Celestial Astronomy’s newest 10-year plan focuses on alien Earths

Housecarl

On TB every waking moment
Posted for fair use.....

DECEMBER 16, 2021
Astronomy’s newest 10-year plan focuses on alien Earths
Stanford astronomer Bruce Macintosh was a co-author of the latest “Decadal Survey,” a once-in-a-decade report that helps set the research priorities for the astronomy and astrophysics communities. Those priorities will include the identification of other habitable Earth-like worlds and determining whether life exists elsewhere in the universe.
BY KER THAN

Every 10 years, the National Academies of Sciences, Engineering and Medicine issues a report that helps set the research priorities for the astronomy and astrophysics communities for the next decade.

Bruce Macintosh(Image credit: Courtesy Stanford Department of Physics)

The seventh and latest “Decadal Survey,” published earlier this fall, recommended a number of new and ambitious ground- and space-based observatories and missions for discovering extrasolar planets – planets beyond our solar system – resembling Earth; studying colliding black holes and other cosmic cataclysms; and understanding the origin and evolution of galaxies. It also outlined new initiatives to help make sure the tools and technologies critical to these missions are developed on time and on budget. And in a departure from past Decadal Surveys, this latest report also focused on broader issues affecting the astronomy and astrophysics communities, including the diversity and mental health of their practitioners and their relationship to society at large.

Stanford astronomer Bruce Macintosh was a member of the National Academies committee that issued the 614-page report, titled “Pathways to Discovery in Astronomy and Astrophysics for the 2020s.”

Macintosh, whose research focuses on directly imaging extrasolar planets, spoke to Stanford News about the report’s conclusions and recommendations.

The Decadal Survey recommends that NASA and the National Science Foundation (NSF) construct several new space- and ground-based observatories, respectively. How will the observatories differ from one another, and what will they be studying?

On the ground, there are three big recommendations to NSF. The highest priority is a federal role in one or two “Extremely Large Telescope” project collaborations – about 25 percent in each the Giant Magellan Telescope and the Thirty Meter Telescope. These are general-purpose facilities that can do almost any kind of astrophysics, from mapping nearby asteroids to the first galaxies billions of light years away, as well as study exoplanets.

The longest-term recommendation is the Next Generation Very Large Array (NGVLA). The current VLA is a network of radio telescope dishes in New Mexico that combine to form a single telescope 20 miles across – we call this a “radio interferometer.” The NGVLA would replace this with a new array that would cover most of the continental U.S., taking advantage of modern computing to combine this into a single telescope thousands of miles across. It would also do a lot of different science missions.

The third ground recommendation, which is joint to NSF and the Department of Energy, is to build a more specialized array of radio telescopes to look at the Cosmic Microwave Background (CMB) – the radiation left over from the Big Bang. Importantly, the Decadal didn’t recommend it just for cosmology and the early universe – the telescope will be surveying the whole sky and will be able to see clusters of galaxies, stellar explosions, etc., and the project has to make the data available to everyone.

In space, the biggest recommendation is a big optical/infrared/ultraviolet telescope optimized for studying Earth-like planets, and the Great Observatories program – more on that below. While those are developing, there will be a regular program for a new kind of mission called a “Probe.” About the cost of the [$690 million] Stanford-led Fermi spacecraft, these are powerful but specialized missions; teams will compete to see who gets to lead which mission. The two Probe missions proposed so far are a far-infrared telescope that could study dust in early galaxies or trace water as planets are forming, or an X-ray telescope with incredibly precise optics to make ultra-sharp images of things like black holes.

According to the survey, exoplanets should be a major research focus for the field in the coming decade. Why is that? And what do astronomers want to learn about planets beyond our solar system?
Exoplanets are a focus because they’re awesome

SCIENCE & TECHNOLOGY
Physics professor explains exoplanets
A Q&A with astronomer Bruce Macintosh on what people should understand about exoplanets – planets outside our solar system – and what exoplanet research means for life on Earth.

But more seriously, we’re in a position to make some really transformative discoveries. In the past decade we’ve been studying exoplanets but mostly by counting them – figuring out how many planets of different sizes exist. We have no idea what many of them are really like.

Now we’re starting to study them in detail and measure their atmospheres. With the telescopes we have right now, we can do that for giant planets (Neptune- or Jupiter-sized) that are either very close to their star or very far away.

In the next decade, we’ll measure the spectra, or light, of new kinds of planets. Even the new James Webb Space Telescope (JWST) launching later this month will still be limited to planets close to their stars – closer than Mercury is to our sun – but sensitive enough to measure the atmospheres of Earth-sized planets. Most will be superheated, but some, orbiting close to the smallest and coldest stars, could have Earth-like conditions such as liquid water on their surface. The Extremely Large Telescopes will play a role too, probing planets like our own gas giants, and helping put together a comprehensive picture of how planets form and evolve and maybe approach conditions for life.

What other research priorities did the committee suggest the astronomy and astrophysics community focus on in the coming decade?

Other than stars and planets, the committee identified two additional major research themes and priority areas within them. For thousands of years astronomers have studied the universe with light – whether that’s visible light or X-ray light or radio light. But the universe throws a lot of other things at us – cosmic rays, neutrinos and the ripples in space we call gravitational waves. These “new messengers” come from energetic and exotic physics. New messenger projects will focus on the dynamic universe, which I mostly consider to be “things that blow up” – exploding stars, black holes crashing into each other.

The third theme is “cosmic ecosystems.” The universe is made out of three kinds of things. The moderately mysterious one is “dark matter” – something invisible and intangible that still contributes most of the mass and gravity in the universe. The most mysterious is “dark energy,” the force accelerating the universe apart. The third is ordinary matter – gas and dust and stars.

Although ordinary matter seems the least mysterious, in some ways it’s the hardest to model with our computers, because matter can interact with itself in so many ways. The priority focus within this theme is the growth of galaxies. Thanks to people like Risa Weschler, we’re beginning to understand how dark matter condenses to form the gravitational well of galaxies. The facilities of the 2020s map dark matter by seeing the light of stars under its influence. New facilities will study the gas and dust and the feedback that comes from gravitational wells – gas turning into stars that then explode and blow the gas right out of the galaxy – and the details of how galaxies form and make stars and planets.

The committee recommends that NASA establish a new initiative, called the Great Observatories Mission and Technology Maturation Program (GOMTMP), that would represent a fundamental shift in how NASA plans and develops large astronomy projects. What are some key aspects of this initiative?

Big space-based telescopes are extremely expensive – ranging from $3 billion for the Chandra X-ray Observatory to $10 billion for Hubble and JWST. These are scientifically amazing but have also had complicated track records. For example, the cost of JWST has grown enormously since a previous Decadal recommended it.

The GOMTMP is supposed to reduce the uncertainty. Before a new space mission would truly start, NASA would make a major investment in developing the technology and the mission design early, so that when a mission is finally approved to start, NASA and scientists and Congress would have an accurate estimate of what it costs and know whether or not it’s feasible.

What role do you see Stanford playing in the projects outlined in the survey?
Stanford is in a good position to be involved in many of these initiatives. The current fourth-generation ground-based cosmic microwave background experiment, or CMB S4, grows out of previous CMB projects that we are leaders in, and SLAC National Accelerator Laboratory and Stanford will be a major part of the collaboration. Stanford scientists and engineers have been working on the detectors for the next-generation X-ray telescopes, and the Probe mission concept provides a good way for universities and national labs to join and compete to help lead these missions. Our exoplanet scientists will likely be part of the process that defines the LuvEx mission [a new infrared/optical/UV telescope proposed in the Decadal].

This Decadal also focused on broad issues such as increasing diversity and inclusion in the profession and maintaining the mental health of its practitioners. Can you talk more about that?

A new thing this survey includes is a careful, thoughtful look at the state of our profession and its relationship to society. Astronomy is amazing and exciting. But we also need to make sure it’s humane and just, that we treat people in it well, that we reflect the population of the nation, and that we respect the people whose mountains we build telescopes on. A whole chapter and appendix of the report are devoted to this – discussing the profession, ways in which we are improving, while acknowledging our failures on diversity, harassment and our complicated history, and continuing the (long) process of remedying these failings.

KIPAC and Stanford astrophysics have been leaders in improving equity and inclusion in the profession of astrophysics, and the voices of people like me and Risa will be important to advancing the improvements the survey recommended.

What must happen now for any of these proposed projects to become a reality?
First, we need to do a lot of engineering and management and design – proving these projects are feasible and getting the best estimate as to how much they cost.

Then, building them will require real national will – these are grand projects. Congress has to approve them. For that, astronomers and the public have to make it clear that these really are priorities – that answering fundamental questions about the universe is something that we want to do as a nation.

Macintosh is a professor of physics in the School of Humanities and Sciences and deputy director of the Kavli Institute for Particle Astrophysics and Cosmology.
 

jward

passin' thru
'scuse me. U R droppin the purties again :: sad look ::

I get this feeling that by the time they invent the tools they need & begin their projects, they'll be out of people who are able to maintain, repair & replace the tool sets, or understand, interpret and extrapolate from the data sets. May yet prove we do our progeny more good drawing pictorials on cave walls exhorting them to never place their loos upstream & to wash their hands (and mask up lol) frequently :: shrug ::
The longest-term recommendation of the latest Decadal Survey of the National Academies is the Next Generation Very Large Array (NGVLA). Pictured above is the Karl G. Jansky Very Large Array west of Socorro, New Mexico. The NGVLA would replace this with a new array that would cover most of the continental U.S., taking advantage of modern computing to combine this into a single telescope thousands of miles across. (Image credit: NRAO/AUI/NSF, Jeff Hellerman)
karlsVeryLgArray21.jpg
 

jward

passin' thru
coincidentally- or not- the biggest telescope (in space) launched successfully just hours ago.






Latest in space
@latestinspace

3h

Launch of the world's largest and most powerful telescope ever, James Webb. #JamesWebbSpaceTelescope
View: https://twitter.com/latestinspace/status/1474937404867977218?s=20


NASA Webb Telescope
@NASAWebb

18h

#NASAWebb’s fairing has been jettisoned, revealing the telescope for the first time in space! Also, we have successfully received telemetry from the observatory. #UnfoldTheUniverse https://blogs.nasa.gov/webb/2021/12/2
View: https://twitter.com/NASAWebb/status/1474718163115851781?s=20
 

jward

passin' thru
James Webb Space Telescope lifts off in spectacular Christmas morning launch
Scott Sutherland

7-9 minutes


James Webb Space Telescope lifts off in spectacular Christmas morning launch


James Webb Space Telescope lifts off in spectacular Christmas morning launch

After years of waiting, the day finally arrived! On Christmas morning, the astronomy and space community received what could be the best present of all — the launch of the most powerful space telescope ever built.
Early in the morning, on Saturday, December 25, an Ariane 5 rocket lifted off from Europe's Spaceport in French Guiana. Perched atop this rocket was the James Webb Space Telescope, quite possibly the most important astronomy payload to be sent to space of the past two decades.
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JamesWebbSpaceTelescope-separation-launch-NASATV

The James Webb Space Telescope is seen here in low-Earth orbit, after it separated from the launch vehicle. Unlike the Hubble Space Telescope, which orbits Earth and can be spotted from the ground, until we build ships that regularly carry humans around the solar system, this is the last time we will see Webb, as it begins its journey to Lagrange point 2, 1.5 million km away. Credit: NASA TV
As the long-awaited successor to the Hubble Space Telescope, Webb is over 100 times more powerful than Hubble and is expected to revolutionize astronomy. It will give us our clearest views yet of objects both near and far distant in the cosmos, and it will allow us to look farther back in time than we ever have before, to when the first stars ignited in the early universe.
According to NASA: "Webb will directly observe a part of space and time never seen before. Webb will gaze into the epoch when the very first stars and galaxies formed, over 13.5 billion years ago. Ultraviolet and visible light emitted by the very first luminous objects has been stretched or 'redshifted' by the universe's continual expansion and arrives today as infrared light. Webb is designed to 'see' this infrared light with unprecedented resolution and sensitivity."
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This graphic explores the differences between the Hubble Space Telescope and the new James Webb Space Telescope. Credit: ESA/M. Kornmesser
Webb launched at 7:20 a.m. EST on Saturday, December 25. Complete coverage of the launch was broadcast by NASA, which can be watched below.

CANADA KEEPS WEBB ON TARGET
As a contributor to the JWST mission, along with NASA and the ESA, the Canadian Space Agency has provided two essential instruments to the new space telescope.
The first, the Fine Guidance Sensor (FGS), is quite possibly the most crucial instrument for Webb's mission, allowing the telescope to:
  • use the stars as cosmic reference points to determine its position in space,
  • pinpoint the celestial targets astronomers want to observe,
  • track moving targets across the backdrop of space, and
  • maintain a steady, high-precision lock on its celestial targets.
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Canada's stellar navigator on the James Webb Space Telescope. Credit: Canadian Space Agency
Integrated into the same unit as the FGS is the second Canadian contribution, the Near-Infrared Imager and Slitless Spectrograph, or NIRISS.
Working alongside Webb's other instruments, NIRISS will contribute to our understanding of the universe. Most remarkably, though, this instrument will also allow astronomers to closely study exoplanets — alien worlds orbiting distant stars. Collecting detailed information on their atmospheres may even reveal which of these worlds are capable of supporting life.
James Webb


James Webb

This artist's impression shows the James Webb Space Telescope floating in space. Credit: ESA/Northrup Grumman
WATCHING THE WEATHER
Given the importance of this launch, the mission team is taking no chances with the weather — both here on Earth and in space.
After a few delays due to technical issues, an original launch date of December 24 was set. However, this was pushed back by a day due to some troublesome weather in the forecast for the Guiana Space Center. With better conditions expected on Christmas Day, the launch team has turned their attention to space weather.
According to NASA: "A mission this complex faces many challenges — not least the delicate operation of unfolding its instruments in space. But as the mission readies for launch, operators must evaluate another risk: space weather, the fluctuating, sometimes dangerous conditions in space driven by the Sun."
There are three main concerns when it comes to the space weather impact on a launch.
The first is how space weather can impact Earth's ionosphere, the electrically-charged region of the upper atmosphere. The effects of the solar wind and coronal mass ejections (aka solar storms) can supercharge the ionosphere. This can result in disruptions to radio communications between orbiting spacecraft and the ground.
Space-Weather-Graphic-NASA


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This graphic captures the varied impacts of space weather. Credit: NASA
The second is how changes in space weather affect the Van Allen radiation belts.
"The Van Allen Belts are always active, but an arriving solar storm can pour new electrons into them and energize those already there," says NASA. "Colliding with spacecraft, these energized electrons can build up a charge on the spacecraft's surface."
Charge buildup on a spacecraft can create a perilous situation for the mission. In a worst-case scenario, this charge can produce arcs of electricity across the spacecraft's instruments and computers, causing electrical shorts, which could damage sensitive electronics.
Van-Allen-Belts-JWST-NASA


Van-Allen-Belts-JWST-NASA

This artist's impression shows the donut-shaped Van Allen radiation belts around Earth, which are caused by high-energy particles becoming trapped in Earth's geomagnetic field. Credit: NASA
The third problem is solar energetic particles, or SEPs, which are high-energy particles accelerated at very high speeds away from the Sun during solar flares.
If SEPs strike spacecraft electronics, they can trigger events known as 'bit flips'. This is where one specific bit of the binary code of any particular command is changed from a zero to a one, or from one to zero, due to the electrical charge introduced by the particle strike.
The exact results of these events depend on what part of the spacecraft's computer was affected or which command was disrupted. Some, we'd never notice. Others can cause a complete loss of the spacecraft.
"Impacts of space weather come in many forms and can cause problems for what we're doing," Jim Spann, the space weather lead at NASA Headquarters, said in a press release. "We're going to have to pay a lot of attention to space weather."
AND NOW WE WAIT...
Now, after the launch, with the James Webb Space Telescope flying in space under its own solar power, we are going to have a long wait before the first images come in — 29 days for the telescope to reach its final orbit around Lagrange point 2, and another four to five months for testing and calibration.
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James-Webb-Space-Telescope-journey-to-L2-STScI

There is a carefully planned timeline for the deployment of Webb as it journeys to its orbit at Lagrange point 2, 1.5 million km 'behind' the Earth in its orbit around the Sun. Credit: NASA/M. Clampin (GSFC).
Just to go over exactly what this wait is all about, and why there is a lot of anxiety about the wait and the processes that will go on throughout it, Vlogbrother Hank Green recorded a short video that very handily explains it:

Check out more information on Webb at NASA's website, and watch for more updates on this mission in the days and months ahead!
 

jward

passin' thru
Webb arrives in orbit of L2, teams look ahead to five months of commissioning
written by Haygen Warren January 24, 2022



The joint NASA/ESA/CSA James Webb Space Telescope (JWST) has successfully inserted itself into its orbit at the Earth-Sun Lagrange Point 2 (L2), doing so at 2:05 pm EST (19:05 UTC) on January 24, 2022. The insertion into L2 orbit signifies the end of the observatory’s immensely complex deployment process and the beginning of the telescope’s commissioning activities.

The orbit insertion maneuver began at 2pm EST (19:00 UTC), lasted for five minutes, and added 1.6 meters per second velocity to Webb to send it into its proper orbit.

Before the insertion, which occurred at T+29 days from launch, JWST had to perform a series of complex deployments to get into its final configuration for deep space observations. The entire deployment sequence consisted of 344 unfolds, which saw the observatory unfurl from its launch position. Of those unfolds, 307 (87%) were single-point failure areas — meaning if any of those 307 unfolds had failed, the entire mission would be lost.

But every single one of those 344 highly complex unfolds worked. Additionally, the completion of JWST’s L2 insertion burn marked the end of the telescope’s mid-course correction burns — all three of which were completed successfully.
JWST’s journey to L2 began on December 25, 2021, when the observatory launched atop an Arianespace Ariane 5 rocket from pad ELA-3 at the Guiana Space Centre in Kourou, French Guiana. JWST separated from the Ariane 5 upper stage at T+27 minutes on a trajectory to L2.

The trajectory Ariane 5 placed James Webb on was accurate enough to minimize the amount of fuel the observatory needed for its trip to L2, allowing JWST to have enough fuel for around 20 years — 10 years more than originally expected — of scientific operations.
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The launch of the James Webb Space Telescope from Kourou, French Guiana. (Credit: ESA)
In the seconds following separation, JWST deployed its solar array, allowing the observatory to begin producing power. The first of Webb’s three planned mid-course correction burns took place 12 hours later, allowing the observatory to correct for the minor mistakes in its trajectory that remained from launch. The solar array deployment and first mid-course correction burn were the only time-critical steps in James Webb’s deployment sequence.
See Also
The next day saw the final autonomous deployments with the Gimballed Antenna Assembly (GAA) — which will allow the observatory to communicate and transfer data from L2 to ground stations on Earth. The second of three mid-course correction burns was also performed on T+2 days.

Three days after launch saw the beginning of the deployment sequence of the sunshield — one of the critically important components on the entire observatory. The forward and aft Unitized Pallet Structures were also deployed, marking the beginning of all major deployments.
The following day, the Deployable Tower Assembly (DTA) unfolded, lifting the mirror away from the sunshield to give room to the sunshield membranes to deploy.

T+5 days then saw the Aft Momentum Flap deploy from the aft UPS pallet. The Aft Momentum Flap offsets the amount of solar pressure that affects the observatory, minimizing fuel usage. Furthermore, T+5 days also marked the retraction of the sunshield covers.
The following day came the true test of JWST’s deployment sequence — sunshield mid-boom unfurling that pulled the entire sunshield out for tensioning.
This is it: we’ve just wrapped up one of the most challenging steps of our journey to #UnfoldTheUniverse.
With all five layers of sunshield tensioning complete, about 75% of our 344 single-point failures have been retired! pic.twitter.com/P9jJhu7bJX
— NASA Webb Telescope (@NASAWebb) January 4, 2022

The mid-booms and sunshield successfully deployed, leaving one critical step in the sequence: tensioning of the five sunshield membrane layers. The entire membrane tensioning process lasted two days as teams worked to individually and carefully tension each of the five fragile sunshield layers.
As planned, all five membranes were successfully deployed, marking the end of the sunshield deployment process and the beginning of James Webb’s initial cooling period.

However, one vital system had yet to deploy — the mirror and observatory optics.
The deployments of JWST’s Secondary Mirror Support Structure (SMSS) and the secondary mirror were completed on T+10 days, following which the Aft Deployed Instrument Radiator (ADIR) was successfully released from its launch position.
On T+12 days, primary mirror deployments began. This involved rotating the port and starboard mirror wings into place from their launch positions and latching them to the primary mirror structure. The port primary mirror wing was deployed and latched into place first.

The next day, the starboard primary mirror wing successfully rotated and latched into its final operational position, signifying the end of all major deployments on Webb and marking the successful deployment of all observatory systems — a major achievement more than two decades in the making.

View: https://www.youtube.com/watch?v=RzGLKQ7_KZQ&t=2s


But the observatory’s journey was not yet complete. It still needed to finish its transfer to L2 and move each of its 18 individual primary mirror segments out of their launch position to ready them for the alignment process.
JWST’s mirror system is the most complex ever flown into space. The primary mirror consists of 18 individual mirrors that each feature a small motor to allow each segment to move into a position that allows them to efficiently bounce light onto the secondary mirror — which then bounces light into the tertiary mirror which then carries the light to the instruments.
However, due to the nature of launch and how the telescope needed to fold, each of the 18 mirrors could not launch in their operational positions — which means they now have to be aligned with each other to “focus” the overall primary mirror.

In the days following completion of the observatory’s main deployment sequence, the JWST mirror team moved each of the 18 mirror segments to ensure each mirror’s motor successfully made it through launch and deployment and confirming that the team can perform the months-long alignment process following insertion at L2.
At this point, the final step in the deployment sequence of Webb was the telescope’s insertion into L2.
So…you’ve heard that the Webb telescope will be orbiting Lagrange point 2. But what even is that, anyway? And how do you orbit something that isn’t an object?
We’ve got you! Here’s a thread #UnfoldTheUniverse pic.twitter.com/7YTUeKh3Me
— NASA Webb Telescope (@NASAWebb) January 21, 2022

However, even though JWST is now in orbit of the L2 point, it is still not ready to begin observing the universe. The telescope still has nearly five months of commissioning before science teams from around the world can begin using the observatory for groundbreaking astrophysics research.

Throughout the next five months, JWST teams will continue bringing the observatory online and slowly testing its various systems while the mirror team aligns and focuses the telescope for observations.
Furthermore, observatory teams will continue to monitor the temperature of the telescope while the sunshield and cryocooler bring the array’s temperature down to the needed 6 Kelvin for the sensitive Infrared observations Webb is tasked with performing.

Currently, the first images from JWST are expected in mid-2022, assuming no errors or delays occur during the observatory’s commissioning phase.
(Lead image: Artist’s rendering of the James Webb Space Telescope fully deployed in space. Credit: NASA/GSFC/CIL/Adriana Manrique Gutierrez)
 

jward

passin' thru
The James Webb Space Telescope has sent back its clearest image yet

A crucial phase of mirror alignment has been completed for the James Webb Space Telescope, and the process resulted in the highest resolution infrared image ever taken from space
16 March 2022
By Leah Crane


While the purpose of this image was to focus on the bright star at the center for alignment evaluation, Webb's optics and NIRCam are so sensitive that the galaxies and stars seen in the background show up. At this stage of Webb?s mirror alignment, known as ?fine phasing,? each of the primary mirror segments have been adjusted to produce one unified image of the same star using only the NIRCam instrument. This image of the star, which is called 2MASS J17554042+6551277, uses a red filter to optimize visual contrast.

The James Webb Space Telescope focused on this bright star to align its mirrors
NASA/STScI

The James Webb Space Telescope (JWST) has reached a crucial phase in the alignment of its mirrors. Images from this process have shown that everything is working even better than expected, and the telescope’s operators say that its performance will be able to meet or even exceed the goals that were originally set for it.

JWST peers into the cosmos with the help of 18 gold-plated hexagonal mirrors. For it to work properly, all of these mirrors have to be aligned with extraordinary precision – within nanometres – so that they act as one. When the observatory sent back its first images in February, the mirrors weren’t yet aligned and the images were blurry. Now, although the alignment process isn’t quite complete, the image is crystal clear.
“This is as sharp an image as you can get from a telescope of this size,” said JWST scientist Marshall Perrin at the Space Telescope Science Institute in Maryland during a 16 March press conference. It is the highest resolution infrared image ever taken from space.

Read more: How the James Webb telescope will rewrite the story of the universe
The picture itself shows a bright star called 2MASS J17554042+6551277. If the alignment hadn’t been precise enough, there would be multiple copies of the star in the image, but it shows that the mirrors are now all working together to create a single image of a star flanked by distant galaxies.
“The telescope performance so far is everything that we dared hope,” said JWST scientist Jane Rigby at NASA’s Goddard Space Flight Center in Maryland during the press conference. There are a few more alignment steps before the observatory can take its first science images, which are expected in June or July.

This image of a single star is only the beginning. Once JWST begins taking science images, it should help unravel some of the universe’s biggest mysteries, from exoplanet habitability to dark energy.

James Webb Space Telescope sends back highest resolution infrared image ever taken from space
26,719 views
Mar 17, 2022
View: https://www.youtube.com/watch?v=P779qATKFNs&t=5s



 

jward

passin' thru
ohh ahhh so booful <3

James Webb Space Telescope enters 'homestretch' of commissioning with stunning image

By Elizabeth Howell published about 19 hours ago
We've never seen a neighboring galaxy like this before.

Old Man Weasel
7 hours ago (edited)

According to the official JWST site, the cameras are still being fine tuned. The image shown here is still a preliminary image....once all the fine tuned calibrations are completed, I'm sure we'll all be amazed! Considering all the obstacles that needed to be overcome, the JWST is one amazing new space telescope that will surely impress us, and grant us more knowledge of how minuscule we really are in the grand scheme of things! I'm glad this channel at least offers the ability to comment, as I've seen several channels promoting "JWST" images (which were really Hubble images), that blocked the ability to comment, when it was still undergoing instrument calibrations...as they were just seeking an attempt to scoop viewers. The image posted here is at least a legitimate JWST image!
View: https://www.youtube.com/watch?v=3QdcoMyF-Xg



Click here for more Space.com videos...

The Large Magellanic Cloud is sharper than ever in the infrared eyes of the James Webb Space Telescope.
As the $10 billion observatory enters the "homestretch" of its commissioning work, according to officials, Webb's latest image showed off the telescope's literally stellar performance using its coldest instrument, the Mid-Infrared Instrument (MIRI).

The new MIRI image showed the chemistry of interstellar gas in the best detail yet, including emission from molecules of carbon and hydrogen called "polycyclic aromatic hydrocarbons," considered some of life's building blocks. This imaging capability is crucial to help Webb understand how stars and protoplanetary systems are formed, officials said during a livestreamed news conference Monday (May 9).

"This is a really nice science example of what Webb will do for us in the coming years," Chris Evans, the telescope's project scientist at the European Space Agency, a partner on the mission, said during the event.
Live updates: NASA's James Webb Space Telescope mission
Related: How the James Webb Space Telescope works in pictures

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A comparison of views of the same part of the sky as seen by NASA's retired Spitzer Space Telescope and the newly launched James Webb Space Telescope. (Image credit: NASA/JPL-Caltech (left), NASA/ESA/CSA/STScI (right))
"We've done a lot of studies of star and planet formation in our own galaxy, but here we're looking at it in the Magellanic Clouds, so small external galaxies, where they're chemically less evolved than our own Milky Way," Evans added. "So this gives us a chance to look at the processes of star and planet formation... in a very different environment to our own galaxy."
The image, taken at 7.7 microns, shows a sharp view of the nearby Large Magellanic Cloud that is a dwarf galaxy neighbor to the Milky Way. Alongside the Webb image, engineers re-released an image from the now-retired Spitzer Space Telescope at 8.0 microns. Spitzer was a pioneer in its day in generating high-resolution images of the near- and mid-infrared universe, but Webb is much more powerful.

Spitzer did "amazing things," Evans said, but he noted that observatory was limited by its spatial resolution, as it was optimized for wide-field surveys that capture celestial objects in context.
By comparison, Webb's detailed, close-up perspective will provide "an amazing view of the processes in a different galaxy for the first time, cutting through the dust," Evans said. "We're using the mid-infrared to look through the material that otherwise would be obscured at visible wavelengths."
In addition, Webb has a much larger primary mirror, improved detectors and a superior observation point when compared with Spitzer; the now-retired telescope used to operate in an Earth-trailing orbit, as opposed to Webb's orbit at Earth-sun Lagrange point 2, about 930,000 miles (1.5 million kilometers) away. These factors will allow the new telescope to access infrared information with more clarity than its predecessor.

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The James Webb Space Telescope will be able to see the first stars and galaxies that emerged in the universe after the Big Bang. (Image credit: ESA/ATG medialab)
Webb has been clicking through commissioning milestones with few issues. Engineers are now in the final tweaking stages to the instruments, now that all of the mirrors have cooled to the deep-space temperatures that infrared observations require.
The LMC was identified as an ideal release target given that the Hubble Space Telescope and other observatories have studied it before. Knowing the locations of the galaxy's stars is a key advantage for scientists, Michael McElwain, Webb observatory project scientist at NASA's Goddard Space Flight Center in Maryland, said in the same press conference.
"We can use them [the stars] for astrometric calibrations," he explained, adding that this is important to calibrate the science instruments. "Of course, these images are also very spectacular."

In the near future, mission personnel will also test Webb's ability to track objects in the solar system, such as planets, satellites, rings, asteroids and comets. Scientists will be focused on making sure Webb can do this properly, given that the observatory is particularly sensitive to starlight.

Related stories:
NASA's $10 billion James Webb Space Telescope launches on epic mission to study early universe
James Webb Space Telescope: The scientific mysteries no other observatory could unravel
James Webb Space Telescope: The engineering behind a 'first light machine' that is not allowed to fail

"We will also measure changes in the telescope alignment as we point the telescope to different locations," Evans said. To test this, Webb will soon swing between slightly hotter and colder attitudes, so everyone can learn how quickly its mirrors heat up and cool down as the observatory slews in space.
While officials still have not released information on which commissioning target Webb will focus on first when its testing work completes, they emphasized the observatory remains on schedule to begin its early release science this summer.
"When this phase is complete, we'll be ready to turn the science instruments loose on the universe," Evans said.
Follow Elizabeth Howell on Twitter @howellspace. Follow us on Twitter @Spacedotcom and on Facebook.
 

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Lone_Hawk

Resident Spook
I am truly excited about this project. Hubble was a real leap in this technology, but now it is a model A in comparison.
 

jward

passin' thru
Astronomers will train James Webb Telescope's high-precision spectrographs on two intriguing rocky exoplanets

by Space Telescope Science Institute




Illustration of exoplanet 55 Cancri e, a rocky planet with a diameter almost twice that of Earth orbiting just 0.015 astronomical units from its Sun-like star. Because of its tight orbit, the planet is extremely hot, with dayside temperatures reaching 4,400 degrees Fahrenheit (about 2,400 degrees Celsius). Credit: NASA, ESA, CSA, Dani Player (STScI)
With its mirror segments beautifully aligned and its scientific instruments undergoing calibration, NASA's James Webb Space Telescope is just weeks away from full operation. Soon after the first observations are revealed this summer, Webb's in-depth science will begin.


Among the investigations planned for the first year are studies of two hot exoplanets classified as "super-Earths" for their size and rocky composition: the lava-covered 55 Cancri e and the airless LHS 3844 b. Researchers will train Webb's high-precision spectrographs on these planets with a view to understanding the geologic diversity of planets across the galaxy, and the evolution of rocky planets like Earth.


Super-hot super-earth 55 Cancri e


55 Cancri e orbits less than 1.5 million miles from its sun-like star (one twenty-fifth of the distance between Mercury and the sun), completing one circuit in less than 18 hours. With surface temperatures far above the melting point of typical rock-forming minerals, the day side of the planet is thought to be covered in oceans of lava.


Planets that orbit this close to their star are assumed to be tidally locked, with one side facing the star at all times. As a result, the hottest spot on the planet should be the one that faces the star most directly, and the amount of heat coming from the day side should not change much over time.


But this doesn't seem to be the case. Observations of 55 Cancri e from NASA's Spitzer Space Telescope suggest that the hottest region is offset from the part that faces the star most directly, while the total amount of heat detected from the day side does vary.

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Illustration comparing rocky exoplanets LHS 3844 b and 55 Cancri e to Earth and Neptune. Credit: NASA, ESA, CSA, Dani Player (STScI)

Does 55 Cancri e have a thick atmosphere?


One explanation for these observations is that the planet has a dynamic atmosphere that moves heat around. "55 Cancri e could have a thick atmosphere dominated by oxygen or nitrogen," explained Renyu Hu of NASA's Jet Propulsion Laboratory in Southern California, who leads a team that will use Webb's Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI) to capture the thermal emission spectrum of the day side of the planet. "If it has an atmosphere, [Webb] has the sensitivity and wavelength range to detect it and determine what it is made of," Hu added.




Or is it raining lava in the evening on 55 Cancri e?


Another intriguing possibility, however, is that 55 Cancri e is not tidally locked. Instead, it may be like Mercury, rotating three times for every two orbits (what's known as a 3:2 resonance). As a result, the planet would have a day-night cycle.


"That could explain why the hottest part of the planet is shifted," explained Alexis Brandeker, a researcher from Stockholm University who leads another team studying the planet. "Just like on Earth, it would take time for the surface to heat up. The hottest time of the day would be in the afternoon, not right at noon."


Brandeker's team plans to test this hypothesis using NIRCam to measure the heat emitted from the lit side of 55 Cancri e during four different orbits. If the planet has a 3:2 resonance, they will observe each hemisphere twice and should be able to detect any difference between the hemispheres.


In this scenario, the surface would heat up, melt, and even vaporize during the day, forming a very thin atmosphere that Webb could detect. In the evening, the vapor would cool and condense to form droplets of lava that would rain back to the surface, turning solid again as night falls.



Possible thermal emission spectrum of the hot super-Earth exoplanet LHS 3844 b, as measured by Webb’s Mid-Infrared Instrument. A thermal emission spectrum shows the amount of light of different infrared wavelengths (colors) that are emitted by the planet. Researchers use computer models to predict what a planet’s thermal emission spectrum will look like assuming certain conditions, such as whether or not there is an atmosphere and what the surface of the planet is made of. Credit: NASA, ESA, CSA, Dani Player (STScI)

Somewhat cooler super-earth LHS 3844 b
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While 55 Cancri e will provide insight into the exotic geology of a world covered in lava, LHS 3844 b affords a unique opportunity to analyze the solid rock on an exoplanet surface.


Like 55 Cancri e, LHS 3844 b orbits extremely close to its star, completing one revolution in 11 hours. However, because its star is relatively small and cool, the planet is not hot enough for the surface to be molten. Additionally, Spitzer observations indicate that the planet is very unlikely to have a substantial atmosphere.


What is the surface of LHS 3844 b made of?


While we won't be able to image the surface of LHS 3844 b directly with Webb, the lack of an obscuring atmosphere makes it possible to study the surface with spectroscopy.


"It turns out that different types of rock have different spectra," explained Laura Kreidberg at the Max Planck Institute for Astronomy. "You can see with your eyes that granite is lighter in color than basalt. There are similar differences in the infrared light that rocks give off."
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Illustration of exoplanet LHS 3844 b, a rocky planet with a diameter 1.3 times that of Earth orbiting 0.006 astronomical units from its cool red dwarf star. The planet is hot, with dayside temperatures calculated to be greater than 1,000 degrees Fahrenheit (greater than about 525 degrees Celsius). Credit: NASA, ESA, CSA, Dani Player (STScI)

Kreidberg's team will use MIRI to capture the thermal emission spectrum of the day side of LHS 3844 b, and then compare it to spectra of known rocks, like basalt and granite, to determine its composition. If the planet is volcanically active, the spectrum could also reveal the presence of trace amounts of volcanic gases.


The importance of these observations goes far beyond just two of the more than 5,000 confirmed exoplanets in the galaxy. "They will give us fantastic new perspectives on Earth-like planets in general, helping us learn what the early Earth might have been like when it was hot like these planets are today," said Kreidberg.


These observations of 55 Cancri e and LHS 3844 b will be conducted as part of Webb's Cycle 1 General Observers program. General Observers programs were competitively selected using a dual-anonymous review system, the same system used to allocate time on Hubble.

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