Ten years ago, on 19 December 2013, our billion star-mapping satellite Gaia launched.
Since then, Gaia has been scanning the sky and gathering an enormous amount of data on the positions and motions of 1.8 billion stars, enabling discoveries about the history of our galaxy.
Gaia is creating an extraordinarily precise three-dimensional map of more than a billion stars throughout our Milky Way galaxy and beyond, mapping their motions, luminosity, temperature and composition.
This huge stellar census will provide the data needed to tackle an enormous range of important questions related to the origin, structure and evolutionary history of our galaxy.
Gaia’s catalogue is ever-growing containing data on stars and other cosmic objects such as galaxies, exoplanets, and binary stars. Here’s to more discoveries!
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Today, our Gaia mission releases a goldmine of knowledge about our galaxy and beyond. Among other findings, the star surveyor surpasses its planned potential to reveal half a million new and faint stars in a massive cluster, identify over 380 possible cosmic lenses, and pinpoint the positions of more than 150 000 asteroids within the Solar System.
This image was captured by NIRCam, Webb’s primary near-infrared camera, and contains the lensing galaxy cluster SDSS J1226+2149. It lies at a distance of around 6.3 billion light-years from Earth, in the constellation Coma Berenices. By combining Webb’s sensitivity with the magnifying effect of gravitational lensing, astronomers were able to use this gravitational lens to explore the earliest stages of star formation in distant galaxies. To do so, they relied on earlier studies by the NASA/ESA Hubble Space Telescope, which provided the ‘prescription’ for this gravitational lens.
Credit: ESA/Webb, NASA & CSA, J. Rigby Music: Stellardrone – Twilight
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
This image takes the viewer to space to finish at Webb’s view of the galaxy merger II ZW 96.
This pair of galaxies is roughly 500 million light-years from Earth and lies in the constellation Delphinus, close to the celestial equator. As well as the wild swirl of the merging galaxies, a menagerie of background galaxies are dotted throughout the image. Learn more about the object here.
Credit: ESA/Webb, NASA, CSA, L. Armus, A. Evans, SDSS, E. Slawik, N. Risinger, M. Zamani (ESA/Webb), N. Bartmann (ESA/Webb) Music: Tonelabs – The Red North
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
These are termed “tidal disruption events.” But the wording belies the complex, raw violence of a black hole encounter. There is a balance between the black hole’s gravity pulling in star stuff, and radiation blowing material out. In other words, black holes are messy eaters. Astronomers are using Hubble to find out the details of what happens when a wayward star plunges into the gravitational abyss.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
This video takes the viewer on a journey to NGC 346, one of the most dynamic star-forming regions in nearby galaxies, as seen by the NASA/ESA/CSA James Webb Space Telescope.
NCG 346 is located in the Small Magellanic Cloud (SMC), a dwarf galaxy close to our Milky Way.
Credit: ESA/Webb, NASA, CSA, ESO, ESA/Hubble, Digitized Sky Survey 2, A. Nota, N. Bartmann, M. Zamani Music: Music for the Zoom: Tonelabs – The Red North
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
The first clue came when the star mysteriously darkened in late 2019. An immense cloud of obscuring dust formed from the ejected surface as it cooled. Astronomers have now pieced together a scenario for the upheaval. And the star is still slowly recovering; the photosphere is rebuilding itself. And the interior is reverberating like a bell that has been hit with a sledgehammer, disrupting the star’s normal cycle. This doesn’t mean the monster star is going to explode any time soon, but the late-life convulsions may continue to amaze astronomers.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
These spectacular images feature the spiral galaxy IC 5332, taken by the @NASA/ESA Hubble Space Telescope and the NASA/ESA/ @Canadian Space Agency James Webb Space Telescope. The images display the powerful capabilities that both world-leading space telescopes provide, especially when combining their data.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
The Small Magellanic Cloud has a simpler chemical composition than the Milky Way, making it similar to the galaxies found in the younger Universe, when heavier elements were more scarce. Because of this, the stars in the Small Magellanic Cloud burn hotter and so run out of their fuel faster than in our Milky Way. Though a proxy for the early universe, at 200 000 light-years away the Small Magellanic Cloud is also one of our closest galactic neighbours.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Thousands of never-before-seen young stars are spotted in a stellar nursery called 30 Doradus, captured by the @NASA/ESA/@Canadian Space Agency James Webb Space Telescope. Nicknamed the Tarantula Nebula for the appearance of its dusty filaments in previous telescope images, the nebula has long been a favourite for astronomers studying star formation. In addition to young stars, Webb reveals distant background galaxies, as well as the detailed structure and composition of the nebula’s gas and dust.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
New images of the spectacular Phantom Galaxy, M74, showcase the power of space observatories working together in multiple wavelengths. In this case, data from the @NASA / ESA / @canadianspaceagency James Webb Space Telescope and the NASA/ESA Hubble Space Telescope compliment each other to provide a comprehensive view of the galaxy.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
NASA revealed the first five full-color images and spectrographic data from the world’s most powerful space telescope, the James Webb Space Telescope, a partnership with ESA (European Space Agency), and CSA (Canadian Space Agency). The world got its first look at the full capabilities of the mission at a live event streamed from the agency’s Goddard Space Flight Center in Greenbelt, Maryland, on July 12, 2022.
The event showcased these targets: – Carina Nebula: A landscape speckled with glittering stars and cosmic cliffs – Stephan’s Quintet: An enormous mosaic with a visual grouping of five galaxies – Southern Ring Nebula: A nebula with rings of gas and dust for thousands of years in all directions – WASP 96-b: A distinct signature of water in the atmosphere of an exoplanet orbiting a distant Sun-like star – SMACS 0723: The deepest and sharpest infrared image of the distant universe to date
The full set of the telescope’s first full-color images and spectroscopic data are available at: https://nasa.gov/webbfirstimages
One of the surprising discoveries coming out of Gaia data release 3, is that Gaia is able to detect starquakes – tiny motions on the surface of a star – that change the shapes of stars, something the observatory was not originally built for.
Previously, Gaia already found radial oscillations that cause stars to swell and shrink periodically, while keeping their spherical shape. But Gaia has now also spotted other vibrations that are more like large-scale tsunamis. These nonradial oscillations change the global shape of a star and are therefore harder to detect.
Nonradial oscillation modes cause a star’s surface to move while it rotates, as shown in the animation. Dark patches are slightly cooler than bright patches, giving rise to periodic changes in the brightness of the star. The frequency of the rotating and pulsating stars was increased 8.6 million times to shift them into the audible range of humans.
Credit: ESA/Gaia/DPAC, CC BY-SA 3.0 IGO. Acknowledgement: Animation and sonification were created by: Dr. Joey Mombarg, KU Leuven, Belgium. Based on information from Gaia Data Release 3: Pulsations in main-sequence OBAF stars as observed by Gaia by the Gaia Collaboration, De Ridder et al., 2022, submitted to A&A. Van Reeth et al. 2015, ApJS 218, id.2, 32 pp. Mombarg et al. 2021, A&A 650, id.A58, 23 pp.
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Since its launch in 2013 ESA’s Gaia observatory has been mapping our galaxy from Lagrange point 2, creating the most accurate and complete multi-dimensional map of the Milky Way. By now two full sets of data have been released, the first set in 2016 and a second one in 2018. These data releases contained stellar positions, distances, motions across the sky, and colour information, among others. Now on 13 June 2022 a third and new full data set will be released. This data release will contain even more and improved information about almost 2 billion stars, Solar System objects and extragalactic sources. It also includes radial velocities for 33 million stars, a five-time increase compared to data release 2. Another novelty in this data set is the largest catalogue yet of binary stars in the Milky Way, which is crucial to understand stellar evolution.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Watch over one hour of our planet, seen from the International Space Station, in 4K resolution. This compilation was made from video taken by ESA astronauts, mostly by Thomas Pesquet during his first mission, Proxima, and ESA astronaut Alexander Gerst on his second mission, Horizons, as well as footage from Samantha Cristoforetti’s Futura mission and Paolo Nespoli’s Vita mission.
Flying 400 km above our amazing planet Earth, the Space Station travels at 28 800 km/h to stay in orbit. The videos are in real time and not sped up or edited. Most of the scenes were filmed in the European-built Cupola module, the Space Station’s observatory.
On 21 April 2001, the first ESA astronaut Umberto Guidoni arrived at the Space Station. Since then, the Space Station has grown immensely, as have the number of Europeans to have worked in it, together with the science experiments performed in orbit.
Europe contributes around 8% of the running costs of the International Space Station, but has built a large part of the structure, including ESA’s Columbus laboratory, the Cupola observatory, the Tranquillity and Harmony modules, as well as the computers that collect data and provide navigation, communications and operations for the Russian segment.
ESA also provided the Space Station with supplies and boosted its orbit through five Automated Transfer Vehicles, the heaviest and most versatile Space Station supply ferry. This programme evolved into the European Service Modules that ESA is supplying for @NASA’s Artemis programme, taking humans forward to the Moon and thus continuing the exemplary international collaboration beyond Earth’s orbit.
Since Umberto’s mission, there have been 26 further ESA astronaut missions to the International Space Station, with astronauts flying to Station on either the Russian Soyuz or US Space Shuttle spacecraft.
Thomas Pesquet’s second mission, Alpha, is the 28th mission for ESA, with ESA astronaut Matthias Maurer already lined up for his first flight later this year, and ESA astronaut Samantha Cristoforetti scheduled for the 30th ESA International Space Station mission in 2022.
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Each year, the NASA/ESA Hubble Space Telescope dedicates a small portion of its precious observing time to taking a special anniversary image, showcasing particularly beautiful and meaningful objects. These images continue to challenge scientists with exciting new surprises and to enthral the public with ever more evocative observations.
To celebrate Hubble’s 30th anniversary, let’s look back at the beauty and science behind each of the anniversary images unveiled as of 2005. In this video, we will also feature the very special 2020 Hubble Space Telescope 30th anniversary image.
Credit:
Directed by: Bethany Downer
Visual design and editing: Martin Kornmesser
Written by: Bethany Downer
Narration: Sara Mendes da Costa
Images & VIdeos: NASA, ESA, M.Kornmesser, L. Calçada, ESO, NAOJ, G. Bacon, L. Frattare, Z. Levay and F. Summers (STScI/AURA), D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S.E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), L. Bedin (INAF, Padua), C. Evans (STFC), H. Sana (Amsterdam), N. Langer (Bonn), P. Crowther (Sheffield), A. Herrero (IAC, Tenerife), N. Bastian (USM, Munich), and E. Bressert (ESO), the Hubble Heritage Team, T. Davis, L. Frattare, Z. Levay, (Viz 3D team, STScI), J. Anderson (STScI), the Hubble Heritage Team (STScI/AURA), A. Nota (ESA/STScI), and the Westerlund 2 Science Team, Eckhard Slawik (e.slawik@gmx.net).
Music: Johan B. Monell (www.johanmonell.com
Web and technical support: Raquel Yumi Shida
Executive producer: Mariya Lyubenova
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
On 24 April 1990 the NASA/ESA Hubble Space Telescope was sent into orbit aboard the space shuttle Discovery, the first space telescope of its kind. It offered a new view of the Universe and has, for 30 years, reached and surpassed all expectations, beaming back data and images that have changed scientists’ understanding of the Universe and the public’s perception of it. Hubble’s discoveries have revolutionised nearly all areas of current astronomical research, from planetary science to cosmology, and its pictures are unmistakably out of this world.
This video revisits some of Hubble’s biggest science discoveries throughout its three decades of operation to celebrate the telescope’s 30th anniversary.
Credit:
Directed by: Bethany Downer
Visual design and editing: Martin Kornmesser
Written by: Bethany Downer
Narration: Sara Mendes da Costa
Images & Videos: NASA, ESA, M.Kornmesser, L. Calçada, ESO, G. Bacon (STScI), theHubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration, and H. Bond (STScI and Pennsylvania State University), A. Feild (STScI), and A. Riess (STScI/JHU), D. Jewitt (UCLA), F. Summers, Z. Levay, J. DePasquale, L. Hustak, L. Frattare, M. Robberto (STScI), R. Hurt (Caltech/IPAC) Acknowledgement: R. Gendler, spaceengine.org.
Music: Johan B. Monell (www.johanmonell.com)
Web and technical support: Raquel Yumi Shida
Executive producer: Mariya Lyubenova
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
This month marks the 30th anniversary of the international Hubble Space Telescope.
Launched on 24 April 1990, and deployed from the Space Shuttle Discovery cargo bay a day later (25 April 1990), the telescope has given us a new perspective on the Universe.
The joint NASA/ESA mission has shown us distant galaxies and spectacular nebulae. It has revealed supermassive black holes and planets in distant solar systems; and has proved that the Universe is not only expanding, the expansion is accelerating.
Hubble’s mission has also been eventful. When it was first launched, a defect in the mirror meant it sent back blurry images. Since then, five servicing missions have enabled the telescope to be improved and upgraded. Today, it is still going strong.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
🇳🇱Jump to the Dutch section: 0:57:50
🇩🇪Jump to the German section: 1:57:57
🇮🇹Jump to the Italian section: 2:57:44
🇫🇷Jump to the French section: 3:57:50
🇬🇧Jump to the English section: 4:58:41
Asteroid Day and the European Space Agency connected Europe and the world with astronauts, scientists and performers bringing a message of hope and support for those facing the global Coronavirus crisis.
This online programme was broadcast sequentially in Dutch, German, Italian, French and English to inspire armchair explorers everywhere.
Featuring
André Kuipers, Frank De Winne, Matthias Maurer, Alexander Gerst, Thomas Reiter, Samantha Cristoforetti, Jean-François Clervoy, Thomas Pesquet, Timothy Peake, Rusty Schweickart, Nicole Stott, Tom Jones, Dumitru-Dorin Prunariu, Anousheh Ansari
Special guests
Gianluca Masi, Jan Wörner, Mayim Bialik, Murad Osmann, Alison Pill, Paulina Chávez, Angélique Kidjo, Grig Richters
Moderators
Sander Koenen, Ranga Yogeshwar, Rossella Panarese, Bruce Benamran, Brian Cox
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
What is ESA’s Characterising Exoplanet Satellite, Cheops, and how will it improve our knowledge of exoplanets? Find out more in this interview with Kate Isaak, ESA Cheops project scientist.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
A powerful space telescope, due for launch from Europe’s Spaceport in French Guiana on 17 December 2019, will give scientists a new insight into the nature of planets outside our Solar System.
Cheops, the ‘Characterising Exoplanet Satellite’, will study known exoplanets that are orbiting bright stars.
More than 4000 exoplanets have been discovered and Cheops will be targeting known planets between the size of Earth and Neptune, to find out more about their composition, internal structure and whether they might be able to support life.
Cheops’ mission is a partnership between ESA and Switzerland with additional contributions from Austria, Belgium, France, Germany, Hungary, Italy, Portugal, Spain, Sweden and the UK.
This film examines the nature of exoplanets, the challenge of exoplanet exploration and features the Cheops Science Operations Centre in Geneva, it includes interviews with Didier Queloz, Chair of the Cheops Science Team and 2019 Nobel Physics Laureate, University of Geneva; Willy Benz, Cheops Principal Investigator, University of Bern; and Matthias Beck, Cheops Ground Segment Manager, University of Geneva).
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
ESA’s first mission dedicated to investigating planets outside our solar system is scheduled for launch on a Soyuz rocket from the European spaceport in French Guiana on 17 December 2019.
Cheops – Characterising ExOPlanet Satellite – will study known exoplanets that are orbiting bright stars. The aim is to obtain detailed information about these planets to find out more about their composition and internal structure.
The mission is a partnership between ESA and Switzerland with additional contributions from Austria, Belgium, France, Germany, Hungary, Italy, Portugal, Spain, Sweden and the UK.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
Launched in December 2013, the Gaia mission is revolutionising our understanding of the Milky Way. The space telescope is mapping our galaxy in unprecedented detail – measuring the position, movement and distance of stars.
At a meeting in Groningen in the Netherlands, scientists have been discussing the challenge of processing and visualising Gaia data.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
Scientists at the Geneva Observatory in Switzerland will be processing data from Cheops, ESA’s Characterising Exoplanet Satellite, scheduled to launch soon to study planets orbiting stars outside our Solar System.
The Observatory has a rich history studying exoplanets. In 1995, Michel Mayor and Didier Queloz discovered the first exoplanet orbiting a Sun-like star. Now, over 4000 planets are known around stars other than the Sun.
By observing stars that are already known to host exoplanets, Cheops will make measure very precisely the sizes of planets in the super-Earth to Neptune size range. Combined with existing measurements of planet masses, the Cheops data will make it possible to determine the density of these planets, giving us vital clues about its composition and structure, indicating for example if it is predominantly rocky or gassy, or perhaps harbours significant oceans.
The Cheops mission is a partnership between ESA and Switzerland with important contributions from Austria, Belgium, France, Germany, Hungary, Italy, Portugal, Spain, Sweden, and the United Kingdom. The Cheops launch slot is scheduled for the last quarter of 2019. This film contains contributions from Didier Queloz, Chair of the Cheops Science Team (University of Geneva); Willy Benz, the Cheops Principal Investigator (University of Bern); and the Cheops Ground Segment Manager, Matthias Beck (University of Geneva).
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
ESA is the only space agency in the world that covers the whole range of space activities. We’re exploring our Solar System and unlocking the secrets of the Universe. We’re monitoring space and protecting our planetary environment. We’re making space accessible and developing the technologies for the future, and we’re also using space to benefit citizens and meet future challenges on Earth.
In November 2019, European ministers in charge of space activities will gather at the Space19+ conference in Seville, Spain, to decide on ESA’s vision for the future of Europe in space. Space19+ will be an opportunity to direct Europe’s ‘next generation’ ambitions in space, and address the challenges facing not only the European space sector but also European society as a whole.
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
Launched in December 2013, ESA’s Gaia satellite has been scanning the sky to perform the most precise stellar census of our Milky Way galaxy, observing more than one billion stars and measuring their positions, distances and motions to unprecedented accuracy.
The second Gaia data release, published in April, has provided scientists with extraordinary data to investigate the formation and evolution of stars in the Galaxy and beyond, giving rise to hundreds of scientific studies that are revolutionising our view of the cosmos.
Credits: ESA / CNES / Arianespace; ESA / Gaia / DPAC; Gaia Sky / S. Jordan / T. Sagristà; Koppelman, Villalobos and Helmi; Marchetti et al. 2018; NASA / ESA / Hubble; ESO, M. Kornmesser, L. Calçada
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ESA is Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.
Astronomy is undergoing a revolution with the release of precision data on 1.7 billion stars in our galaxy from the Gaia space telescope. We head to the historic Observatory of Paris and ESA’s ESTEC base in the Netherlands to find out more.
It’s fair to say that science has been waiting for centuries, or even millennia for such a detailed survey of the Milky Way, and right now star-gazers are swamped with fresh, high-quality data that they can use to answer every question about the galaxy they ever wanted to ask.
The second data release of ESA’s Gaia mission has produced an extraordinary catalogue of over one and a half billion stars in our galaxy. Based on observations between July 2014 to May 2016, it includes the most accurate information yet on the positions, brightness, distance, motion, colour and temperature of stars in the Milky Way as well as information on asteroids and quasars.
Animated 3D view of the sky as observed by ESA’s Gaia satellite using information from the mission’s second data release.
The bright band in the left half of the image is the Milky Way, where most of the stars in our Galaxy reside. The animation starts with the Orion constellation at the centre; we then move towards the neighbouring Taurus constellation and to the Hyades star cluster, which is part of this constellation. Hyades is the closest open cluster to the Solar System, some 150 light-years away.
The animation first shows the 3D structure of the cluster, based on accurate position and distance information from Gaia. Then an animated view of the future motions of stars is shown – both in Hyades and beyond. This is based on Gaia’s measurements of the velocity of stars across the sky, also known as proper motion.
Credit: ESA/Gaia/DPAC, CC BY SA 3.0 IGO
Acknowledgement: Gaia Data Processing and Analysis Consortium (DPAC); Gaia Sky; S. Jordan / T. Sagristà, Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Germany
Animated view of 14 099 asteroids in our Solar System, as viewed by ESA’s Gaia satellite using information from the mission’s second data release. The orbits of the 200 brightest asteroids are also shown, as determined using Gaia data.
In future data releases, Gaia will also provide asteroid spectra and enable a complete characterisation of the asteroid belt. The combination of dynamical and physical information that is being collected by Gaia provides an unprecedented opportunity to improve our understanding of the origin and the evolution of the Solar System.
Credit: ESA/Gaia/DPAC, CC BY SA 3.0 IGO
Acknowledgement: Gaia Data Processing and Analysis Consortium (DPAC); Orbits: Gaia Coordinating Unit 4; P. Tanga, Observatoire de la Côte d’Azur, France; F. Spoto, IMCCE, Observatoire de Paris, France; Animation: Gaia Sky; S. Jordan / T. Sagristà, Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Germany
A 360° animated view of the entire sky on 25 April 2018.
After a few seconds, the stars start moving in the sky according to parallax, an apparent shift caused by Earth’s yearly motion around the Sun. Then, constellation outlines appear as visual aids. Finally, stars start moving according to their true motion through space, which is visible on the sky as proper motion. Parallaxes have been exaggerated by 100 000 and proper motions have been speeded up by one trillion (10^12) to make them visible in this animation. This animation is based on data from the second data release of ESA’s Gaia satellite, which has measured the positions, parallaxes and motions of more than one billion stars across the sky to unprecedented accuracy.
ESA/Gaia/DPAC, CC BY SA 3.0 IGO
Acknowledgement: Gaia Data Processing and Analysis Consortium (DPAC); Gaia Sky; S. Jordan / T. Sagristà, Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Germany
On 25 April 2018, ESA’s Gaia mission will publish its much awaited second data release, including high-precision measurements of nearly 1.7 billion stars in our Galaxy.
Scientists who have been working on creating and validating the data contained in the catalogue tell us why they are waiting for this extraordinary release.
Featured in the video: Antonella Vallenari (INAF, Astronomical Observatory of Padua), Anthony Brown (Leiden University), Timo Prusti (European Space Agency), Annie Robin (Institut UTINAM, OSU THETA Franche-Comté-Bourgogne), Laurent Eyer (University of Geneva) and Federica Spoto (IMCCE, Observatory of Paris).
A media briefing on the second Gaia data release will be held at the ILA Berlin Air and Space Show in Germany on 25 April 11:00-12:15 CEST. Watch the webstream at www.esa.int/live
This evidence seems to suggest that the dark matter is particles that are less than four times the mass of a proton and are moving at non-relativistic speeds. This is consistent with dark matter particles being so-called WIMPs: https://en.wikipedia.org/wiki/Weakly_interacting_massive_particles.
NOVA has teamed up with Cook’s Illustrated to cook up a recipe for stars and black holes – a culinary “course” on how the most mysterious objects in the universe are created.
Scientific notes:
Stellar mass black holes vs. supermassive black holes
* Stellar mass black holes form from the collapse of massive stars at the ends of their lives, so they have roughly the same mass as a star. Supermassive black holes are physically identical to their smaller counterparts, except they are 10 thousand to a billion times the size of the sun. However, their formation is more of a mystery. They may form from the merging of smaller black holes. http://astronomy.swin.edu.au/cosmos/S/Supermassive+Black+Hole
Supermassive black holes at the center of galaxies
* Almost every large galaxy has a supermassive black hole at its center, but researchers are not yet sure (https://jila.colorado.edu/research/astrophysics/black-holes-galaxies) why that’s the case, how they originate, and what their role is in the creation and evolution of galaxies.
Why are stars different colors?
* The color of a star depends on its temperature (http://www.atnf.csiro.au/outreach/education/senior/astrophysics/photometry_colour.html). The hotter a star, the higher energy its light will be. Higher energy/temperature corresponds with the blue end of the visible spectrum and lower energy/temperature corresponds with the red end.
How does dark matter make stars spin faster?
* In the 1960s, astronomers Vera Rubin and Kent Ford noticed that stars at the edges of galaxies were moving just as fast as stars at the center, which surprised them: it appeared that the force of gravity causing stars to orbit the center of the galaxy was not weakening over distance. Their observation implied that something else, distributed throughout the galaxy, was exerting a gravitation pull. We now know that that “something else,” now named dark matter, accounts for about 85% of the matter in the universe. (It existence was inferred in the 1930s, when the astronomer Fritz Zwicky(http://www2.astro.psu.edu/users/rbc/a1/week_10.html) noticed that galaxies in clusters were moving faster than they should.)
Size of the universe
* The universe is only 13.8 billion years old, but has a radius of about 46 billion light-years. If nothing can travel faster than the speed of light, how can that be? The expansion of the universe, driven by dark energy, is causing distances between objects to grow. Note that it is not moving those objects apart; rather, it is increasing the amount of space between them. https://phys.org/news/2015-10-big-universe.html
Cosmic webs
* Galaxies are not distributed randomly (http://skyserver.sdss.org/dr1/en/astro/structures/structures.asp) in space; instead, clusters of galaxies form web-like patterns. These webs consist of filaments, where dark matter and ordinary (baryonic) matter are concentrated, and voids, where galaxies are scarce. Researchers believe that these large-scale structures grew out of minor fluctuations in density at the beginning of the universe.
Composition of the early universe
* Moments after the Big Bang, the universe formed the nuclei for what would be come the universe’s hydrogen and helium atoms, with one helium nucleus for every 10 or 11 hydrogen (http://umich.edu/~gs265/bigbang.htm). When the first stars formed, there were no heavier elements — those elements formed inside stars.
String Theory Landscape
* The String Theory Landscape is a theory that the universe we live in is one of many universes. It attempts to explain how certain constants of nature seem “fine-tuned” for life, which contradicts the anthropic principle, or the notion that we humans hold a special place in the universe. https://www.scientificamerican.com/article/multiverse-the-case-for-parallel-universe/%0A
Disintegration of the universe
* In the future Degenerate Era of the universe, as space-time expands and stars burn up, all of the matter in stars will be consumed by black holes. But even black holes are not forever. Stephen Hawking theorized that black holes will slowly radiate away their mass in what is now called Hawking radiation until they too dissipate away. http://www.nytimes.com/books/first/a/adams-universe.html
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MEDIA CREDITS:
Music provided by APM
Sound effects: Freesound.org
Additional Animations:
– Galaxy within Universe: Edgeworx;
– Stars at center of Milky Way – NASA/NCSA University of Illinois Visualization by Frank Summers, Space Telescope Science Institute, Simulation by Martin White and Lars Hernquist, Harvard University
This video reveals the evolution of stars in our Galaxy over the past million of years.
It starts from the positions of stars in the sky 1 035 000 years ago, which were calculated using data from the Tycho-Gaia Astrometric Solution, or TGAS, one of the products of the first Gaia data release. The video follows the evolution of stellar positions until the present day, ending with a view of the sky as measured by Gaia between 2014 and 2015.
Highlighted in yellow are the trajectories of six special stars: these are hypervelocity stars, moving through the Galaxy at several hundred of km/s. While it might not be apparent from the video, which shows the motions of stars as projected on the sky, they are moving through space much faster than the galactic average.
Scientists spotted these speeding stars from the TGAS data set of two million stars with the help of an artificial neural network – software that mimics a human brain – and they are looking forward to finding many more in future Gaia data releases.
These stars owe their high speeds to past interactions with the supermassive black hole that sits at the centre of the Milky Way and, with a mass of four million Suns, governs the orbits of stars in its vicinity. Having travelled great distances through the Galaxy, they provide crucial information about the gravitational field of the Milky Way from the centre to its outskirts.
One of the six stars (labelled 1 at the end of the video) seems to be speeding so fast, at over 500 km/s, that it is no longer bound by the gravity of the Galaxy and will eventually leave. The other five stars are somewhat slower (over 400 km/s for the stars labelled 2, 3, 4 and 6, and 360 km/s for the star labelled 5) and are still bound to the Galaxy.
These slightly slower stars are perhaps even more fascinating, as scientists are eager to learn what slowed them down – the invisible dark matter that is thought to pervade the Milky Way might also have played a role.
The stars are plotted in Galactic coordinates and using a rectangular projection: in this, the plane of the Milky Way stands out as the horizontal band with greater density of stars. The stripes visible in the final frames reflect the way Gaia scans the sky and the preliminary nature of the first data release; these artefacts are gradually washed out in the video as stars move across the sky.
