Home Blog Page 118

Landing on alien worlds is our highest form of exploration

0

The expression ‘We’ve landed!’ connects to something deep and instinctive in the human psyche. Those words mean that we have crossed an inhospitable expanse and staked our place on the other side. At first, the expression referred only to voyages across the ocean, then also across the sky, and now across space as well. Through all those leaps, the essential elements have remained the same: a specially built craft, a long and daunting journey, a burst of fresh danger on arrival – and a pause to celebrate merely surviving. Then comes the magical moment when we look up and cast our eyes over an unfamiliar horizon. We become a species of explorers all over again.

idea_SIZED-curiosity_sol-177bodrov600-NASA/JPL/CalTech/MSSS
NASA/JPL/CalTech/MSSS

Forty-seven years after the fact, Neil Armstrong’s message ‘Houston… the Eagle has landed’ remains one of the defining moments of the space age. Landings don’t even have to involve humans to be emotionally stirring. A robotic landing was what first drew me into planetary science and astrobiology. In 1976, while I was starting my first year of graduate school, the twin Viking probes touched down on Mars. They inspired me, far more than the earlier Mariner spacecraft that had flown past or orbited the planet. The images were both tangible and shocking: a salmon-coloured sky hanging over a rusty desert, its rocks scoured by thin, persistent winds. We were on the surface of Mars! My general interest in astronomy quickly narrowed into a specific fascination with Mars that persists to this day.

Despite their emotional power, space landings are few and far between. There are good, practical reasons for that. Landings are complex and expensive. Flybys and even orbiters are cheaper, easier and in many ways more sensible from a pure-science point of view. But NASA and the other space agencies are missing a huge opportunity here to make space exploration more evocative, and more personal. There simply is no other space vista that compares with seeing an alien horizon, capturing the perspective of an astronaut standing on another world.

After Viking, a full two decades passed before the next Mars touchdown. When the Pathfinder probe landed on Mars in the late afternoon of 4 July 1997, I was standing before a packed audience in the Stanford Theatre in Palo Alto, California. All of us were held spellbound by the first images from the lander and its little rover arriving back to Earth. Those pictures were processed in a specialty shop and projected by 35mm slides hand-carried to the theatre. Technology has changed since then, but the thrill has not. In 2012, when the two-ton Curiosity rover landed on Mars, rappelling down dramatically from a rocket-powered platform, the public response was once again immediate and intense. Thousands waited at science museums around the country to hear Curiosity’s heartbeat signal and to see the first views from the ground.

Most recently, the European Space Agency’s Philae probe made the first-ever soft landing on a comet on 12 November 2014, sending back provocative images of craggy, dust-coated cliffs. As a scientist focused on astrobiology, I have a keen interest in the organic chemistry of comets. Comets could have bought the building blocks of life to the early Earth, and might have jump-started the prebiotic reactions. But on that November day, the landing is what captured my imagination. A spindly robot bounced, tripped, tumbled and still managed to peer out on the utterly unknown surface of a comet. The science could, and did, come later.

There is an important lesson from these experiences: space missions to other worlds are not just about the science. They are about the human instinct to explore. The fascination with landing is part of that instinct. Even if the science is best served by merely orbiting or flying by, we should land whenever we can. They don’t have to be conflicting choices; often they can (and have been) done together. As for where we should land, the options are staggering. It’s been three decades since the last Venus landing; humans have only ever landed on one moon other than our own. There are many, many vistas waiting for us.

Jupiter’s large, ice-covered moon Europa is the next major target for a landing, but there has been a reluctance to commit. NASA scientists worry that the challenge is too hard, and that we have not surveyed Europa’s surface enough to find the ideal, safe landing site. Yes, there would be risks in landing there. Europa has no atmosphere in which to use parachutes. Then again, its surface gravity is similar to that of Earth’s moon, so we could use some of the technologies already developed for landing earlier robotic Moon landings. The risks of landing are similar to those of putting Pathfinder on Mars and Philae on the comet. The risks of not trying to land on Europa are more severe: we could lose the momentum for exploring this fascinating moon and searching for life in the global ocean beneath its frozen surface.

A Europa lander could be the beginning of a whole new era of space exploration. Landers don’t all have to be complex, costly machines like Curiosity. A stationary, battery-powered robot on Europa could still last long enough to survey an alien horizon unlike any seen before – our first view from the surface of an ice world. It could inspire follow-up missions to put eyes on the ground all across the solar system, so people hear the words ‘We’ve landed’ more often. There will be a rich scientific payoff but, even better, it would allow people around the world to experience other worlds from a distinctly human perspective.

I would like to volunteer as lookout with the crew that makes the first (robotic) landing on Europa. Hurray for distant lands, and for the humans and machines that land on them.

This article was originally published at Aeon and has been republished under Creative Commons.

Northrop Grumman-Built Space Sensor Satellites Launch in Support of US Space Force-8 Mission

0

Two Northrop Grumman Corporation (NYSE: NOC) Geosynchronous Space Situational Awareness Program (GSSAP) satellites were successfully launched into orbit on a United Launch Alliance (ULA) Atlas V rocket today from Cape Canaveral Space Force Station as part of the U.S. Space Force (USSF)-8 mission. The two satellites, GSSAP-5 and GSSAP-6, will enhance space situational awareness, a top priority for the U.S. Space Force. In addition to manufacturing and delivering both GSSAP payloads, Northrop Grumman also provided the sole strap-on solid rocket booster adding propulsion to the rocket launch, as well as essential aeronautical components in support of the USSF-8 launch.  

Northrop Grumman-built GSSAP satellites collect space situational awareness data allowing for more accurate tracking and characterization of man-made orbiting objects.
Northrop Grumman-built GSSAP satellites collect space situational awareness data allowing for more accurate tracking and characterization of man-made orbiting objects.

The GSSAP program delivers a space-based capability operating in a near-geosynchronous Earth orbit (GEO), in support of the U.S. Space Command space surveillance operations. GSSAP satellites allow for more accurate tracking and characterization of orbiting objects and uniquely contribute to timely and precise orbital predictions, enhancing knowledge of the GEO environment and improving spaceflight safety. Northrop Grumman has manufactured all GSSAP satellites since the program’s inception in 2011.

“For over a decade, Northrop Grumman has delivered products that improve U.S. Space Command’s ability to monitor human-made orbiting objects in the geosynchronous environment,” said Matt Verock, vice president, space security, Northrop Grumman. “As dedicated Space Surveillance Network (SSN) sensors, the capabilities our GSSAP satellites bring demonstrate our leadership in space domain awareness.”

The company’s facilities in Dulles, Virginia along with Goleta and San Diego, California, and Beltsville, Maryland provided numerous subsystems, including the satellite’s solar arrays, primary structure, thermal control, avionic boxes, flight computer, shunt regulator assembly, composite components and deployable structures.   

This was the third ULA Atlas V rocket launch supported by Northrop Grumman’s 63-inch-diameter Graphite Epoxy Motor (GEM 63). The GEM 63 solid rocket booster, manufactured at the company’s Magna, Utah facility, provided nearly a third of the total thrust at liftoff. The GEM family of solid rocket motors recently expanded with the development of the GEM 63XL variation to support ULA’s Vulcan Centaur launch vehicle, scheduled for its first flight later this year.

The company manufactured the Atlas V rocket’s reaction control system propellant tanks at its Commerce, California, facility, and eight retro motors at its Elkton, Maryland, facility that assist first and second stage separation. Using advanced fiber placement manufacturing and automated inspection techniques, Northrop Grumman produced the composite heat shield that provides essential protection to the Atlas V first-stage engine, the Centaur Interstage Adapter that houses the second-stage engine, and the broadtail that adapts from the core vehicle to the five-meter diameter fairing. Northrop Grumman fabricated these structures at its Iuka, Mississippi, facility.

Northrop Grumman is a technology company, focused on global security and human discovery. Our pioneering solutions equip our customers with capabilities they need to connect, advance and protect the U.S. and its allies. Driven by a shared purpose to solve our customers’ toughest problems, our 90,000 employees define possible every day.

NASA to Discuss Webb’s Arrival at Final Destination, Next Steps

0

Scientists and engineers operating NASA’s James Webb Space Telescope will answer questions about the mission’s latest milestones in a NASA Science Live broadcast at 3 p.m. EST Monday, Jan. 24, followed by a media teleconference at 4 p.m.

The broadcast will air live online on the NASA Science Live website, as well as YouTubeFacebook, and Twitter. Audio of the teleconference will stream live on the agency’s website.

This artist’s conception shows the fully unfolded James Webb Space Telescope in space. Credits: Adriana Manrique Gutierrez, NASA Animator
This artist’s conception shows the fully unfolded James Webb Space Telescope in space. Credits: Adriana Manrique Gutierrez, NASA Animator

Ground teams plan to fire Webb’s thrusters at 2 p.m. Monday, Jan. 24 to insert the space telescope into orbit around the Sun at the second Lagrange point, or L2, its intended destination, nearly 1 million miles from Earth. This mid-course correction burn has long been planned for approximately 29 days after launch. This week, the mission operations team selected the target date and time for the burn. Engineers also finished remotely moving Webb’s mirror segments out of their launch positions to begin the months-long process of aligning the telescope’s optics.

Viewers of this episode, “What’s Next for the James Webb Space Telescope?” can submit questions on social media using the hashtag #UnfoldtheUniverse or by leaving a comment in the chat section of the Facebook or YouTube stream. Questions from the public will be answered by:

  • Amber Straughn, deputy project scientist for Webb communications, NASA’s Goddard Space Flight Center in Greenbelt, Maryland
  • Scarlin Hernandez, flight systems engineer, Space Telescope Science Institute in Baltimore

Following the episode, NASA will host a media teleconference focused on the L2 insertion burn and mirror movements, as well as the next steps in preparing Webb to conduct science. The call will feature:

  • Lee Feinberg, Webb optical telescope element manager, Goddard
  • Amy Lo, Webb vehicle engineering lead, Northrop Grumman
  • Keith Parrish, Webb observatory commissioning manager, Goddard
  • Jane Rigby, Webb operations project scientist, Goddard

To participate in the teleconference, media must RSVP no later than two hours prior to the event to Laura Betz at: [email protected]. NASA’s media accreditation policy for virtual activities is available online.

Webb, an international partnership with the ESA (European Space Agency) and the Canadian Space Agency, launched Dec. 25 from Europe’s Spaceport in Kourou, French Guiana. On Jan. 8, Webb finished unfolding in space after having been stowed inside the nose cone of an Arianespace Ariane 5 rocket for launch.

The observatory is now preparing for science operations, a human-controlled process called commissioning that provides the team with the flexibility to pause and adjust as needed. NASA provides regular updates about commissioning milestones on the Webb telescope blog. The public also can follow Webb’s progress online via a “Where is Webb?” interactive tracker.

Webb will explore every phase of cosmic history – from within the solar system to the most distant observable galaxies in the early universe, and everything in between. Webb will reveal new and unexpected discoveries and help humanity understand the origins of the universe and our place in it.

One Year into the Biden Administration, NASA Looks to Future

0

Over the past year, NASA has made valuable contributions to Biden-Harris Administration’s goals – leading on the global stage, addressing the urgent issue of climate change, creating high paying jobs, and inspiring future generations.

“Since President Biden and Vice President Harris were sworn in one year ago, their administration has made generational progress for Americans – and made NASA a priority. This spring, as Artemis I lifts off from Kennedy Space Center, the world will once again witness America’s unrivaled ingenuity and inspiration as NASA prepares the next generation to return to the Moon and on to Mars,” said NASA Administrator Bill Nelson. “I am proud of the work the agency has done to support this administration’s priorities on climate change, global leadership, diversity, equity, STEM education, and so much more. And we all should look forward to an even more robust future as NASA continues to explore the heavens and benefit life here on Earth.”

Vice President Kamala Harris delivers opening remarks at the first meeting of the National Space Council, Wednesday, Dec. 1, 2021, at the United States Institute of Peace in Washington. Credits: NASA/Joel Kowsky
Vice President Kamala Harris delivers opening remarks at the first meeting of the National Space Council, Wednesday, Dec. 1, 2021, at the United States Institute of Peace in Washington. Credits: NASA/Joel Kowsky

Highlights of NASA’s efforts are below.

NASA Missions:

Since its inception, NASA has led the world in space, both in human spaceflight and science.

Mars: Perseverance and Ingenuity

  • The Perseverance Mars rover landed on the Red Planet in February 2021 where it is studying the rock and sediment in Mars’ Jezero Crater and aiding in the search for signs of ancient microbial life.
  • Perseverance collected its first rock core into its sampling tube. The core is enclosed in a sample tube, and available for retrieval on a future Mars Sample Return mission.
  • Ingenuity became the first aircraft to make a powered, controlled flight on another planet, successfully logging 18 flights and completing more than 30 minutes of cumulative flight time.
  • Perseverance, first funded and approved under the Obama-Biden Administration, is made possible by thousands of scientists and engineers from countries and organizations around the world.

James Webb Space Telescope

  • Webb launched from Kourou, French Guiana Dec. 25th, in partnership with the European and Canadian space agencies.
  • In an incredible feat of engineering, the team has successfully completed the most critical and complex deployments, and the spacecraft now is on its way to its future home, nearly a million miles from Earth.
    • Webb will explore a wide range of science questions to help us understand the origins of the universe and our place within it. It will peer back to reveal the first stars and galaxies that formed about 13.5 billion years ago in the aftermath of the Big Bang.

International Space Station Extension

  • The Biden-Harris Administration has announced its commitment to extend International Space Station operations through 2030, and to work with our international partners in Europe (European Space Agency), Japan (Japan Aerospace Exploration Agency), Canada (Canadian Space Agency), and Russia (State Space Corporation Roscosmos) to enable continuation of the groundbreaking research being conducted in this unique orbiting laboratory through the rest of this decade.
  • Over the past two decades, the United States has maintained a continuous human presence in orbit around the Earth to test technologies, conduct scientific research, and develop skills needed to explore farther than ever before. The unique microgravity laboratory has hosted more than 3,000 research investigations from over 4,200 researchers across the world and is returning enormous scientific, educational, and technological developments to benefit people on Earth.

Humans in Space: NASA’s Commercial Crew Program, Astronaut Candidate Announcement

  • NASA and SpaceX successfully launched eight astronauts to the International Space Station in 2021. NASA’s Commercial Crew Program, a cornerstone of private-public partnership passed into law under the Obama-Biden administration, has brought value to the American taxpayer and enabled incredible growth in the commercial space sector, all while providing safe, reliable transportation to the space station on American rockets from American soil.
  • Nelson introduced the members of the 2021 astronaut class, the first new class in four years Dec. 6 at  NASA’s Johnson Space Center in Houston. Ten new astronaut candidates were selected from more than 12,000 applicants. The astronaut candidates recently began two years of training at Johnson and have the potential to walk on the Moon as part of Artemis.

Double Asteroid Redirection Test (DART)

  • DART, the world’s first full-scale mission to test technology for defending Earth against potential asteroid or comet hazards, launched in November.
  • DART will test whether a spacecraft can autonomously navigate to a target asteroid and intentionally collide with it in a method of deflection called kinetic impact.
    • The test in the fall of 2022 will provide important data to help better prepare for an asteroid that might pose an impact hazard to Earth, should one ever be discovered.

Moon to Mars

  • NASA took critical steps in 2021 to prepare for the historic launch of Artemis I, an uncrewed flight test of NASA’s powerful Space Launch System (SLS) rocket and Orion spacecraft in spring 2022, including the green run engine test and completing assembly of SLS and Orion for the first time.
    • NASA will land the first woman and person of color on the Moon as part of the Artemis program – missions that will help the agency in preparation for human exploration of Mars.
    • SLS is the most powerful rocket in the world – and the only rocket that can send Orion, astronauts, and supplies 239,000 miles to the Moon in a single mission.

Addressing Climate Change and Natural Disasters:

NASA unequivocally provides the most comprehensive data in the world on the Earth’s systems and is the only space agency in the world providing end-to-end research on our home planet to analyze and understand the processes involved.  

National Climate Task Force

  • NASA joined the National Climate Task Force established by President Biden and released a climate action plan aimed at averting mission impacts due to climate change, ensuring the resiliency of facilities and assets, and providing the nation and world unique climate observations, analysis, and modeling through scientific research.

Senior Climate Advisor

  • NASA established the new position of senior climate advisor to the administrator to ensure effective fulfillment of the Biden Administration’s climate science objectives for NASA. In January, NASA hired Dr. Katherine Calvin to serve a dual role as both the climate advisor and agency’s chief scientist.

Earth System Observatory

  • NASA announced a new Earth System Observatory, five integrated satellites that will provide key information to help mitigate and guide efforts related to climate change, disaster mitigation, fighting forest fires, and improve real-time agricultural processes.

Landsat 9

  • In September, NASA and United States Geological Survey launched Landsat 9, an Earth-observing satellite that will build on the most advanced measurements made in the program’s history.
  • The Landsat Program represents the longest, continuous, global satellite record of the Earth’s surface, allowing us to track the impacts of climate change.
  • These satellites have documented Earth’s changing landscape, helping farmers and scientists understand and manage land resources needed to sustain human life, like food, water, and forests.

INCUS

  • NASA selected a new Earth science mission that will study the behavior of tropical storms and thunderstorms, including their impacts on weather and climate models.
  • The mission will be a collection of three SmallSats, flying in tight coordination, called Investigation of Convective Updrafts (INCUS), and is expected to launch in 2027 as part of NASA’s Earth Venture Program.
  • INCUS fills an important niche to help understand extreme weather and its impact on climate models – all of which serves to provide crucial information needed to mitigate weather and climate effects on our communities.

TROPICS

  • To bring more data to forecasters and have a more consistent watch over Earth’s tropical belt where these storms form, NASA launched a test satellite, or pathfinder, ahead of a constellation of six weather satellites called TROPICS (Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsats).
  • Planned for launch in 2022, the TROPICS satellites will work together to provide near-hourly microwave observations of a storm’s precipitation, temperature, and humidity – a revisit time for these measurements not currently possible with other satellites.

National Space Council:

Vice President Kamala Harris Chairs First National Space Council Meeting

  • The vice president leads the National Space Council, and she announced a new, whole-of-government framework to ensuring that space activities create opportunities that benefit the American people and the world, and enhances our ability to maintain a vibrant space sector across civilian, commercial, and national security.
  • The Vice President charged the Council with an initial focus on the rules and norms governing space, leveraging space to tackle the climate crisis, and building a diverse space and STEM workforce.
  • In conjunction with the Vice President leading her first National Space Council meeting, President Biden also signed a new Executive Order that addresses the membership, duties, and responsibilities of the Council. The Order added five new members to the Council: The Secretaries of Education, Labor, Agriculture, and the Interior, as well as the National Climate Advisor. These new members demonstrate the Administration’s emphasis on ensuring the benefits of American space activities are applied broadly throughout society and employed to solve the toughest challenges, including addressing the climate crisis and building a vibrant workforce for the future.
  • At the meeting, Nelson highlighted the breadth of NASA’s STEM engagement, from the more than 6,400 internships, fellowships, and other direct student higher education awards, to the $35 million in direct financial support to students enrolled in higher education programs.

Vice President Harris Tours NASA’s Goddard Space Flight Center

  • During the visit, the Vice President got a first-hand look at NASA’s Earth science missions and presented the first images from the Landsat 9 satellite.
  • While chairing her first National Space Council meeting, she highlighted the opportunities that the aerospace sector offers – for science, the economy, national competitiveness, STEM education, and more.

International Collaboration:

NASA is a global leader in space and here on Earth. International partnerships play a key role in achieving mission success – from collaboration on climate, to planetary science, and human exploration.

Ukrainian President Visits with NASA Administrator

  • Ukrainian President Volodymyr Zelenskyy met with NASA Administrator Bill Nelson at the Mary W. Jackson NASA Headquarters in Washington.
  • They two discussed a renewed commitment to partnership in space, shared interest in exploration and discovery, and the importance of international cooperation for achieving mutual ambitions in space.

Artemis Accords

  • Several nations joined a growing list of countries in signing the Artemis Accords, principles that will help establish a safe, peaceful, and prosperous future in space.

COP26

  • NASA expanded its presence at COP26, a global summit brings parties together to accelerate action towards the goals of the Paris Agreement and the U.N. Framework Convention on Climate Change. The NASA Hyperwall served as the main attraction at the U.S. Center.

Partnered with ESA on Climate

  • Formed a strategic, first-of-its-kind partnership with ESA to observe Earth and its changing environment.
  • The partnership was formalized through a joint statement of intent, signed Tuesday, which outlines how the agencies will collaborate to ensure continuity of Earth observations; advance understanding of the Earth System, climate change and application of that knowledge; and collaborate on an open data policy that promotes open sharing of data, information, and knowledge within the scientific community and the wider public.

Lead Multilateral Meeting with Nearly 30 Space Agencies

  • Hosted a multilateral event with nearly 30 space agencies around the world at the International Aeronautical Congress to discuss the future of space exploration and underscore the importance of the safe, sustainable use of outer space.

Diversity, Equity, Inclusion and Accessibility:

NASA is entirely committed to the full participation and empowerment of a wide variety of people, organizations, capabilities, and assets because we know this best enables the workforce to accomplish our missions.

Mission Equity

  • In response to Executive Order 13985 (Advancing Racial Equity and Support for Underserved Communities Through the Federal Government), NASA rolled out “Mission Equity,” held a public meeting to solicit feedback, and is reviewing public comments to a request for information.
  • Mission Equity is a comprehensive effort to assess agency programs, procurements, grants, and policies, and examine what potential barriers and challenges may exist for communities that are historically underrepresented and underserved.

NASA Headquarters Officially Named for Mary W. Jackson

  • NASA celebrated the agency’s first African American female engineer, Mary W. Jackson, with a ceremony to formally name the agency’s headquarters building in Washington in her honor.

Dual Anonymous Science Grant Proposal System

  • NASA is experimenting with changing its science grant proposal system to a dual anonymous system – one where names of reviewers and proposers are both kept hidden – which has been proven to increase fairness and reduce hidden biases for research awards. 
  • NASA has pilot programs underway and used this method to choose the recently announced set of first research projects for the James Webb Space Telescope.

STEM Education:

NASA STEM education and engagement is critical to our nation’s goal of building a diverse future STEM workforce and engages students in authentic learning experiences that spark interest and provide connections to NASA’s missions.

NASA 2021 STEM-a-Thon

  • NASA hosted STEM-a-Thon with a series of activities and engagements for students with more than 6,600 registrants from across the globe. NASA’s STEM-a-Thon is aimed at sparking interest in careers and broadening student participation in STEM. This year’s event highlighted paths to careers at NASA and encouraged students to pursue their interests in STEM.

NASA’s Minority University Research and Education Project (MUREP)

  • NASA awarded grants to MSIs to support Artemis Space Technology. $3.5 million will be distributed to selected universities over two years. NASA’s MUREP called upon Minority Serving Institutions to develop proposals for how they could use NASA funding to strengthen their support for underrepresented communities.
  • NASA chose six MSIs to receive the MUREP INCLUDES award. Each award provides up to $1.2 million for a three-year period to implement the institution’s proposal.

EPSCoR

  • In fiscal year 2021, NASA’s Established Program to Stimulate Competitive Research (EPSCoR) conducted five competitive awards processes aimed toward increasing research and development capacity and improvement, while enabling valuable contributions to NASA mission needs and challenges. These five competitive solicitations yielded 94 selected proposals for a total of over $45 million in awards to institutions. 

Space Grant

  • In fiscal year 2021, Space Grant awarded $42 million in cooperative agreements to institutions in all 50 states, Washington DC & Puerto Rico, resulting in over 3,700 Significant Student awards.  FY21 also saw the expansion of the Space Grant Consortia to include over 1,100 partner institutions throughout Academia, Industry, State/Local Government, and non-profit organizations. 
  • In addition to direct awards made to Higher Education students, the program had over 193,000 student participants, 16,700 faculty participants, and over 400 peer-reviewed manuscripts with another 180 pending.

Next Gen STEM

  • In FY21, Next Gen STEM, OSTEM’s K-12 project, reached 467,805 students and 35,562 educators through various events, activities and STEM learning.

Million Girls Moonshot

  • NASA partnered with Million Girls Moonshot’s Reach for the Stars Downlink Event, part of the Million Girls Moonshot, a five-year partnership designed to cultivate an engineering mindset within one million girls by 2025. Over 24,000 students registered for the event.

Internships

  • NASA nearly doubled the number of participants in its internship program over the fiscal year, and both the fall and spring intern cohorts were NASA’s largest to date for those sessions.

Statistics:

  • NASA activities supported more than $60 billion in total economic output and supported more than 300,000 jobs nationwide.
  • NASA grew the agency’s social media following to 277 million in 2021 – up 14% from 240 million in 2020.
  • 4.2 million viewers watched live as Perseverance landed on Mars. Currently, the landing broadcast is the most-watched video of all time on NASA’s YouTube channel with almost 24 million views.
  • NASA also conducted its first live Spanish language broadcast for the Mars Perseverance landing, which received more than 2.6 million views.
  • More than 1 million students participated in NASA’s Mission to Mars Student Challenge.
  • More than 7.7 million viewers tuned into the launch of the James Webb Space Telescope. The launch broadcast is now among the top 20 videos of all time on NASA’s flagship channel. 
  • The YouTube NASA en español broadcast of the Webb Telescope launch, “Desplegando el universo,” reached 465,000 views.

Hubble Finds A Black Hole Igniting Star Formation In A Dwarf Galaxy

0

Dwarf galaxy Henize 2-10 continues to make a big impact, defying astronomers’ expectations

Black holes are often described as the monsters of the universe—tearing apart stars, consuming anything that comes too close, and holding light captive. Detailed evidence from NASA’s Hubble Space Telescope, however, shows a black hole in a new light: fostering, rather than suppressing, star formation. Hubble imaging and spectroscopy of the dwarf starburst galaxy Henize 2-10 clearly show a gas outflow stretching from the black hole to a bright star birth region like an umbilical cord, triggering the already dense cloud into forming clusters of stars. Astronomers have previously debated that a dwarf galaxy could have a black hole analogous to the supermassive black holes in larger galaxies. Further study of dwarf galaxies, which have remained small over cosmic time, may shed light on the question of how the first seeds of supermassive black holes formed and evolved over the history of the universe.


Often portrayed as destructive monsters that hold light captive, black holes take on a less villainous role in the latest research from NASA’s Hubble Space Telescope. A black hole at the heart of the dwarf galaxy Henize 2-10 is creating stars rather than gobbling them up. The black hole is apparently contributing to the firestorm of new star formation taking place in the galaxy. The dwarf galaxy lies 30 million light-years away, in the southern constellation Pyxis.

A decade ago this small galaxy set off debate among astronomers as to whether dwarf galaxies were home to black holes proportional to the supermassive behemoths found in the hearts of larger galaxies. This new discovery has little Henize 2-10, containing only one-tenth the number of stars found in our Milky Way, poised to play a big part in solving the mystery of where supermassive black holes came from in the first place.

A pullout of the central region dwarf starburst galaxy Henize 2-10 traces an outflow, or bridge of hot gas 230 light-years long, connecting the galaxy’s massive black hole and a star-forming region. Hubble data on the velocity of the outflow from the black hole, as well as the age of the young stars, indicates a causal relationship between the two. A few million years ago, the outflow of hot gas slammed into the dense cloud of a stellar nursery and spread out, like water from a hose impacting a mound of dirt. Now clusters of young stars are aligned perpendicular to the outflow, revealing the path of its spread. Image credits: CREDITS: SCIENCE: NASA, ESA, Zachary Schutte (XGI), Amy Reines (XGI), Alyssa Pagan (STScI)
A pullout of the central region dwarf starburst galaxy Henize 2-10 traces an outflow, or bridge of hot gas 230 light-years long, connecting the galaxy’s massive black hole and a star-forming region. Hubble data on the velocity of the outflow from the black hole, as well as the age of the young stars, indicates a causal relationship between the two. A few million years ago, the outflow of hot gas slammed into the dense cloud of a stellar nursery and spread out, like water from a hose impacting a mound of dirt. Now clusters of young stars are aligned perpendicular to the outflow, revealing the path of its spread. Image credits: NASA, ESA, Zachary Schutte (XGI), Amy Reines (XGI), Alyssa Pagan (STScI)

“Ten years ago, as a graduate student thinking I would spend my career on star formation, I looked at the data from Henize 2-10 and everything changed,” said Amy Reines, who published the first evidence for a black hole in the galaxy in 2011 and is the principal investigator on the new Hubble observations, published in the January 19 issue of Nature

“From the beginning I knew something unusual and special was happening in Henize 2-10, and now Hubble has provided a very clear picture of the connection between the black hole and a neighboring star forming region located 230 light-years from the black hole,” Reines said.

That connection is an outflow of gas stretching across space like an umbilical cord to a bright stellar nursery. The region was already home to a dense cocoon of gas when the low-velocity outflow arrived. Hubble spectroscopy shows the outflow was moving about 1 million miles per hour, slamming into the dense gas like a garden hose hitting a pile of dirt and spreading out. Newborn star clusters dot the path of the outflow’s spread, their ages also calculated by Hubble.

This is the opposite effect of what’s seen in larger galaxies, where material falling toward the black hole is whisked away by surrounding magnetic fields, forming blazing jets of plasma moving at close to the speed of light. Gas clouds caught in the jets’ path would be heated far beyond their ability to cool back down and form stars. But with the less-massive black hole in Henize 2-10, and its gentler outflow, gas was compressed just enough to precipitate new star formation.

Dwarf starburst galaxy Henize 2-10 sparkles with young stars in this Hubble visible-light image. The bright region at the center, surrounded by pink clouds and dark dust lanes, indicates the location of the galaxy’s massive black hole and active stellar nurseries. Image credit: NASA, ESA, Zachary Schutte (XGI), Amy Reines (XGI), Alyssa Pagan (STScI)
Dwarf starburst galaxy Henize 2-10 sparkles with young stars in this Hubble visible-light image. The bright region at the center, surrounded by pink clouds and dark dust lanes, indicates the location of the galaxy’s massive black hole and active stellar nurseries. Image credit: NASA, ESA, Zachary Schutte (XGI), Amy Reines (XGI), Alyssa Pagan (STScI)

“At only 30 million light-years away, Henize 2-10 is close enough that Hubble was able to capture both images and spectroscopic evidence of a black hole outflow very clearly. The additional surprise was that, rather than suppressing star formation, the outflow was triggering the birth of new stars,” said Zachary Schutte, Reines’ graduate student and lead author of the new study.

Ever since her first discovery of distinctive radio and X-ray emissions in Henize 2-10, Reines has thought they likely came from a massive black hole, but not as supermassive as those seen in larger galaxies. Other astronomers, however, thought that the radiation was more likely being emitted by a supernova remnant, which would be a familiar occurrence in a galaxy that is rapidly pumping out massive stars that quickly explode.

“Hubble’s amazing resolution clearly shows a corkscrew-like pattern in the velocities of the gas, which we can fit to the model of a precessing, or wobbling, outflow from a black hole. A supernova remnant would not have that pattern, and so it is effectively our smoking-gun proof that this is a black hole,” Reines said.

Reines expects that even more research will be directed at dwarf galaxy black holes in the future, with the aim of using them as clues to the mystery of how supermassive black holes came to be in the early universe. It’s a persistent puzzle for astronomers. The relationship between the mass of the galaxy and its black hole can provide clues. The black hole in Henize 2-10 is around 1 million solar masses. In larger galaxies, black holes can be more than 1 billion times our Sun’s mass. The more massive the host galaxy, the more massive the central black hole.

Current theories on the origin of supermassive black holes break down into three categories: 1) they formed just like smaller stellar-mass black holes, from the implosion of stars, and somehow gathered enough material to grow supermassive, 2) special conditions in the early universe allowed for the formation of supermassive stars, which collapsed to form massive black hole “seeds” right off the bat, or 3) the seeds of future supermassive black holes were born in dense star clusters, where the cluster’s overall mass would have been enough to somehow create them from gravitational collapse.

So far, none of these black hole seeding theories has taken the lead. Dwarf galaxies like Henize 2-10 offer promising potential clues, because they have remained small over cosmic time, rather than undergoing the growth and mergers of large galaxies like the Milky Way. Astronomers think that dwarf galaxy black holes could serve as an analog for black holes in the early universe, when they were just beginning to form and grow.

“The era of the first black holes is not something that we have been able to see, so it really has become the big question: where did they come from? Dwarf galaxies may retain some memory of the black hole seeding scenario that has otherwise been lost to time and space,” Reines said.

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 in Washington, D.C.

Our Universe is too vast for even the most imaginative sci-fi

0

As an astrophysicist, I am always struck by the fact that even the wildest science-fiction stories tend to be distinctly human in character. No matter how exotic the locale or how unusual the scientific concepts, most science fiction ends up being about quintessentially human (or human-like) interactions, problems, foibles and challenges. This is what we respond to; it is what we can best understand. In practice, this means that most science fiction takes place in relatively relatable settings, on a planet or spacecraft. The real challenge is to tie the story to human emotions, and human sizes and timescales, while still capturing the enormous scales of the Universe itself.

Relative positions of distant spacecraft. Courtesy NASA/JPL-Caltech
Relative positions of distant spacecraft. Courtesy NASA/JPL-Caltech

Just how large the Universe actually is never fails to boggle the mind. We say that the observable Universe extends for tens of billions of light years, but the only way to really comprehend this, as humans, is to break matters down into a series of steps, starting with our visceral understanding of the size of the Earth. A non-stop flight from Dubai to San Francisco covers a distance of about 8,000 miles – roughly equal to the diameter of the Earth. The Sun is much bigger; its diameter is just over 100 times Earth’s. And the distance between the Earth and the Sun is about 100 times larger than that, close to 100 million miles. This distance, the radius of the Earth’s orbit around the Sun, is a fundamental measure in astronomy; the Astronomical Unit, or AU. The spacecraft Voyager 1, for example, launched in 1977 and, travelling at 11 miles per second, is now 137 AU from the Sun.

But the stars are far more distant than this. The nearest, Proxima Centauri, is about 270,000 AU, or 4.25 light years away. You would have to line up 30 million Suns to span the gap between the Sun and Proxima Centauri. The Vogons in Douglas Adams’s The Hitchhiker’s Guide to the Galaxy (1979) are shocked that humans have not travelled to the Proxima Centauri system to see the Earth’s demolition notice; the joke is just how impossibly large the distance is.

Four light years turns out to be about the average distance between stars in the Milky Way Galaxy, of which the Sun is a member. That is a lot of empty space! The Milky Way contains about 300 billion stars, in a vast structure roughly 100,000 light years in diameter. One of the truly exciting discoveries of the past two decades is that our Sun is far from unique in hosting a retinue of planets: evidence shows that the majority of Sun-like stars in the Milky Way have planets orbiting them, many with a size and distance from their parent star allowing them to host life as we know it.

Yet getting to these planets is another matter entirely: Voyager 1 would arrive at Proxima Centauri in 75,000 years if it were travelling in the right direction – which it isn’t. Science-fiction writers use a variety of tricks to span these interstellar distances: putting their passengers into states of suspended animation during the long voyages, or travelling close to the speed of light (to take advantage of the time dilation predicted in Albert Einstein’s theory of special relativity). Or they invoke warp drives, wormholes or other as-yet undiscovered phenomena.

When astronomers made the first definitive measurements of the scale of our Galaxy a century ago, they were overwhelmed by the size of the Universe they had mapped. Initially, there was great skepticism that the so-called ‘spiral nebulae’ seen in deep photographs of the sky were in fact ‘island universes’ – structures as large as the Milky Way, but at much larger distances still. While the vast majority of science-fiction stories stay within our Milky Way, much of the story of the past 100 years of astronomy has been the discovery of just how much larger than that the Universe is. Our nearest galactic neighbour is about 2 million light years away, while the light from the most distant galaxies our telescopes can see has been travelling to us for most of the age of the Universe, about 13 billion years.

We discovered in the 1920s that the Universe has been expanding since the Big Bang. But about 20 years ago, astronomers found that this expansion was speeding up, driven by a force whose physical nature we do not understand, but to which we give the stop-gap name of ‘dark energy’. Dark energy operates on length- and time-scales of the Universe as a whole: how could we capture such a concept in a piece of fiction?

The story doesn’t stop there. We can’t see galaxies from those parts of the Universe for which there hasn’t been enough time since the Big Bang for the light to reach us. What lies beyond the observable bounds of the Universe? Our simplest cosmological models suggest that the Universe is uniform in its properties on the largest scales, and extends forever. A variant idea says that the Big Bang that birthed our Universe is only one of a (possibly infinite) number of such explosions, and that the resulting ‘multiverse’ has an extent utterly beyond our comprehension.

The US astronomer Neil deGrasse Tyson once said: ‘The Universe is under no obligation to make sense to you.’ Similarly, the wonders of the Universe are under no obligation to make it easy for science-fiction writers to tell stories about them. The Universe is mostly empty space, and the distances between stars in galaxies, and between galaxies in the Universe, are incomprehensibly vast on human scales. Capturing the true scale of the Universe, while somehow tying it to human endeavours and emotions, is a daunting challenge for any science-fiction writer. Olaf Stapledon took up that challenge in his novel Star Maker (1937), in which the stars and nebulae, and cosmos as a whole, are conscious. While we are humbled by our tiny size relative to the cosmos, our brains can none the less comprehend, to some extent, just how large the Universe we inhabit is. This is hopeful, since, as the astrobiologist Caleb Scharf of Columbia University has said: ‘In a finite world, a cosmic perspective isn’t a luxury, it is a necessity.’ Conveying this to the public is the real challenge faced by astronomers and science-fiction writers alike.

Welcome to the Universe: An Astrophysical Tour by Michael Strauss, Neil deGrasse Tyson and J Richard Gott is out now through Princeton University Press.

This article was originally published at Aeon and has been republished under Creative Commons.

Leading space innovator ClearSpace opens for business in the UK

0

ClearSpace, the innovative Swiss start-up with mission to make the booming commercial space economy more sustainable, affordable and resilient, has announced the formation of a UK subsidiary, its first significant engineering presence outside of Switzerland. The new ClearSpace facility has the potential to create more than 20 high-skill jobs as part of the company’s drive to deliver a wide range of in-orbit services, including orbital debris removal, in-orbit transport, and satellite life extension.

Since its formation in 2018, ClearSpace has innovated rapidly and has recently signed an €86.2M in-orbit service contract with the European Space Agency to remove orbital debris, the first step in cleaning up Space for future generations. The formation of ClearSpace Today Ltd will allow critical parts of that ClearSpace-1 Mission, and other future commercial missions, to be developed in the UK.

The ClearSpace-1 satellite (left) docking with a piece of space debris (right), before safely removing it from orbit. Image credit: ClearSpace SA.
The ClearSpace-1 satellite (left) docking with a piece of space debris (right), before safely removing it from orbit. Image credit: ClearSpace SA.

ClearSpace’s UK lead Rory Holmes said:
“We are thrilled to be part of the thriving UK space ecosystem and are excited to build our engineering presence here, tapping into the highly-relevant experience that exists within the high-tech talent pool and the local industry.
“We are very grateful for the invaluable support provided by the UK Space Agency and the Department for International Trade throughout the setup of our UK subsidiary.”

The UK is Europe’s largest contributor to ESA projects to remove debris from Space. Science Minister Amanda Solloway said:
“I want the UK to be the destination of choice for the world’s most enterprising space companies, and it is brilliant news that ClearSpace has chosen to carry out its world-leading work here.
“This ambitious project to clean up space will help create highly skilled jobs for the UK’s thriving space sector while ensuring that the scientific and commercial exploration of space remains sustainable for generations to come.”

Minister for Investment Gerry Grimstone said:
“I welcome Clearspace to the UK’s dynamic and cutting-edge space industry where they will be able to carry out their important work to remove orbital debris.”
“Space will increasingly play a role in growing UK prosperity through high skilled jobs and investment in R&D, providing solutions to some of our shared global problems. I am excited to see how Clearspace, through developing their UK capability, will be a key part of addressing these.”

ClearSpace CEO and co-founder Luc Piguet said:
“Space sustainability and resilient operations is a challenge at the global scale – now is the time to build capabilities that will make our space operations more sustainable and affordable. We need to ambitiously grow space activities while safeguarding this precious environment for future generations.”
“We are enthusiastic to expand our team in the UK to develop key enabling technologies and to foster robust partnerships with other forward-thinking companies and organizations.”

ClearSpace-1 will be the first space mission to remove an item of debris from orbit, planned for launch in 2025. UK Space Agency International Director Alice Bunn said:
“Space represents the future of our economy, but we must make use of it sustainably. With thousands of pieces of space debris, including defunct satellites, rocket bodies and launch adapters remaining in orbit, the need for new techniques and technologies to remove them could not be greater.
“We want UK to be the best place for space and are committed to delivering access to skills, investment, and regulatory reform to make that happen.”


About ClearSpace

ClearSpace SA, a Swiss start-up founded in Lausanne in 2018, brings together space experts including astronauts, engineers and researchers from all over the world at EPFL (Ecole Polytechnique Fédérale Lausanne). They aim to harness their respective talents to clean up space debris and build the future of in-orbit services. The team of experts were originally hired for an academic mission to bring down SwissCube, a cubesat launched in 2009 by EPFL, but they left the University in 2012 to focus on ClearSpace-1, their mission for the European Space Agency (ESA). On 13 November 2020, ClearSpace signed a contract worth 86 million euros with ESA to send their first robot cleaner into space in 2025.

What high-speed astronomy can tell us about the galactic zoo

0

For most of human history, the distant ‘celestial sphere’ was regarded as perfect and unchanging. Stars remained in place, planets moved predictably, and the few rogue comets were viewed as atmospheric phenomena. This began to change with the Danish astronomer Tycho Brahe’s observation of the supernova of 1572 – apparently, a new star – and his studies of the Great Comet of 1577, which he proved was actually a distant object. Nonetheless, the impression of permanence is strong. There are very few astronomical objects that noticeably vary to the naked eye: only the brightest comets, novae and supernovae. For observers in the northern hemisphere, the last naked-eye supernova was in 1604.

Modern telescopic studies tell a quite different story. Today, we know of roughly a half-million variable stars in our galaxy, and identify thousands of transient objects each year. Although many stars vary in predictable ways, the Universe is also full of unpredictable violence. When two stars orbit close to each other, mass can flow from one to the other. If one of the stars is an old, collapsed white dwarf, the gas it pulls from its companion can accumulate until the dwarf undergoes a sudden thermonuclear explosion – a supernova like the one seen by Tycho. There is also another, more common type of supernova produced by the deaths of solitary stars more than about 10 times the mass of the Sun.

Supernovae show a broad range of behaviours that depend on the detailed properties of the system at the time of the final, fatal cataclysm. The atoms that emerge from supernova explosions have provided the raw material for all planets, including our own. Astronomers are understandably eager to learn more about them, but the two classes of supernovae combined happen only about once per century in our galaxy.

Obviously, for events occurring on time scales of a century, searching for them in our galaxy alone is not terribly profitable. Fortunately, our galaxy is only one of about a trillion galaxies in the visible Universe. If you monitor millions of galaxies all the time, it is possible to find many supernovae each and every day. This is one of the most exciting challenges of modern high-speed astronomy.

Other than supernovae, there are only a few variable sources luminous enough to be seen at the great distances to other galaxies, even using powerful telescopes. By far the most common is the random variability of quasars. Quasars consist of a supermassive black hole, millions to billions of times the mass of our Sun, which shine as material falls towards the black hole, heats up and radiates energy.

Today we think that essentially every galaxy contains a supermassive black hole at its centre, and something like 1 per cent of them are accreting mass fast enough to be seen as luminous quasars. The supermassive black hole at the centre of our own galaxy is essentially ‘off’. On rare occasions, though, such a black hole rapidly turns itself ‘on’. The most fascinating cause is a so-called ‘tidal disruption event’ in which a star like the Sun passes too close to the black hole and is ripped apart by the black hole’s tides. Some of the debris then falls into the black hole to power a transient flare. These tidal disruption events are far rarer than supernovae, occurring only about once every 10,000 years in any particular galaxy. In the distant Universe, the study of variability is essentially the study of black holes and supernovae.

This gives you some sense of the remarkable astronomical zoo of variable and transient objects. The challenge for the professional astronomer is to find and characterise all these different sources not only for how they work individually, but also to determine their overall demographics and statistics. To find large numbers of them, you need a big telescope that can detect the much more numerous distant, faint objects. In general, however, bigger telescopes see only smaller pieces of the sky. This frustrating rule can be bent only by spending large sums of money.

If your scientific goal is to find the largest possible number of transients, and to study their evolution across the cosmic history of the Universe, then you want to use a big telescope that covers as much of the sky as you can afford. This is fundamentally the goal of the Large Synoptic Survey Telescope (LSST). Located in Chile, LSST is (effectively) a 6.7-metre diameter telescope, scheduled to start full science operations in 2022.

LSST will be the closest astronomers have ever come to creating a movie camera to watch the whole universe. It will survey approximately half the sky using a camera that spans more than 40 times the area of the full Moon. But LSST can obtain a new image of each patch of that sky only once every three nights. LSST can detect transients 30 million times fainter than visible to the naked eye, making it a phenomenal project for finding huge numbers of faint transient sources across the visible Universe – LSST should find some 1,000 supernovae per day! But this capability comes at a cost: roughly $600 million just for construction, plus a significant operation cost as well.

At the other limit from LSST is a project I am working on: the All-Sky Automated Survey for Supernovae (ASAS-SN). By the end of this year, ASAS-SN will consist of 20 14-cm aperture telescopes spread across the globe, and costing roughly $3.5 million for both construction and operation through to 2022. With such small telescopes – big telephoto camera lenses, really – ASAS-SN can find only bright transients, roughly 25,000 times fainter than are visible to the human eye. Even so, it should still find about one supernova a day. And because ASAS-SN is comprised of small telescopes, it can image the sky far faster than LSST. The combined ‘image’ from all the ASAS-SN telescopes spans 1,600 times the area of the Moon. This allows them to survey the entire visible sky every night.

The two projects are highly complementary, essentially balancing a trade-off between ‘quantity’ and ‘quality’. LSST provides ‘quantity’: the large numbers of faint sources needed for statistical studies of distant sources, and for studying the evolution of transient sources across cosmic time. However, the typical LSST transient is faint and hard to study in detail for long periods of time, even with the world’s largest telescopes. ASAS-SN provides ‘quality’. The bright sources found by ASAS-SN are the ones that best survey the nearby Universe, and that can be studied in the greatest detail and for the longest periods of time using larger telescopes.

One of the most important tools for astronomers is the spectrum of an object: how much light is emitted as a function of its colour. A spectrum is the best way to classify the velocities, temperatures, elemental composition and type of an object (eg, which type of supernova? What were its unique properties?). Because you must chop up the light into narrow bins of colour, you need far more light to make a spectrum of an object than to get an image of it. LSST is already a large telescope, so it will be difficult or impossible to get a spectrum of the typical, faint LSST transient.

Even for the minority of LSST sources bright enough to obtain one spectrum, the source will quickly fade and become too faint to get another spectrum to study how it evolves with time. Therefore, a negligible fraction of LSST discoveries will be studied by this fundamentally important astronomical tool. The ASAS-SN transients are far fewer in number but are far brighter, so a very large fraction of ASAS-SN transients can be studied spectroscopically, and they can be studied for long periods of time even as they fade away.

Projects like LSST and ASAS-SN are continuing the revolution begun by Tycho, revealing the variable and sometimes violent events that light up the highly imperfect, ever-changing celestial sphere.

This article was originally published at Aeon and has been republished under Creative Commons.

Gravitational waves will bring the extreme universe into view

0

The first direct detection of gravitational waves on 14 September 2015 proved that massive objects can ripple the structure of space, verifying a key prediction of Albert Einstein’s general theory of relativity. The second detection, made on 26 December 2015 and announced this June, firmly established gravitational waves as a new window to the Universe. But even more exciting are the detections yet to come: the thousands of signals that should soon be observed by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo experiments. They will transform our understanding of black holes, neutron stars, supernova explosions, and perhaps even the origin and fate of the cosmos itself.

gravitational-waves-idea_sized-ns_gw_art
An artist’s impression of gravitational waves generated by binary neutron stars. R. Hurt/Caltech-JPL

Changes to the fields of physics and astronomy are already being felt. The two events reported so far have significantly increased the number of known stellar-mass black holes, and have demonstrated that black holes can form tight pairs and merge violently within the lifetime of the Universe; such mergers are the inferred cause of the September 14 and December 26 signals. Drawing on data from those two events, my colleagues in the LIGO and Virgo collaborations have tested general relativity in novel ways, far outside our terrestrial experience. And we have shown that black holes collide more often than expected, which has lead some researchers to speculate that black holes might be abundant enough to qualify as a variety of dark matter.

As with any new observational tool, the most important discoveries from the new detectors will surely be the ones that are unexpected. But we also have a good sense of the amazing things that the gravitational universe will tell us, even in the absence of surprises.

First, we can be certain that we will detect many more merging pairs of black holes comparable to the two already detected. The current instruments are about three times less sensitive than their full potential. At their ultimate sensitivity, the two LIGO detectors (in Louisiana and Washington state) and the Virgo experiment (near Pisa in Italy) will register dozens to hundreds of black-hole events per year. This large sample will yield a detailed census of black holes, and will allow astronomers to characterise their population all across the Universe, evaluating theories of how they form.

We also expect to observe mergers of neutron stars, the ultradense remains of stars that were too small to form black holes. Whereas black holes are so extreme that they are breathtakingly simple (completely described by their mass, spin and charge), neutron stars show the Universe at its most bizarre and complex. They contain more mass than our Sun packed into a sphere the size of Manhattan, with magnetic fields that can be more than a billion times as powerful as Earth’s. We do not understand how matter this dense behaves, nor do we know how their magnetic fields are sustained. What we do know is that pairs of neutron stars sometimes spiral into each other. The resulting gravitational waves will give us, for the first time, an unobstructed picture of neutron stars as they interact.

Unlike black holes, naked neutron stars emit light and other forms of radiation. Neutron-star mergers can produce a rapid flash of gamma rays or X-rays, along with a faint optical afterglow that can linger for days or weeks. With LIGO and Virgo operating in concert, we can localise the position of colliding neutron stars to within a few degrees in the sky. Optical telescopes can then search this patch of sky for a fading signal emitted by radioactive material ejected during the merger. This simultaneous observation of gravitational and electromagnetic signals could solve many long-standing mysteries in astronomy, such as the nature of energetic flashes known as short gamma-ray bursts, and the origin of heavy elements, including much of the gold found on Earth.

Gravitational waves can also show what happens in a ‘core-collapse’ supernova explosion, which occurs when the core of a massive star exhausts its nuclear fuel and is crushed under the star’s immense mass. This is an open question in astrophysics, because the mechanism that drives the explosion is hidden deep inside the star. Gravitational waves from supernovae will travel directly from the star’s centre to our detectors. Core-collapse supernovae are exceptionally rare, however; the last such one near our galaxy was in 1987, and the last known event in our galaxy proper was 400 years ago. Gravitational-wave scientists will have to be lucky and patient.

Looking out on an even grander scale, gravitational waves from neutron star mergers will give us a fresh way to study the expansion of the Universe. Our current picture of cosmology­ – in which the Universe is expanding following the Big Bang, and is accelerating due to an unseen ‘dark energy’ – relies heavily on observations of supernovae in distant galaxies. Gravitational waves will provide complementary information: the intensity (amplitude) of the gravitational signal tells us the distance to the event, while the optical appearance of the merger reveals how much its light has been stretched, or redshifted, on its way to Earth. These two pieces of information define the rate at which the Universe is expanding. Measuring this rate independently will provide an important check of our cosmological models.

Finally, LIGO and Virgo might detect a faint background hum of gravitational waves that pervades the entire Universe, constantly vibrating all of empty space. Many theories predict an omnipresent gravitational energy produced either from the accumulation of astrophysical events such as black hole mergers or from an early, extremely rapid episode of cosmic inflation immediately after the Big Bang. If the hum is loud enough, it will show up as a correlated signal between widely separated detectors such as LIGO and Virgo. Measuring the gravitational-wave background would be a dramatic achievement.

For the next few years, progress in gravitational-wave science will be limited by the sensitivity of the detectors. With each boost to their performance, it’s likely that we will uncover events from new types of sources. Eventually, perhaps after a large international investment in new facilities, progress in the field will be limited only by the willingness of the Universe to provide rare, exotic signals to observe.

LIGO and Virgo have already performed a staggering feat. Consider the properties of the September 14 event: the signal was generated by two objects, each roughly 35 times the mass of our Sun, locked in a decaying orbit the size of Switzerland, circling each other 50 times a second. The energy involved was staggering, briefly exceeding that of all the starlight in the Universe, but the signal that reached Earth was among the most imperceptible things that humans have ever measured. As gravitational-wave detections make the transition from sensational discoveries to routine tools for astrophysics and cosmology, the invisible shaking of space will, paradoxically, illuminate parts of the Universe that were entirely dark until now.

This article was originally published at Aeon and has been republished under Creative Commons.

How pigeon droppings nearly derailed a massive discovery in cosmology

0

The pigeon, the antenna and me

Great cosmology research requires accounting for an enormous number of variables, everything from nuclear detonations to bird droppings. In this animation from Nature, the American radio astronomer Robert Wilson discusses how a pair of pigeons living in a large antenna frustrated attempts to measure the minimum brightness of the sky. Even once the pigeons were removed, the measurements still weren’t right. The issue, it turned out, was cosmic microwave background radiation left behind by the Big Bang – a discovery that would eventually earn Wilson part of the 1978 Nobel Prize in physics.

Video by Dog & Rabbit