lundi 8 juillet 2019

A New Plan for Keeping NASA's Oldest Explorers Going











NASA - Voyager 1 & 2 Mission patch.

July 8, 2019


Image above: This artist's concept depicts one of NASA's Voyager spacecraft, including the location of the cosmic ray subsystem (CRS) instrument. Both Voyagers launched with operating CRS instruments. Image Credits: NASA/JPL-Caltech.

With careful planning and dashes of creativity, engineers have been able to keep NASA's Voyager 1 and 2 spacecraft flying for nearly 42 years — longer than any other spacecraft in history. To ensure that these vintage robots continue to return the best science data possible from the frontiers of space, mission engineers are implementing a new plan to manage them. And that involves making difficult choices, particularly about instruments and thrusters.

One key issue is that both Voyagers, launched in 1977, have less and less power available over time to run their science instruments and the heaters that keep them warm in the coldness of deep space. Engineers have had to decide what parts get power and what parts have to be turned off on both spacecraft. But those decisions must be made sooner for Voyager 2 than Voyager 1 because Voyager 2 has one more science instrument collecting data — and drawing power — than its sibling.

After extensive discussions with the science team, mission managers recently turned off a heater for the cosmic ray subsystem instrument (CRS) on Voyager 2 as part of the new power management plan. The cosmic ray instrument played a crucial role last November in determining that Voyager 2 had exited the heliosphere, the protective bubble created by a constant outflow (or wind) of ionized particles from the Sun. Ever since, the two Voyagers have been sending back details of how our heliosphere interacts with the wind flowing in interstellar space, the space between stars.

Not only are Voyager mission findings providing humanity with observations of truly uncharted territory, but they help us understand the very nature of energy and radiation in space — key information for protecting NASA's missions and astronauts even when closer to home.

Mission team members can now preliminarily confirm that Voyager 2's cosmic ray instrument is still returning data, despite dropping to a chilly minus 74 degrees Fahrenheit (minus 59 degrees Celsius). This is lower than the temperatures at which CRS was tested more than 42 years ago (down to minus 49 degrees Fahrenheit, or minus 45 degrees Celsius). Another Voyager instrument also continued to function for years after it dropped below temperatures at which it was tested.

"It's incredible that Voyagers' instruments have proved so hardy," said Voyager Project Manager Suzanne Dodd, who is based at NASA's Jet Propulsion Laboratory in Pasadena, California. "We're proud they've withstood the test of time. The long lifetimes of the spacecraft mean we're dealing with scenarios we never thought we'd encounter. We will continue to explore every option we have in order to keep the Voyagers doing the best science possible."

Voyager 2 continues to return data from five instruments as it travels through interstellar space. In addition to the cosmic ray instrument, which detects fast-moving particles that can originate from the Sun or from sources outside our solar system, the spacecraft is operating two instruments dedicated to studying plasma (a gas in which atoms have been ionized and electrons float freely) and a magnetometer (which measures magnetic fields) for understanding the sparse clouds of material in interstellar space.

Taking data from a range of directions, the low-energy charged particle instrument is particularly useful for studying the probe's transition away from our heliosphere. Because CRS can look only in certain fixed directions, the Voyager science team decided to turn off CRS's heater first.

Voyager probe. Animation Credits: NASA/JPL

Voyager 1, which crossed into interstellar space in August 2012, continues to collect data from its cosmic ray instrument as well, plus from one plasma instrument, the magnetometer and the low-energy charged particle instrument.

Why Turn Off Heaters?

Launched separately in 1977, the two Voyagers are now over 11 billion miles (18 billion kilometers) from the Sun and far from its warmth. Engineers have to carefully control temperature on both spacecraft to keep them operating. For instance, if fuel lines powering the thrusters that keep the spacecraft oriented were to freeze, the Voyagers' antennae could stop pointing at Earth. That would prevent engineers from sending commands to the spacecraft or receiving scientific data. So the spacecraft were designed to heat themselves.

But running heaters — and instruments — requires power, which is constantly diminishing on both Voyagers.

Each of the probes is powered by three radioisotope thermoelectric generators, or RTGs, which produce heat via the natural decay of plutonium-238 radioisotopes and convert that heat into electrical power. Because the heat energy of the plutonium in the RTGs declines and their internal efficiency decreases over time, each spacecraft is producing about 4 fewer watts of electrical power each year. That means the generators produce about 40% less than what they did at launch nearly 42 years ago, limiting the number of systems that can run on the spacecraft.

The mission's new power management plan explores multiple options for dealing with the diminishing power supply on both spacecraft, including shutting off additional instrument heaters over the next few years.

Revving Up Old Jet Packs

Another challenge that engineers have faced is managing the degradation of some of the spacecraft thrusters, which fire in tiny pulses, or puffs, to subtly rotate the spacecraft. This became an issue in 2017, when mission controllers noticed that a set of thrusters on Voyager 1 needed to give off more puffs to keep the spacecraft's antenna pointed at Earth. To make sure the spacecraft could continue to maintain proper orientation, the team fired up another set of thrusters on Voyager 1 that hadn't been used in 37 years.

Voyager 2's current thrusters have started to degrade, too. Mission managers have decided to make the same thruster switch on that probe this month. Voyager 2 last used these thrusters (known as trajectory correction maneuver thrusters) during its encounter with Neptune in 1989.

Many Miles to Go Before They Sleep

The engineers' plan to manage power and aging parts should ensure that Voyager 1 and 2 can continue to collect data from interstellar space for several years to come. Data from the Voyagers continue to provide scientists with never-before-seen observations of our boundary with interstellar space, complementing NASA's Interstellar Boundary Explorer (IBEX), a mission that is remotely sensing that boundary. NASA is also preparing the Interstellar Mapping and Acceleration Probe (IMAP), due to launch in 2024, to capitalize on the Voyagers' observations.

"Both Voyager probes are exploring regions never before visited, so every day is a day of discovery," said Voyager Project Scientist Ed Stone, who is based at Caltech. "Voyager is going to keep surprising us with new insights about deep space."

The Voyager spacecraft were built by JPL, which continues to operate both. JPL is a division of Caltech in Pasadena. The Voyager missions are a part of the NASA Heliophysics System Observatory, sponsored by the Heliophysics Division of the Science Mission Directorate in Washington. For more information about the Voyager spacecraft, visit:

https://www.nasa.gov/voyager

https://voyager.jpl.nasa.gov

Related links:

Interstellar Boundary Explorer (IBEX): https://www.nasa.gov/mission_pages/ibex/index.html

Interstellar Mapping and Acceleration Probe (IMAP): https://www.nasa.gov/press-release/nasa-selects-mission-to-study-solar-wind-boundary-of-outer-solar-system

Image (mentioned), Animation (mentioned), Text, Credits: NASA/Tony Greicius/JPL/Calla Cofield.

Greetings, Orbiter.ch

samedi 6 juillet 2019

What’s happening to Greenland’s ice?









ESA - European Space Agency patch.

6 July 2019

Heatwave conditions catapulted Greenland into an early Arctic summer in June, prompting widespread melting across its icesheet surface, according to researchers at the Danish Meteorological Institute.

Although unusually early, this weather-related event is not unprecedented, according to climate scientist Dr Ruth Mottram, who has published a comprehensive assessment that details major longer-term changes occurring across the planet’s second largest icesheet, in the journal Remote Sensing.

Meltwater lake

The research, involving scientists from DMI, the Technical University of Denmark and the Geological Survey of Denmark and Greenland, combined 30 years of satellite observations of the icesheet’s surface height, mass and movement with climate model output. Collectively this work provides a ‘health check on the icesheets current status and helps to establish the extent of ice loss due to surface melt or from other ocean processes, such as iceberg calving.

An average 255 gigatonnes of ice was lost each year from 2003 to 2016, according to the research team’s findings.

Worringly, the loss of ice shows a marked three-fold acceleration (83 Gt) compared to the preceding decade and consistent with similar studies at the North and South poles, and a potential concern for the international community.

Loss of land ice is a potential indicator of climate change and contributes directly to sea level rise, posing a risk to people living near the coast across the world.

“The Greenland losses have raised sea level by around half a millimeter each year over the observed period,” explains Dr Mottram. She also emphasises the importance of continuing monitoring as scientists are still yet to fully understand the reasons for interannual variability that they observe.

Changing Greenland icesheet height 1995-2017

Almost all of the ice loss was due to changes in surface mass budget, with thinning found virtually everywhere. At some locations, the icesheet surface decreased by over two and a half metres per year between 1995 and 2017 based on measurements using space-borne radar altimeters.

The researchers point to increased melting and changes in snowfall rates for the decrease.

“If an icesheet is to maintain its mass balance, or volume, we would expect to see the height increase at its centre due to snow accumulation. It is striking how this pattern has changed when comparing the early 1990s to the last few years,” explains Dr Mottram.

The rate of ice flow and iceberg calving of glaciers can also be measured from Space, with the study finding that all but one from a representative sample of 28 Greenland glaciers had substantially retreated since the 1990s.

Such changes were found in areas around Jakobshavn Isbrae in western Greenland and Helheim glacier in south east Greenland with the increase in ice flow pulling more ice out of the interior, contributing to a thinning of the icesheet.

The observational datasets used in this study have been developed through the European Space Agency’s Climate Change Initiative. Covering 21 key components of the Earth climate system, including information on the cryosphere and the Greenland icesheet, the continuous and long-term time series are generated by merging historic satellite missions with today’s current satellites, including the Copernicus Sentinels. Referred to as Essential Climate Variables, they provide the empirical evidence of a changing climate and support policy and decision-makers to address the consequences.

Ice velocity maps of Greenland

This latest study used these observations to validate and identify improvements to the existing climate and icesheet computer models, used to simulate the icesheet’s current state and predict how it may change into the future.

Despite huge strides being made in understanding the icesheet, the models and observations did not fully agree in certain areas, such as Southern Greenland, nor were the simulations able to fully capture the variability in year to year ice loss.

The authors emphasise the importance of continuing accurate monitoring of the icesheet to help investigate and model its dynamic processes and point to the Copernicus Sentinel satellites as game-changers.

“With Copernicus Sentinel-1 and -3, we are moving from only being able to take a short snapshot of icesheet flow speeds or calving front changes beginning to be able to monitor the Greenland icesheet remotely, in almost real time.

“We now get consistent, weekly repeat, and with such a richness of data we can more accurately understand how Greenland is responding to a changing environment.”

Related links:

Remote Sensing: https://www.mdpi.com/2072-4292/11/12/1407

Observing the Earth: http://www.esa.int/Our_Activities/Observing_the_Earth

Space for our climate: http://www.esa.int/Our_Activities/Observing_the_Earth/Space_for_our_climate

Climate Change Initiative: http://cci.esa.int/

Sentinel-1: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus/Sentinel-1

Sentinel-3: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus/Sentinel-3

Copernicus: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus

Images, Text, Credits: ESA/Nasa/Jim Yungel/Mottram et al.

Greetings, Orbiter.ch

vendredi 5 juillet 2019

Another successful launch from Vostochny Cosmodrome













ROSCOSMOS logo.

July 05, 2019

Soyuz-2.1b launches Meteor-M No. 2-2 and 32 small satellites

Today, on July, 5 2019 at 08:41:46 Moscow time Soyuz 2.1b carrier rocket with Fregat booster was successfully launched from Vostochny Cosmodrome. The rocket carried Meteor-M Russian meteorological spacecraft No. 2-2 as well as 32 spacecraft as secondary payload. The injection into orbit took place during 4.5 hours after the launch.

The launch vehicle including Soyuz 2.1 (built by Progress Russian Space Center), Fregat booster (built by NPO Lavochkin) operated as expected. According to the flight program the booster put the main and secondary spacecraft into three different orbits. After the completion of the program the booster will be sunk in a non-navigable district of the Pacific ocean.

Soyuz-2.1b launches Meteor-M No. 2-2 and 32 small satellites

Meteor-M spacecraft No. 2-2 was built by VNIIEM Corporation and falls into the category of Earth remote sensing satellites. The spacecraft is capable of providing images of clouds, Earth surface, ice and snow cover in visible, infrared and microwave bands. It is also capable of receiving data about the sea surface temperature and ozone layer condition, as well as measuring humidity level. This data will help to improve weather forecast accuracy in Russia.

29 satellites were launched for Germany, France, USA, Israel, UK, Sweden, Finland, Thailand, Ecuador, Czech Republic and Estonia. Three Russian academic CubeSats were launched as well.

Meteor-M Russian meteorological spacecraft No. 2-2

To make the injection into orbit as precise and comfortable as possible, Fregat booster formed three various orbits depending on the spacecraft mission. The first orbit is a heliosynchronous one with the height of 828 kilometers and inclination of 98.57 degrees, the second one is 580 kilometers high and with the inclination of 97.7 degrees, the third orbit is 530 kilometers high with the inclination of 97.5 degrees. All the spacecraft separated from the booster as expected and will further be managed by the customer companies of the launch.

Roscosmos Press Release: http://en.roscosmos.ru/20804/

Images, Video, Text, Credits: Роскосмос/ЦЭНКИ/SciNews/Wikipedia.

Best regards, Orbiter.ch

New Crew in Final Preps Before Historic July 20 Launch













ISS - Expedition 60 Mission patch.

July 5, 2019

The next crew to liftoff to the International Space Station arrived at the Baikonur Cosmodrome launch site on the U.S. Independence Day awaiting a historic July 20 liftoff.

New Expedition 60 crewmates Andrew Morgan, Luca Parmitano and Alexander Skvortsov are in final mission preparations in Kazakhstan. The trio arrived July 4 counting down to a July 20 launch to the orbiting lab 50 years to the NASA landed humans on the Moon for the first time.


Image above: Expedition 60 crewmembers (from left) Drew Morgan, Alexander Skvortsov and Luca Parmitano affix a crew insignia sticker to the hull of the Gagarin Cosmonaut Training Center aircraft as they flew to their training base in Kazakhstan July 4. Image Credit: NASA.

Morgan is going to space for the first time and will meet his fellow Class of 2013 NASA astronaut members, Christina Koch and Nick Hague, who have been at the station since March. Parmitano is on his second mission. Skvortsov, who is leading the mission aboard the Soyuz MS-13 spacecraft, is making his third visit to the space station.

International Space Station (ISS). Image Credit: NASA

Back aboard the station, the three orbiting Expedition 60 crewmembers continued science and maintenance duties. Koch sampled the station’s life support system for microbes while Hague serviced a specialized science furnace. Skvortsov checked on Russian station systems and monitored a radiation exposure study.

Related links:

Expedition 60: https://www.nasa.gov/mission_pages/station/expeditions/expedition60/index.html

Specialized science furnace: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=1536

Radiation exposure study: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/search.html?#q=matroyshka&i=&p=&c=&g=&s=

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

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

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

Best regards, Orbiter.ch

Hubble Watches Stars in Bloom












NASA - Hubble Space Telescope patch.

July 5, 2019


This NASA/ESA Hubble Space Telescope image shows bright, colorful pockets of star formation blooming like roses in a spiral galaxy named NGC 972.

The orange-pink glow is created as hydrogen gas reacts to the intense light streaming outwards from nearby newborn stars; these bright patches can be seen here amid dark, tangled streams of cosmic dust.

Astronomers look for these telltale signs of star formation when they study galaxies throughout the cosmos, as star formation rates, locations, and histories offer critical clues about how these colossal collections of gas and dust have evolved over time. New generations of stars contribute to — and are also, in turn, influenced by — the broader forces and factors that mold galaxies throughout the universe, such as gravity, radiation, matter, and dark matter.

German-British astronomer William Herschel is credited with the discovery of NGC 972 in 1784. Astronomers have since measured its distance, finding it to be just under 70 million light-years away.

Hubble Space Telescope (HST)


For more information about Hubble, visit:

http://hubblesite.org/

http://www.nasa.gov/hubble

http://www.spacetelescope.org/

Text Credits: ESA (European Space Agency)/NASA/Rob Garner/Image, Animation, Credits: ESA/Hubble, NASA, L. Ho.

Greetings, Orbiter.ch

Space Station Science Highlights: Week of July 1, 2019













ISS - Expedition 60 Mission patch.

July 5, 2019

International Space Station (ISS). Animation Credit: NASA

Crew members aboard the International Space Station conducted scientific investigations last week that tracked radiation, studied heat transfer in space and supported future explorations. The current crew includes Expedition 60 Commander Alexey Ovchinin of Roscosmos and NASA astronauts Nick Hague and Christina Koch. NASA astronaut Andrew Morgan, Alexander Skvortsov of the Russian space agency Roscosmos, and Luca Parmitano of the European Space Agency (ESA) are scheduled to join them on July 20 – the 50th anniversary of the Apollo 11 Moon landing. Research on the space station supports Artemis, NASA’s program to return humans to the Moon and establish a sustained presence there.

Here are details on some of the science conducted on the orbiting lab during the week of July 1:

A direct line to the space station


Image above: During an ISS HAM radio session, NASA astronaut Nick Hague answers questions from students on the ground. Image Credit: NASA.

Crew members conducted an ISS Ham session last week. Using amateur or ham radio, groups of students talk directly to the crew aboard the space station when it passes overhead. The students learn about the space station, radio waves, and other science and engineering topics and prepare questions before their scheduled calls. Hundreds more listen in from classrooms or auditoriums. This real-time contact with the orbiting lab sparks interest in science, technology, engineering and mathematics and inspires the next generation of explorers.

Tracking neutron radiation

The RADI N2 investigation seeks to better characterize the neutron radiation environment aboard the space station using bubble detectors attached to fixed locations and carried by crew members. The data could help define the risk that this type of radiation poses to crew members and support development of advanced protective measures for future spaceflight. The crew continued to deploy detectors on the space station last week.

A better way to keep cool


Image above: NASA astronaut Christina Koch demonstrates behavior of fluids in the microgravity environment aboard the International Space Station. Image Credit: NASA.

Last week, the crew conducted a session for the Two Phase Flow investigation, which examines the heat transfer characteristics of flow boiling in microgravity. Boiling removes heat by turning liquid into vapor at the heated surface. Returning that vapor to a liquid by way of a condenser creates a cooling system. In microgravity, though, liquid and bubble behaviors differ drastically from that on Earth. The investigation creates a database on the heat transfer efficiency of liquids in space that can inform design of thermal management systems for future spacecraft. It also can support development of improved cooling systems for hybrid cars and other electronics systems that generate high heat in small spaces on Earth.

Meeting the demand for small satellites


Image above: The sun glints off the Celebes Sea of Southeast Asia in this image captured as the space station flew 225 miles above Indonesia. Image Credit: NASA.

Crew members installed the NanoRacks External Cygnus CubeSat Deployer (extCygnus NRCSD), a stackable, modular case for launching small satellites. Each deployer accommodates up to eight launch cases, helping to meet the growing demand for this type of satellite for a variety of customers. The extCygnus NRCSD releases CubeSats from the Cygnus resupply vehicle after it completes its resupply mission and leaves the space station.

Other investigations on which the crew performed work:

- The Veg-04A investigation focuses on how light quality and fertilizer affect growth of Mizuna mustard, a leafy green crop, as part of an effort to develop the capability to produce fresh food in space. It also looks at microbial food safety, nutritional value, taste acceptability by the crew, and the overall behavioral health benefits of having plants and fresh food in space: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7896

- Team Task Switching looks at whether crew members have difficulty switching from one task to another and the effects of such switches to reduce negative consequences and improve individual and team motivation and effectiveness: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7538

- The ISS Experience creates short virtual reality videos from footage taken during the yearlong investigation covering different aspects of crew life, execution of science, and the international partnerships involved on the space station: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7877

- Standard Measures captures a consistent and simple set of measures from crew members throughout the ISS Program to characterize adaptive responses to and risks of living in space: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7711

Space to Ground: On the Bubble: 07/05/2019

Related links:

Expedition 60: https://www.nasa.gov/mission_pages/station/expeditions/expedition60/index.html

ISS Ham: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=337

RADI N2: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=874

Two Phase Flow: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=1034

NanoRacks External Cygnus CubeSat Deployer (extCygnus NRCSD): https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=2015

ISS National Lab: https://www.issnationallab.org/

Spot the Station: https://spotthestation.nasa.gov/

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

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

Animation (mentioned), Images (mentioned), Video (NASA), Text, Credits: NASA/Michael Johnson/Vic Cooley, Lead Increment Scientist Expedition 60.

Best regards, Orbiter.ch

X-rays Spot Spinning Black Holes Across Cosmic Sea













NASA - Chandra X-ray Observatory patch.

July 5, 2019


Like whirlpools in the ocean, spinning black holes in space create a swirling torrent around them. However, black holes do not create eddies of wind or water. Rather, they generate disks of gas and dust heated to hundreds of millions of degrees that glow in X-ray light.

Using data from NASA’s Chandra X-ray Observatory and chance alignments across billions of light years, astronomers have deployed a new technique to measure the spin of five supermassive black holes. The matter in one of these cosmic vortices is swirling around its black hole at greater than about 70% of the speed of light.

The astronomers took advantage of a natural phenomenon called a gravitational lens. With just the right alignment, the bending of space-time by a massive object, such as a large galaxy, can magnify and produce multiple images of a distant object, as predicted by Einstein.

In this latest research, astronomers used Chandra and gravitational lensing to study six quasars, each consisting of a supermassive black hole rapidly consuming matter from a surrounding accretion disk. Gravitational lensing of the light from each of these quasars by an intervening galaxy has created multiple images of each quasar, as shown by these Chandra images of four of the targets. The sharp imaging ability of Chandra is needed to separate the multiple, lensed images of each quasar.

The key advance made by researchers in this study was that they took advantage of “microlensing,” where individual stars in the intervening, lensing galaxy provided additional magnification of the light from the quasar. A higher magnification means a smaller region is producing the X-ray emission.  

The researchers then used the property that a spinning black hole is dragging space around with it and allows matter to orbit closer to the black hole than is possible for a non-spinning black hole. Therefore, a smaller emitting region corresponding to a tight orbit generally implies a more rapidly spinning black hole. The authors concluded from their microlensing analysis that the X-rays come from such a small region that the black holes must be spinning rapidly.

The results showed that one of the black holes, in the lensed quasar called the “Einstein Cross,” is spinning at, or almost at, the maximum rate possible. This corresponds to the event horizon, the black hole’s point of no return, spinning at the speed of light, which is about 670 million miles per hour. Four other black holes in the sample are spinning, on average, at about half this maximum rate. (The 6th did not enable an estimate of spin.)

For the Einstein Cross the X-ray emission is from a part of the disk that is less than about 2.5 times the size of the event horizon, and for the other 4 quasars the X-rays come from a region four to five times the size of the event horizon.

How can these black holes spin so quickly? The researchers think that these supermassive black holes likely grew by accumulating most of their material over billions of years from an accretion disk spinning with a similar orientation and direction of spin, rather than from random directions. Like a merry-go-round that keeps getting pushed in the same direction, the black holes kept picking up speed.

Chandra X-ray Observatory

The X-rays detected by Chandra are produced when the accretion disk surrounding the black hole creates a multimillion-degree cloud, or corona, above the disk near the black hole. X-rays from this corona reflect off the inner edge of the accretion disk, and the strong gravitational forces near the black hole distort the reflected X-ray spectrum, that is, the amount of X-rays seen at different energies. The large distortions seen in the X-ray spectra of the quasars studied here imply that the inner edge of the disk must be close to the black holes, giving further evidence that they must be spinning rapidly.

The quasars are located at distances ranging from 8.8 billion to 10.9 billion light years from Earth, and the black holes have masses between 160 and 500 million times that of the sun. These observations were the longest ever made with Chandra of gravitationally lensed quasars, with total exposure times ranging between 1.7 and 5.4 days.

A paper describing these results is published in the July 2nd issue of The Astrophysical Journal, and is available online. The authors are Xinyu Dai, Shaun Steele and Eduardo Guerras from the University of Oklahoma in Norman, Oklahoma, Christopher Morgan from the United States Naval Academy in Annapolis, Maryland, and Bin Chen from Florida State University in Tallahassee, Florida.

The Astrophysical Journal: https://arxiv.org/abs/1901.06007

NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

Read more from NASA's Chandra X-ray Observatory: http://chandra.harvard.edu/photo/2019/quasars/

For more Chandra images, multimedia and related materials, visit: http://www.nasa.gov/chandra

Image, Animation, Text, Credits: NASA/Lee Mohon/CXC/Univ. of Oklahoma/X. Dai et al.

Greetings, Orbiter.ch