Nobel Prize Awarded for Sensational Gravitational Waves Discovery

Nobel Prize Awarded for Sensational Gravitational Waves Discovery
By Megan Gannon, Live Science Contributor | October 3, 2017 09:10am ET

BERLIN — As expected by many, the 2017 Nobel Prize in physics went to three scientists who helped detect gravitational waves, ripples in space-time predicted by Einstein.

“This year’s prize is about a discovery that shook the world,” physicist Thors Hans Hansson said when announcing the winners from Stockholm.

Half of the 9 million Swedish krona ($1.1 million) award will go to Rainer Weiss of MIT. The other half will go jointly to Barry Barish and Kip Thorne of Caltech. All three were founders of the Laser Interferometer Gravitational-Wave Observatory, or LIGO, which detected gravitational waves for the first time in 2015.

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BERLIN — As expected by many, the 2017 Nobel Prize in physics went to three scientists who helped detect gravitational waves, ripples in space-time predicted by Einstein.

“This year’s prize is about a discovery that shook the world,” physicist Thors Hans Hansson said when announcing the winners from Stockholm.

Half of the 9 million Swedish krona ($1.1 million) award will go to Rainer Weiss of MIT. The other half will go jointly to Barry Barish and Kip Thorne of Caltech. All three were founders of the Laser Interferometer Gravitational-Wave Observatory, or LIGO, which detected gravitational waves for the first time in 2015.

https://www.space.com/38347-3-scientists-win-nobel-in-physics-for-detecting-gravitational-waves.html
Moving masses generate waves of gravitational radiation that stretch and squeeze space-time. <a href="http://www.space.com/25089-how-gravitational-waves-work-infographic.html">See how gravitational waves work in this Space.com infographic</a>.

Moving masses generate waves of gravitational radiation that stretch and squeeze space-time. See how gravitational waves work in this Space.com infographic.

Credit: By Karl Tate, Infographics Artist

Albert Einstein had theorized that space-time can be stretched and compressed by collisions of massive objects in the universe. However, experimental proof for such events eluded scientists for 100 years. [The 18 Biggest Unsolved Mysteries in Physics]

On Sept. 14, 2015, LIGO’s two extremely sensitive instruments in Washington state and Louisiana simultaneously observed a faint gravitational-wave signal. The ripples in space-time came from a pair of two massive black holes that spiraled into each other 1.3 billion years ago.

It took scientists such a long time to arrive at the discovery because gravitational waves — even though they come from violent, powerful collisions — are extremely small once they reach Earth.

During the event detected in September 2015, scientists think that about three times the mass of the sun was transformed into gravitational waves in less than a second. [How Gravitational Waves Work (Infographic)]

The L-shaped LIGO detectors have two arms, each 2.48 miles (4 kilometers) long, with identical laser beams inside. If a gravitational wave passes through Earth, the laser in one arm of the detector will be compressed and the other will expand. But the changes are tiny— as tiny as one-thousandth of a diameter of a nucleon, said Walter Winkler, a physicist with the Max Planck Institute for Gravitational Physics in Hannover, Germany.

“You have first to keep all the distortions out and then to increase the sensitivity of the measurement system,” Winkler, who has worked on gravitational-wave detection since the 1970s, told Live Science. “It took thousands of people to come to this. It’s really a new sort of astronomy.”

The Nobel Committee acknowledged that the discovery was a huge collaborative effort. The paper announcing the September 2015 detection had more than 1,000 authors. But, according to the Nobel rules, the prize can be shared by no more than three scientists.

“Without them the discovery would not have happened,” Nils Mårtensson, chairman of the Nobel Committee for Physics, said of the three winners at the news conference in Stockholm.

Using laser beams, scientists have detected the physical distortions caused by passing gravitational waves. <a href="http://www.space.com/25445-how-ligo-lasers-hunt-gravitational-waves-infographic.html">See how the LIGO observatory hunts gravitational waves in this Space.com infographic</a>.

Using laser beams, scientists have detected the physical distortions caused by passing gravitational waves. See how the LIGO observatory hunts gravitational waves in this Space.com infographic.

Credit: By Karl Tate, Infographics Artist

Scientists here at the German Physical Society (DPG) cheered the results.

“I had really hoped for it because it’s a fantastic discovery,” DPG President Rolf-Dieter Heuer told Live Science. He added that the detection of gravitational waves opens “a window into an unseen world that will bring us more information in the future about the universe.”

The findings might seem esoteric, but Heuer said that it’s difficult to predict when and in which field this research could have practical applications. He noted that it took more than 40 years for the discovery of antimatter to be used in positron emission tomography, or PET, scans common in hospitals today.

Some had expected the LIGO team to win the prize last year. But Gunnar Ingelman, secretary of the Nobel Committee and a professor of subatomic physics at Uppsala University in Sweden, said the detection of gravitational waves was not eligible last year. According to the rules of the committee, the discovery has to be published the year before the awards are announced. (The LIGO detection was published in February 2016.)

The LIGO team has made several additional discoveries. Just last week, LIGO scientists announced they had detected gravitational waves for the fourth time, on Aug. 14, 2017. The ripples were also detected by another instrument called VIRGO, near Pisa, Italy.

“In the early days, it was not clear if these gravitational waves were real or could be observed,” Ingelman told reporters here by video. “It was an enormous effort to reach the sensitivity to build a detector which could actually observe such tiny, tiny distortions.”

Originally published on Live Science.

Earth May Be Close to ‘Threshold of Catastrophe’

Earth May Be Close to ‘Threshold of Catastrophe’
By Tia Ghose, LiveScience Staff Writer | October 2, 2017 05:25pm ET

Earth May Be Close to 'Threshold of Catastrophe'

A NASA camera on the Deep Space Climate Observatory satellite captured its first view of the entire sunlit side of the spherical planet Earth, on July 6, 2015.

Credit: NASA

The amount of carbon dioxide that humans will have released into the atmosphere by 2100 may be enough to trigger a sixth mass extinction, a new study suggests.

The huge spike in CO2 levels over the past century may put the world dangerously close to a “threshold of catastrophe,” after which environmental instability and mass die-offs become inevitable, the new mathematical analysis finds.

Even if a mass extinction is in the cards, however, it likely wouldn’t be evident immediately. Rather, the process could take 10,000 years to play out, said study co-author Daniel Rothman, a geophysicist at the Massachusetts Institute of Technology. [7 Iconic Animals Humans Are Driving to Extinction]

However, slashing carbon emissions dramatically in the coming years may also be enough to prevent such global catastrophe, said Lee Kump, a geoscientist at Pennsylvania State University who was not involved in the study.

Over Earth’s 4.5-billion-year history, life has seen a lot of boom and bust times. In the past half-billion years alone, five major extinctions have wiped out huge swaths of life: the Ordovician-Silurian mass extinction, the Late Devonian mass extinction, the Permian mass extinction, the Triassic-Jurassic mass extinction and the Cretaceous-Tertiary mass extinction that wiped out the dinosaurs. The most severe was the Permian extinction, or “The Great Dying,” when over 95 percent of marine life and 70 percent of land-based life died off.

All these major extinctions have one similarity.

“Every time there’s been a major mass extinction — one of the big five — there’s been a serious disruption of the global carbon cycle,” Rothman said. It could be a direct link between CO2 and death due ocean acidification or an indirect link, as carbon dioxide emissions can warm a planet to unlivable temperatures and have even been linked with volcanic eruptions and the related cooling of the atmosphere.

For instance, at the end of the Permian period, about 252 million years ago, ocean carbon dioxide levels skyrocketed, marine rocks reveal. (Carbon dioxide that is in the air gradually dissolves into the ocean’s surface and eventually enters the deep ocean.)  However, carbon doesn’t always equal assured doom for the planet. It’s possible that a change in carbon levels in the atmosphere and oceans are markers for rapid environmental change, which could be the underlying cause of extinctions. In addition, rocks from the past reveal many other “carbon excursions” — or rises in atmospheric or ocean levels of carbon — that did not result in mass extinctions, Rothman said. [Ocean Acidification: The Other Carbon Dioxide Threat]

So what distinguishes the deadly carbon excursions from the ones that don’t cause mass dying?

In the new study, which was published Sept. 20 in the journal Science Advances, the scientists assumed that two factors may play a role: the rate at which carbon levels increase, and the total amount of time that change is sustained, Rothman said.

To calculate those values, Rothman looked at data on carbon isotopes, or versions of the element with differing numbers of neutrons, from rock samples from 31 geologic periods over the past 540 million years. Determining the length and magnitude of rises in atmospheric carbon can be tricky because some periods have thorough rock samples while others are sparsely represented, Rothman said.

From that data, Rothman and his colleagues identified the rates of carbon change and total carbon input that seemed to be correlated to extinctions in the geologic record. Then, they extrapolated to the present day, in which humans are adding carbon to the atmosphere at a furious rate.

Rothman calculated that adding about 310 gigatons of carbon to the oceans was enough to trigger mass extinctions in the past, although there is huge uncertainty in that number, Rothman said.

“Most every scenario that’s been studied for how things will play out, as far as emissions are concerned, suggest on the order of 300 gigatons or more of carbon will be added to the oceans before the end of the century,” Rothman said.

What happens the day after that threshold is reached?

“We run the risk of a series of positive feedbacks in which mass extinction could conceivably be the result,” Rothman said.

Of course, those effects wouldn’t be felt immediately; it could take 10,000 years for the die-off to result. And there’s a lot of uncertainty in the estimates, Rothman added.

“I think it’s a really useful approach, but there are always limitations when we’re working in deep time,” Kump told Live Science. “One of the limitations is that Rothman had to accept the state of our understanding of the timing and duration of these disturbances.”

But even with that uncertainty, “clearly the rate of fossil fuel burning today rivals, if not exceeds, the rate of carbon cycle perturbation in the past” associated with mass extinctions, Kump said.

Because the rate of carbon rise is so steep currently, the best option for preventing eventual catastrophe is to ensure the duration of the carbon increase is short, he said.

“If we can rein ourselves in, we can avoid the Permian catastrophe,” Kump said.

Originally published on Live Science.

NASA to Update EM-1 Schedule in October

NASA to Update EM-1 Schedule in October
By Jeff Foust, SpaceNews Writer | September 30, 2017 07:31am ET

NASA to Update EM-1 Schedule in October

NASA will provide an update for the schedule of Exploration Mission 1, the first launch of the Space Launch System, in October.

Credit: NASA

SYDNEY — NASA plans to publish a revised launch date for the first mission of its Space Launch System in October amid reports that the flight has been pushed back to nearly the end of 2019.

In a statement to SpaceNews Sept. 22, NASA spokesperson Kathryn Hambleton said that NASA will issue an update for the scheduled launch of Exploration Mission (EM) 1 in October.

That schedule, she said, is being influenced by several issues, ranging from work on the European-provided service module for the Orion spacecraft and the impact of several weather events, including both the tornado that struck the Michoud Assembly Facility in New Orleans and Hurricanes Harvey and Irma, which shut down the Johnson Space Center in Houston and Kennedy Space Center in Florida respectively by more than a week.

“All of these factors are influencing launch planning and will result in an EM-1 mission in 2019,” she said. “An update to the agency’s target for EM-1 launch is expected in October.”

That statement came after NASASpaceFlight.com, citing internal documents, reported Sept. 22 that the launch date for EM-1 had been delayed until no earlier than Dec. 15, 2019, with EM-2, the first SLS mission to carry a crew, delayed until no earlier than June 2022.

NASA had already indicated that EM-1, originally scheduled for launch as soon as 2017, would be delayed until some time in 2019. In an April response to a U.S. Government Accountability Office report, Bill Gerstenmaier, NASA associate administrator for human exploration and operations, said that the agency was in the process of establishing a new launch date for EM-1 in 2019 after the report cited issues that threatened to delay the then-scheduled date of November 2018.

NASA confirmed those plans in May when the agency announced that it would not put a crew on EM-1 after performing a study at the request of the White House regarding that. The agency concluded that while it would be feasible to do so, there were cost, schedule and risk issues in doing so.

At that time Gerstenmaier acknowledged schedule issues, including a recent welding mishap at Michoud that damaged a liquid hydrogen tank being built for SLS qualification tests, would push EM-1 to 2019. “We’re probably a month or two away from coming up with a final schedule,” he said at the time, although the agency has not provided a schedule update since the May announcement.

At that time, Gerstenmaier also said that the EM-1 delay would also likely push back EM-2, which was then scheduled for August 2021. Part of any delay is the need to reconfigure ground systems at the Kennedy Space Center after the EM-1 launch to support the use of an upgraded version of the SLS with the more powerful Exploration Upper Stage.

This story was provided by SpaceNews, dedicated to covering all aspects of the space industry.