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Rubin Observatory is rocking The Vera C. Rubin Observatory sits on a mountain peak in Chile. The observatory will soon begin real-time monitoring of the entire southern sky. Credit: RubinObs/NOIRLab/SLAC/NSF/DOE/AURA/P. Horalek (Institute of Physics in Opava) February 24 was the date a new information pipeline began for astronomers around the world. Their computers received a deluge of cosmic notifications — 800,000 alerts about new asteroids, supernovae, and other noteworthy changes in the night sky. The discoveries were made by the Simonyi Survey Telescope at the NSF-DOE Vera C. Rubin Observatory in Chile and distributed globally within about two minutes. Those notifications began the observatory’s Alert Production Pipeline, software developed at the University of Washington (UW) that may eventually produce up to seven million alerts per night. “Rubin’s alert system was designed to allow anyone to identify interesting astronomical events with enough notice to rapidly obtain time-critical follow-up observations,” said Eric Bellm, a research associate professor of astronomy at the UW who leads the Alert Production Pipeline Group for the Rubin Observatory. “Rubin will survey the sky at an unprecedented scale and allow us to find the most rare and unusual objects in the universe. We can’t wait to see the exciting science that comes from these data.” ## **A 10-year survey is coming** Sending out these alerts is one of the final steps before Rubin Observatory launches its Legacy Survey of Space and Time (LSST) later this year. During the LSST, Rubin will scan the Southern Hemisphere sky each night for 10 years to capture visible changes. To do that, it will use the largest digital camera ever built. In the LSST’s first year, Rubin is expected to capture images of more objects than all other optical observatories combined. Ever. The alert pipeline was developed by a team of researchers and software developers in the UW’s astronomy department. The team spent the past decade working with other data management teams around the country to figure out how to process the 10 terabytes of images that Rubin will produce every night. “Enabling real-time discovery on such a massive data stream has required years of technical innovation in image processing algorithms, databases and data orchestration. We’re thrilled to continue the UW’s legacy of excellence in data-driven science.” Bellm said. ## **Alert!** Each alert signals something that’s changed in the sky since Rubin last looked. By receiving them, scientists may catch supernovae in their earliest moments, discover and track possible Earth-threatening asteroids, and spot rare interstellar objects moving through the solar system. “The discoveries reported in these alerts reflect the power of NSF-DOE Rubin Observatory as a tool for astrophysics and the importance of sustained federal support,” said Kathy Turner, program manager in the High Energy Physics program in the U.S. Department of Energy’s Office of Science. “Rubin Observatory’s groundbreaking capabilities are revealing untold astrophysical treasures and expanding scientists’ access to the ever-changing cosmos.” Every 40 seconds each night, Rubin captures a new region of the sky. It then sends the data from Chile to the U.S. Data Facility at the SLAC National Accelerator Laboratory in California for initial processing. There, it’s compared to a template made from previous images of the same region to detect variations. With every change, the system generates a public alert within two minutes. “The scale and speed of the alerts are unprecedented,” says Hsin-Fang Chiang, a SLAC software developer leading operations for data processing at the USDF. “After generating hundreds of thousands of test alerts in the last few months, we are now able to say, within minutes, with each image, ‘Here is everything. Go.’” Finally, Rubin’s alerts are public, meaning anyone — researchers, students, or citizen scientists — can access and explore them.

Rubin Observatory is rocking February 24 was the date a new information pipeline began for astronomers around the world. Their computers received a deluge of cosmic notifications — 800,000 alert...

#Science #Observatories

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Rubin Observatory is rocking The Vera C. Rubin Observatory sits on a mountain peak in Chile. The observatory will soon begin real-time monitoring of the entire southern sky. Credit: RubinObs/NOIRLab/SLAC/NSF/DOE/AURA/P. Horalek (Institute of Physics in Opava) February 24 was the date a new information pipeline began for astronomers around the world. Their computers received a deluge of cosmic notifications — 800,000 alerts about new asteroids, supernovae, and other noteworthy changes in the night sky. The discoveries were made by the Simonyi Survey Telescope at the NSF-DOE Vera C. Rubin Observatory in Chile and distributed globally within about two minutes. Those notifications began the observatory’s Alert Production Pipeline, software developed at the University of Washington (UW) that may eventually produce up to seven million alerts per night. “Rubin’s alert system was designed to allow anyone to identify interesting astronomical events with enough notice to rapidly obtain time-critical follow-up observations,” said Eric Bellm, a research associate professor of astronomy at the UW who leads the Alert Production Pipeline Group for the Rubin Observatory. “Rubin will survey the sky at an unprecedented scale and allow us to find the most rare and unusual objects in the universe. We can’t wait to see the exciting science that comes from these data.” ## **A 10-year survey is coming** Sending out these alerts is one of the final steps before Rubin Observatory launches its Legacy Survey of Space and Time (LSST) later this year. During the LSST, Rubin will scan the Southern Hemisphere sky each night for 10 years to capture visible changes. To do that, it will use the largest digital camera ever built. In the LSST’s first year, Rubin is expected to capture images of more objects than all other optical observatories combined. Ever. The alert pipeline was developed by a team of researchers and software developers in the UW’s astronomy department. The team spent the past decade working with other data management teams around the country to figure out how to process the 10 terabytes of images that Rubin will produce every night. “Enabling real-time discovery on such a massive data stream has required years of technical innovation in image processing algorithms, databases and data orchestration. We’re thrilled to continue the UW’s legacy of excellence in data-driven science.” Bellm said. ## **Alert!** Each alert signals something that’s changed in the sky since Rubin last looked. By receiving them, scientists may catch supernovae in their earliest moments, discover and track possible Earth-threatening asteroids, and spot rare interstellar objects moving through the solar system. “The discoveries reported in these alerts reflect the power of NSF-DOE Rubin Observatory as a tool for astrophysics and the importance of sustained federal support,” said Kathy Turner, program manager in the High Energy Physics program in the U.S. Department of Energy’s Office of Science. “Rubin Observatory’s groundbreaking capabilities are revealing untold astrophysical treasures and expanding scientists’ access to the ever-changing cosmos.” Every 40 seconds each night, Rubin captures a new region of the sky. It then sends the data from Chile to the U.S. Data Facility at the SLAC National Accelerator Laboratory in California for initial processing. There, it’s compared to a template made from previous images of the same region to detect variations. With every change, the system generates a public alert within two minutes. “The scale and speed of the alerts are unprecedented,” says Hsin-Fang Chiang, a SLAC software developer leading operations for data processing at the USDF. “After generating hundreds of thousands of test alerts in the last few months, we are now able to say, within minutes, with each image, ‘Here is everything. Go.’” Finally, Rubin’s alerts are public, meaning anyone — researchers, students, or citizen scientists — can access and explore them.

Rubin Observatory is rocking February 24 was the date a new information pipeline began for astronomers around the world. Their computers received a deluge of cosmic notifications — 800,000 alert...

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🌍 Calling #citizen #observatories #worldwide!

Fellows gain access to #tools, #trainings, and a global peer-learning #network of citizen science initiatives.

🗓️ Applications close February 15
👉 Apply here: citiobs.eu/demonstratio...

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Controversial Chilean energy project scrapped, relieving astronomers Light pollution from green hydrogen plant would have threatened world’s largest telescopes

Controversial Chilean energy project scrapped, relieving astronomers | Science | AAAS www.science.org/content/arti... #astronomy #NightSky #Chile #Observatories #LightPollution

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The University Observatory (Observatoriet) in Frogner, Norway Free tours are regularly arranged at this 1833 observatory right behind Solli plass (check the official website). Although the observatory is today in the heart of Oslo, at the time of its construction the building would have dominated its surroundings; in fact, the observatory predates the 1849 completion of the royal palace. Designed by Christian Grosch (who also designed the University buildings on Karl Johans gate, as well as Oslo stock exchange), the observatory combined a professors residence with cutting edge observational equipment. Today the interior is beautifully preserved, and museum displays on the inside showcase maps and observational equipment used on site.
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Information on Service 'Order Observations at FAI Telescopes'

New in the #VirtualObservatory: “Order Observations at FAI Telescopes” by Fesenkov Astrophysical Institute
https://dachs.fai.kz/soft_order_obs/q/orderobs/info
#AutomatedTelescopes #Observatories #OpticalObservation #OpticalObservatories

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#Space #and #Astronomy #Telescopes #and #Observatories #Moon #Artemis #Program #Blue #Origin

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#Space #and #Astronomy #Telescopes #and #Observatories #Moon #Artemis #Program #Blue #Origin

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Meton's Observatory in Athina, Greece Meton, an ancient Greek astronomer who lived in Athens during the 5th century B.C., is best known for developing the Metonic cycle (although this was also known to the Babylonians). Also known as the _enneadecaeteris_ , or "19 years" in ancient Greek, the cycle is based on the fact that 235 lunar months are almost equal to 19 solar years. Since 235 equals 19 times 12 plus another seven months, by adding one extra lunar month seven times during a 19-year cycle, a calendar can be created that closely follows both the lunar phases and __ the solar seasons. Such calendars are called lunisolar. Examples include the Jewish Calendar, used today predominantly for religious observances, and the Christian Orthodox Church calendar, used to calculate the date of Easter. In contrast, the calendar many people are more familiar with—the Gregorian calendar—is a solar __ one that follows only the seasons of the year, not the phases of the moon. As such, when we specify, for example, the 15th of January, we immediately know which season it is but have no idea what phase the moon is in that day. A lunisolar calendar, on the other hand, would, within a degree of accuracy, indicate both the season and the lunar phase. The lunar phases were fundamental to ancient Athenians, as they defined the timing of their festivals. Behind the ancient podium on the Hill of the Pnyx, where Athenians once held their popular assemblies, visitors will find the site where Meton and his assistant Euctemon made their astronomical observations 2,500 years ago. The two astronomers were particularly interested in observing the sunrise at the summer solstice, which enabled them to establish the Metonic cycle. If you are lucky enough to be there on this important day, you'll notice that the sun rises from the peak of mount Lycabettus. Interestingly, on the shortest day of the year—the winter solstice—the sun rises from the summit of Hymettus. And, at the equinoxes, when day and night are of equal length, it rises from behind the Acropolis. It seems as if Meton knew exactly where to position his observatory!
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Guajara Observatory in Tenerife, Spain Astronomical observatories are found on mountain tops because the weather is much better there. However, this was not always known. The observatory on the peak of the Guajara was built to prove this. Historical observatories are often found at the edges, or even in the middle of cities. Often moving away only to avoid light pollution. However, as time progressed and instruments became better, a need arose for more stable and reliable weather conditions. Newton had already predicted that mountains would be the best place for such buildings in the late 17th century, but there was no need and interest in confirming this claim until the mid-19th century. The person to first attempt mountain observations was the Scottish Charles Piazzi Smyth, who came to Tenerife in 1856 and brought his equipment to the island’s third-highest peak. The observations were an astounding success, and a rush to build on mountains started soon after. The observatory was a simple construction made from rocks to block the wind, and a tarp to give cover. It was abandoned after the observations, but resettled later to photograph Halley's comet. During this setup, part of the structure was knocked down to expand it and include a dark room to develop photographic plates. After this the observatory was truly abandoned, but new and more advanced buildings started popping up in the neighboring Teide observatory. Today the site is a protected monument, commemorating the astronomical history of the island. Not much is left of the observatory, but one can still see its foundations and read about it from a sign. The view is also amazing.
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Oct. 21, 1897: Yerkes Observatory is dedicated In 1892, George Ellery Hale, a professor of astrophysics at the University of Chicago, convinced the university president to acquire two 40-inch telescope lens blanks. With funding from Charles Yerkes, a Chicago mass-transit tycoon looking to refurbish his image, Hale spearheaded the creation of an observatory to house the Great Refractor made with these blanks.Continue reading "Oct. 21, 1897: Yerkes Observatory is dedicated" The post Oct. 21, 1897: Yerkes Observatory is dedicated appeared first on Astronomy Magazine.
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Oct. 21, 1897: Yerkes Observatory is dedicated In 1892, George Ellery Hale, a professor of astrophysics at the University of Chicago, convinced the university president to acquire two 40-inch telescope lens blanks. With funding from Charles Yerkes, a Chicago mass-transit tycoon looking to refurbish his image, Hale spearheaded the creation of an observatory to house the Great Refractor made with these blanks.Continue reading "Oct. 21, 1897: Yerkes Observatory is dedicated" The post Oct. 21, 1897: Yerkes Observatory is dedicated appeared first on Astronomy Magazine.
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Oct. 21, 1897: Yerkes Observatory is dedicated In 1892, George Ellery Hale, a professor of astrophysics at the University of Chicago, convinced the university president to acquire two 40-inch telescope lens blanks. With funding from Charles Yerkes, a Chicago mass-transit tycoon looking to refurbish his image, Hale spearheaded the creation of an observatory to house the Great Refractor made with these blanks.Continue reading "Oct. 21, 1897: Yerkes Observatory is dedicated" The post Oct. 21, 1897: Yerkes Observatory is dedicated appeared first on Astronomy Magazine.
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Oct. 21, 1897: Yerkes Observatory is dedicated In 1892, George Ellery Hale, a professor of astrophysics at the University of Chicago, convinced the university president to acquire two 40-inch telescope lens blanks. With funding from Charles Yerkes, a Chicago mass-transit tycoon looking to refurbish his image, Hale spearheaded the creation of an observatory to house the Great Refractor made with these blanks.Continue reading "Oct. 21, 1897: Yerkes Observatory is dedicated" The post Oct. 21, 1897: Yerkes Observatory is dedicated appeared first on Astronomy Magazine.
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Oct. 21, 1897: Yerkes Observatory is dedicated In 1892, George Ellery Hale, a professor of astrophysics at the University of Chicago, convinced the university president to acquire two 40-inch telescope lens blanks. With funding from Charles Yerkes, a Chicago mass-transit tycoon looking to refurbish his image, Hale spearheaded the creation of an observatory to house the Great Refractor made with these blanks.Continue reading "Oct. 21, 1897: Yerkes Observatory is dedicated" The post Oct. 21, 1897: Yerkes Observatory is dedicated appeared first on Astronomy Magazine.
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#Space #and #Astronomy #Telescopes #and #Observatories #Solar #System #Private #Spaceflight #National

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#Space #and #Astronomy #Telescopes #and #Observatories #Solar #System #Private #Spaceflight #National

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We're on a paved plateau high up in the mountains under a sky of blindingly bright, vibrant blue. Our view to the distant peaks of the dry mountain ranges is blocked by four large structures here. Three of them are observatories: white block buildings topped with domes, each with a thick ridge on its curved surface indicating where it can be opened after rotation for viewing purposes. The observatories on the right and in the centre are the larger two and can be fully seen while the one to the left is smaller and behind two large shipping containers, only its dome peeking out over the top. Leftmost of all is a smaller observatory structure just in front of the containers, shaped like a large 20-sided die mounted on a platform reached by a ladder. It feels quiet and cool here.

We're on a paved plateau high up in the mountains under a sky of blindingly bright, vibrant blue. Our view to the distant peaks of the dry mountain ranges is blocked by four large structures here. Three of them are observatories: white block buildings topped with domes, each with a thick ridge on its curved surface indicating where it can be opened after rotation for viewing purposes. The observatories on the right and in the centre are the larger two and can be fully seen while the one to the left is smaller and behind two large shipping containers, only its dome peeking out over the top. Leftmost of all is a smaller observatory structure just in front of the containers, shaped like a large 20-sided die mounted on a platform reached by a ladder. It feels quiet and cool here.

#FotoVorschlag - Dinge, die mit O beginnen

Photo theme: something beginning with O

Some of the many #observatories at Cerro-Tololo in Chile when we visited in 2019.

#Photography #Travel #Chile #Observatory #Astronomy #CerroTololo #Telescope

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#Black #Holes #(Space) #Space #and #Astronomy #Telescopes #and #Observatories #Physics #Gravitation

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#Black #Holes #(Space) #Space #and #Astronomy #Telescopes #and #Observatories #Physics #Gravitation

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David Dunlap Observatory in Richmond Hill, Ontario When exploring the nooks and crannies of the bustling town of Richmond Hill, many folks overlook this small wooded park near the town's outskirts that houses a historic observatory. This massive white dome used to be the second-largest telescope in the world when it was built in 1935, and remains the largest in Canada. From 1935 to 2007, the observatory was at the forefront of astronomical discoveries, notably Thomas Bolton's 1972 work confirming the existence of a black hole in the Cygnus X-1 system. Since then, its been designated a National Historic Site by the federal government and hosts yearly astronomy programs and events, offering visitors public astronomy nights, educational programs, and hands-on activities, including a viewing through the observatory's 74-inch telescope. The complex is made up of two incredible buildings, the observatory and the administration building. Both structures are worth exploring, but the admin building is the real eye-catcher with its beautiful stonework and triple-domed roof. Overall, this location is a pleasure to visit, not only for its incredible history, but also for its beautiful architecture.
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Tired as anything but I couldn't resist. Who wouldn't want a photograph inside a telescope. #voorheesnj #telescopes #space #nasa #njaa #observatories #paulrobinsonobservatory

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#Stars #and #Galaxies #Space #and #Astronomy #Chemistry #Telescopes #and #Observatories #Nature

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Cannon and City Observatory, Calton Hill, Edinburgh, Scotland, UK 29.06.2006
#edinburgh #scotland #uk #architecture #cannon #cannons #architecturephotography #observatory #observatories #valokuvataivas

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City Observatory, Calton Hill, Edinburgh, Scotland, UK 29.06.2006
#edinburgh #scotland #uk #architecture #architecturephotography #observatory #observatories #valokuvataivas

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UH telescope on Maunakea earns global honor The UH 88 telescope designated as an IEEE Milestone, a significant honor spotlighting innovations that changed the world. The post UH telescope on Maunak...

#Research #astronomy #engineering #Institute #for #Astronomy […]

[Original post on hawaii.edu]

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#Large #Synoptic #Survey #Telescope #Telescopes #and #Observatories #Space #and #Astronomy #Stars

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Vera C. Rubin Observatory releases movies showing our dynamic universe The Simonyi Survey Telescope peers at the sky from inside the dome of the Vera C. Rubin Observatory. Credit: NSF-DOE Vera C. Rubin Observatory/H. Stockebrand It’s been an exciting morning, with the initial release of images from the The National Science Foundation–U.S. Department of Energy Vera C. Rubin Observatory. But these were just the first taste — a press conference this morning unveiled more images as well as videos to the world. “This observatory represents a giant leap in our ability to explore the cosmos and unwrap the mysteries of the universe,” said Kathy Turner, U.S. DOE Program Manager for Rubin Observatory, during the press conference. In addition to its ultra-wide field of view (9.62 square degrees), Rubin Observatory’s 8.4-meter Simonyi Survey Telescope and 3,200-megapixel LSST Camera can snap successive images and move on to a new area of the sky quickly as part of the planned Legacy Survey of Space and Time (LSST), which will begin later this year. That sets the stage for the telescope’s other exciting capability: creating time-stepped “movies” of the entire Southern Hemisphere sky for the next 10 years as part of the Legacy Survey of Space and Time (LSST). Why movies? “The sky is not static — it’s alive,” said Yusra AlSayyad, who manages the observatory’s image-processing algorithms, in a press release last month. Those algorithms allow the observatory to detect changes and issue alerts within seven seconds after each image is taken, resulting in millions of detections for astronomers to follow up on… per night. ## New asteroids Showing off that capability this morning is a video highlighting some of the thousands (yes, thousands!) of asteroids the observatory has already discovered just in this initial phase. Asteroids are notoriously difficult to spot, as they’re small (and thus faint) and are only detectable through their motion through the sky. That means a telescope needs to be taking many images of the same patch of sky over time to notice any foreground object that moves. And that is exactly what Rubin will do. Credit: NSF-DOE Vera C. Rubin Observatory This video shows new asteroids discovered by Rubin Observatory in a span of just 10 hours. In this short time, Not only does the image show the two-dimensional paths of the asteroids across image frames, but it also shows the new asteroids’ 3D positions in space within the solar system. Rubin caught sight of 2,104 previously unknown asteroids, seven of which are considered near-Earth objects whose orbits bring them to within some 28 million miles (45 million kilometers) of Earth. (Don’t worry, astronomers have determined that none of these will pose a hazard to our planet.) As of Monday morning, the discoveries have been reported to the Minor Planet Center at Harvard, said Rubin Observatory Director Zeljko Ivezic during the Monday press conference. He added, with regard to any object that might be found in the future that could be potentially hazardous: “As soon as we have a plausible discovery … within, sometimes even with less than 24 hours, everyone in the world will know that there is a potential object that could be hazardous. And they can get more data … [to] rule out the level of the danger. … Everyone in the world will be able to follow up on Rubin’s discoveries.” Within one year, the LSST will likely discover more asteroids than all those found by other telescopes combined. Within two years, the number of new asteroids is expected to reach into the millions. And some of these won’t be native to our own solar system, but interstellar interlopers like 1I/2017 U1 ʻOumuamua and 2I/Borisov. The observatory might discover 10 or 20 of these during the LSST, Ivezic said. He also noted that “If Planet Nine exists … Rubin is the best positioned observatory to discover it.” ## Stepping through time While many astronomical process take millions or billions of years to occur, some effect changes over minutes, hours, days, or weeks. Some variable stars, such as RR Lyrae stars, can briefly brighten within minutes or hours. Rubin’s sharp eye and sophisticated data analysis algorithms can catch these stars pulsating at distances previously unreachable by other observing programs, creating a three-dimensional map of these stars throughout our galaxy and helping astronomers study the distribution of dark matter in the Milky Way. And then there are sporadic one-time events, such as stars exploding or black holes swallowing a meal, which can light the night without warning for only a brief time before fading away. With telescope time so precious, astronomers must often balance the need for the long exposures in one location required to view faint or faraway objects with regularly scanning the sky to serendipitously catch new events. Of course, both of these goals are achievable with the Rubin Observatory’s technology and through the very design of the LSST. And building up a 10-year record of the sky means that “if something strange appears — an explosion, an object vanishing — we can rewind and see what led up to it,” AlSayyad said in the release. All changes in the sky each night will be published within a day, and catalogs will be released yearly. Any part of the sky that might be of interest — and any time that part of the sky was imaged — will be readily available to astronomers, allowing them to step through the time before, during, and after any detected event for a detailed look. “Once you’ve got the deep image, you go back to every single frame,” said Eli Rykoff, who is in charge of calibrating the images the observatory takes, in the release. “Then you ask: ‘What was the light like at this spot, at this moment?’ By repeating this process for all images, we can reconstruct light curves and track the evolution of an object’s brightness over time.” ## Flying through space But let’s not forget that ultra-wide field of view Rubin has, looking at a portion of the sky more than nine square degrees in a single shot. While the first images released showed only small portions — roughly 2 percent — of a larger image of the vast Virgo Cluster of galaxies, this new video gives a much better sense of just how immense the telescope’s field of view truly is, and how much of the cosmos it can capture in a single glimpse. “The entire Rubin team is so excited about this data. We have been talking about this data for over two decades. It’s finally here,” Ivezic said during the press conference as the video was unveiled. Credit: NSF-DOE Vera C. Rubin Observatory The video of the Virgo Cluster field comprises more than 1,100 images and takes us on a journey that starts with just two galaxies. But then it begins to move, pulling back and zooming around and around, uncovering colorful new galaxies at each turn. The video ultimately reveals a field of view 100 times as large as the small portions made available earlier today, with every bit of the view awash in galaxies — some 10 million in total. That’s just 0.05 percent of the 20 billion galaxies (containing a total of some 18 billion stars) Rubin is expected to observe by the end of its 10-year survey. If you want to view and zoom around this image, Rubin’s web display tool is available at https://skyviewer.app/ and offers both a guided view or the ability to explore the image on your own, bit by bit. The app also offers sonification, allowing you to explore not only the visual landscape with your eyes but also listen in on the cosmic “soundscape” with your ears. Cataloging so many galaxies will allow astronomers to answer questions that range from how galaxies interact and evolve to how clumps and clusters of galaxies are spread throughout the universe. That latter point is related to fundamental properties of our cosmos, including the elusive dark matter and dark energy that dominate it. So, Rubin will not only take pretty pictures and make movies of the sky, it will show us the very makeup of our universe in ultra-high-def and help astronomers answer some of the most fundamental questions there are about why our universe is the way it is and where it might be headed. “We believe the work of this observatory will help us find long-sought answers and ask new and better questions. It will also provide the best map mankind has yet made of our region of the universe,” said Michael Kratsios, Director of the White House Office of Science and Technology Policy. Many of those questions will be about things we haven’t even discovered yet, or perhaps have seen only once or twice before in the history of astronomy. “When you’re talking [about] a survey where everything is on the scale of billions, those one-in-a-million events aren’t that rare anymore,” said Claire Higgs, Astronomy Outreach Specialist for the Rubin Observatory. “You get lots of one-in-a-million events if you’re talking on the scale of billions.” Rubin is now poised to utterly transform our view of the cosmos in nearly countless ways. The journey is just getting started — so stay tuned.

Vera C. Rubin Observatory releases movies showing our dynamic universe It’s been an exciting morning, with the initial release of images from the The National Science Foundation–U.S. Department...

#Science #Asteroids #Galaxies #Observatories

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