can, and their observation is giving us insight into the fundamental processes of a Universe very much different from today’s.”

Things were pretty energetic earlier in the universe, so young galaxies (meaning the most ancient ones we see today) produced stars at a much greater rate than our own galaxy does now. Looking at the types of gases and dusts in those galaxies and their relative proportions can help astronomers answer questions about the rate of star formation and how galaxies like SPT0311-58 interact with one another and the interstellar medium.

ALMA has a terrific habit of imaging these faraway smudges and discerning the minutiae that make them up, thereby helping astronomers better understand the beginning of everything and, maybe, what gave rise to us. Here’s to ALMA and all the discoveries it’s still to make.

More: Scientists Are Turning Earth Into a Telescope to See a Black Hole

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Cleanup Costs at the Damaged Arecibo Observatory Could Reach $50 Million

Damage at the dish following the collapse of the 900-ton instrument platform.
Image: Ricardo Arduengo/AFP (Getty Images)

A new estimate suggests it’ll cost somewhere between $30 million and $50 million to clean up the mess created by the collapse of the iconic Arecibo Observatory dish late last year, according to an NSF report detailing the aftermath of the disaster and possible next steps.

The investigation into the cause of the collapse at the Arecibo Observatory in Puerto Rico is still ongoing, but the National Science Foundation, through the Consolidated Appropriations Act, 2021, was asked to provide a report to Congress outlining the “causes and extent of the damage, the plan to remove debris in a safe and environmentally sound way, the preservation of the associated [Arecibo Observatory] facilities and surrounding areas, and the process for determining whether to establish comparable technology at the site, along with any associated cost estimates.”

The NSF had just 60 days to produce the report upon enactment of the Act, which may explain why it’s so achingly thin on details. The report is just seven pages long and replete with information we already knew. That said, the NSF did provide some new details, such as the cleanup cost estimate, an overview of damage done to the facility, and an update on the cleanup, among other matters.

To recap, an auxiliary cable from a support tower pulled loose from its socket on August 10, 2020, resulting in extensive damage to the reflector panels below. A main cable on the same tower snapped several months later, resulting in even further damage to the dish, which has been used for radar and radio astronomy since 1963. The second cable failure was especially troubling, as “this cable broke under conditions that should have been well within its support capabilities, indicating that it, along with the remaining main cables, may have been weaker than expected,” according to the new report. Engineering firms brought in to evaluate the structure said a subsequent cable failure would be catastrophic, resulting in the decision to decommission the 1,000-foot (305-meter) dish. As plans were being made to demolish the storied radio telescope, however, the 900-ton platform gave way, collapsing on December 1, 2020.

Inspections done after the collapse showed that the platform and Gregorian dome were a “complete loss for scientific purposes,” per the report. The top 59 feet (18 meters) of platform support towers 12 and 4 broke off during the collapse, and the top 121 feet (37 meters) of platform support tower 8 snapped off. As the report states, “further assessments of the structural integrity of the towers continue.”

The roof of the Learning Center sustained significant damage, but the NSF said it’s repairable. A trailer used by Educational and Public Outreach staff was completely “demolished,” while the Visitor Center came away unscathed, save for some minor damage caused by falling bits of concrete, the new report said.

A private contractor and experts from NASA’s Kennedy Space Center are currently conducting a forensics analysis to determine the cause of the original auxiliary cable socket failure. A separate contractor is performing the forensic investigation at Arecibo, with final reports from both contractors expected in December 2021. In addition to these efforts, the NSF is asking that an “expedited independent study” into the cause of the cable failures be completed by the National Academies of Sciences, Engineering, and Medicine.

A company that specializes in disaster cleanup and environmental remediation has been brought in to help. Soils contaminated with hydraulic oils, which were released during the collapse, are being sampled and removed. The cleanup team is also testing groundwater and surface water near the facility. A “Stormwater Pollution Prevention Plan” is in the works to “prevent sediment and pollutants from migrating offsite,” as are wildlife and vegetation surveys to help in the protection of vulnerable species, according to the report.

The report lists the preliminary cost estimates for the cleanup as being between $30 million and $50 million from now until the end of 2022.

The NSF is now working with the Puerto Rico State Historic Preservation Office and the Federal Advisory Council on Historic Preservation on the “protection and preservation of historically important elements of the structures and site.” Valuable or worthwhile objects found during the cleanup process could go on display at the observatory or sent to museums.

The future of the facility remains unclear. The NSF says it’s still too soon to know how the facility might be repaired or reconstructed to enable different kinds of scientific endeavors, adding that restoration will “require differing levels of effort and funding.” The authors said “many technologies and more than a dozen distinct capabilities” are still in place at the site, including a smaller 40-foot (12-meter) radio telescope and a LIDAR facility used to study the composition and motion of the ionosphere. As for repairing or re-inventing the large dish, the NSF said its “process for establishing any significant new scientific facility relies on priorities established by the scientific community and rigorous peer review of the intellectual merit and broader impacts of the proposed activity.”

A community workshop planned for this coming April should provide more information about the Arecibo Observatory and its future.

That a radio dish could be rebuilt at the facility is not out of the question. A proposal to build a $450 million “Next Generation Arecibo Telescope” was tabled by the observatory last month. It’s been dark days at Arecibo, but perhaps there’s reason for optimism.

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