XMM-NEWTON SPACE TELESCOPE

Welcome to my channel! I'm Dr Maggie Lieu and I make youtube videos about space & astronomy. Today, December 10th 2019, XMM-Newton has turned 20 years old, that's a long time for a spacecraft with an expected lifetime of just 10 years! In this week's video, I'm at ESA's European Space Astronomy Centre, in the XMM operations room talking to XMM's Project Scientist, Norbert Schartel (https://www.cosmos.esa.int/web/personal-profiles/norbert-schartel) and XMM's Science Operations Manager, Maria Santos-Lleo (https://www.cosmos.esa.int/web/personal-profiles/maria-santos-lleo) on the legacy of XMM-Newton. Extra reading: XMM overview: https://www.esa.int/Science_Exploration/Space_Science/XMM-Newton_overview XMM science page: https://sci.esa.int/web/xmm-newton/home XMM 20th anniversary page: https://xmm-tools.cosmos.esa.int/external/xmm_news/20th_Anniversary/ Media credits: All XMM: ESA Chandra: NASA/CXC/SAO & J. Vaughan Perseus cluster: Zuhone/Harvard exoplanets: ESA/Hubble/Kornmesser/Christensen Expanding universe: Kornemesser/Calcada/ESA/NASA Neutrinos: NSFC Gliese667: ESO/Calcada erosita: Pietschner,MPE erosita all sky: FAU/DAUSER

Welcome to my channel! I'm Dr Maggie Lieu and I make youtube videos about space & astronomy. On December 10th, XMM-Newton will be turning 20 years old, that's a long time for a spacecraft with an expected lifetime of just 10 years! In this week's video, I'll be talking about what makes XMM so impressive. Extra reading: XMM, Jansen et al 2001: https://www.aanda.org/articles/aa/pdf/2001/01/aaxmm39.pdf XMM overview: https://www.esa.int/Science_Exploration/Space_Science/XMM-Newton_overview XMM science page: https://sci.esa.int/web/xmm-newton/home 4 wheel drive update: https://arc.aiaa.org/doi/abs/10.2514/6.2014-1904 Fuel migration: https://www.esa.int/Enabling_Support/Operations/Teaching_an_old_satellite_new_tricks https://indico.ict.inaf.it/event/720/contributions/5585/attachments/2872/5600/19_Bologna_XMM.pdf Media credits: Lagoon nebula backdrop: ESA/Hubble/NASA/ESO/STSCI/DSS various(Exosat, Exosat launch, XMM): ESA quasar pds456 spectra: NASA/JPL-Caltech/Keele Univ. pointing accuracy: MSSL reaction wheels: Matra Marconi Space, UK XMM launch: esa fuel tanks weissman: et al 2016 Athena: esa If you enjoyed the video, please help me by liking, sharing and subscribing! I'm also on: twitter: https://twitter.com/space_mog instagram: https://instagram.com/space_mog/ facebook: https://facebook.com/spacemog/

A study using NASA's Chandra X-ray Observatory, ESA's XMM-Newton and the Sloan Digital Sky Survey tracked dark engergy back to one billion years after the Big Bang. -- Learn more about it: http://chandra.cfa.harvard.edu/photo/2019/dark/ Credit: NASA/CXC/A. Hobart

XMM-Newton and Chandra combined analysis of the most massive galaxy clusters at z~1 Talk by Dr. Iacopo Bartalucci (CEA, Université Paris-Saclay) Given at the Instituto de Astrofísica de Canarias on May 10th, 2018 10:30 AM We present a detailed study of the spatially resolved thermodynamic and hydrostatic mass profiles of the five most massive clusters detected at z~1 via the Sunyaev-Zel'dovich effect. These objects represent an ideal laboratory to test our models in a mass regime where structure formation is driven mainly by gravity. We present a method to study these objects that optimally exploits information from XMM-Newton and Chandra observations. The combination of Chandra’s excellent spatial resolution and XMM-Newton’s photon collecting power allows us to spatially resolve the profiles from the core to the outskirts, for the first time in such objects.  Evolution properties are investigated by comparison with the REXCESS  local galaxy cluster sample. Finally, we discuss the current limitations of this method in the context of  joint analysis of future Chandra and XMM large programs and, more generally, of  multi-wavelength efforts to study high redshift objects. http://iactalks.iac.es/talks/view/1147 More talks at IACTalks: http://iactalks.iac.es

ESA's XMM-Newton has spotted surprising changes in the powerful streams of gas from two massive stars in the binary star system HD 5980. One of the two stars had a major outburst reminiscent of the 19th-century eruption of Eta Carinae, and astronomers expected that its X-ray emission would fade gently over the years. Instead, they found the pair was two and a half times brighter than a decade earlier, and its X-ray emission was even more energetic, suggesting that colliding stellar winds don’t behave as expected. Full story: Stellar winds behaving unexpectedly - http://www.esa.int/Our_Activities/Space_Science/Stellar_winds_behaving_unexpectedly Music: David Hilowitz – CC BY-NC 4.0

Artist's impression of the XMM-Newton spacecraft. The animation shows how the light is collected by XMM-Newton's three telescopes through their entrance baffles. Within each telescope, the X-ray photons then pass a set of barrel-shaped coaxial mirrors (only a few of the actual 58 concentric mirrors are depicted). After grazing the gold-plated mirrors, the now focused X-ray photons are collected at the other end of the 10-meter-long spacecraft where the detectors of the EPIC [1] and RGS [2] instruments are located. The animation ends with a close-up of a telescope entrance baffle. [1] At the prime focus of each of the spacecraft's three telescopes, behind a six-position filter wheel, is a European Photon Imaging Camera (EPIC). With silicon chips that can register extremely weak X-ray radiation, these advanced Charge-Coupled Device cameras (CCD) are capable of detecting rapid variations in intensity, down to a thousandth of a second and less! [2] For a complementary analysis of the spectrum, two of the three telescopes have a grating structure on their mirror module that reflects about 40 per cent of the incoming rays to a secondary focus, with its own CCD camera. This Reflection Grating Spectrometer (RGS) "fans out" the various wavelengths, thus indicating, in more detail than EPIC, the exact condition of individual elements, such as oxygen and iron. Credit: ESA

This video shows how to interactively analyze XMM-Newton data from the XMM-Newton Science Archive (XSA). XMM-Newton Science Archive: http://nxsa.esac.esa.int/ XMM-Newton Science Operations Centre: https://www.cosmos.esa.int/web/xmm-newton XMM-Newton Helpdesk: http://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk ESAC Science Data Centre: http://archives.esac.esa.int

Imagery of nebula from the Very Large Array, the Spitzer Space Telescope, the Hubble Space Telescope, the XMM-Newton Observatory, and the Chandra X-ray are showcased. The supernova remnant is 6,500 light-years from Earth. Credit: NASA, ESA, and J. DePasquale (STScI)

The "XMM-Newton", also known as the "X-ray Multi-Mirror Mission" and the "High Throughput X-ray Spectroscopy Mission", is an orbiting X-ray observatory launched by ESA in December 1999 on an Ariane 5 rocket. It is named in honor of Sir Isaac Newton. The telescope was placed in a very eccentric 48 hour elliptical orbit at 40°; at its apogee it is nearly 114000 kilometers from Earth, while the perigee is only 7000 kilometers. The observational scope of XMM-Newton includes the detection of X-ray emissions from Solar System objects, detailed studies of star-forming regions, investigation of the formation and evolution of galaxy clusters, the environment of supermassive black holes and the mapping of the mysterious dark matter. The mission was proposed in 1984 and approved in 1985; a project team was formed in 1993 and development work began in 1996. The satellite was constructed and tested from March 1997 to September 1999. Launched in Dec 1999, in-orbit commissioning started Jan 2000, and the first images were published in February 2000. The original mission lifetime was two years, but it was extended for further observations. Its most recent extension was to 31 December 2016. Technically, the observatory could operate until beyond 2018. Observations are managed and archived at the European Space Astronomy Centre at Villafranca, Spain. Until March 2012 the scientific data placed into the archive and distributed to observers were processed by the XMM-Newton Survey Science Centre led by the University of Leicester, England. After this date, responsibility for data processing transferred to the Science Operations Centre at ESAC. Wiz Science™ is "the" learning channel for children and all ages. SUBSCRIBE TODAY Disclaimer: This video is for your information only. The author or publisher does not guarantee the accuracy of the content presented in this video. USE AT YOUR OWN RISK. Background Music: "The Place Inside" by Silent Partner (royalty-free) from YouTube Audio Library. This video uses material/images from https://en.wikipedia.org/wiki/XMM-Newton, which is released under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . This video is licensed under Creative Commons Attribution-Share-Alike License 3.0 http://creativecommons.org/licenses/by-sa/3.0/ . To reuse/adapt the content in your own work, you must comply with the license terms.

NASA's Nuclear Spectroscopic Telescope Array (NuSTAR) and ESA’s (European Space Agency) XMM-Newton telescope are showing that fierce winds from a supermassive black hole blow outward in all directions -- a phenomenon that had been suspected, but difficult to prove until now. http://proxyponder.com/2015/02/supermassive-black-hole-wind-theory-proven-by-nasa-and-esa/ Source: http://www.nasa.gov/press/2015/february/nasa-esa-telescopes-give-shape-to-furious-black-hole-winds/index.html#.VOa81fnF8uk Find Me & Follow Me: https://twitter.com/ShantiUniverse https://www.facebook.com/pages/Shanti-Universe/1405680779677488 http://shantiuniversenewsnow.blogspot.com/ https://plus.google.com/u/0/b/108273886503213598014/108273886503213598014/posts Check Out my NEW Website: http://proxyponder.com ~*Get the ShantiUniverse App! For Android & iphone: http://fanapp.mobi/shantiuniverseapp

The mysterious signal was detected by NASA's X-Ray Observatory and ESA's XMM-Newton in the Perseus galaxy cluster and 73 others. Scientists think that this may be the work of a hypothetical particle called a sterile neutrino.

This video provides an introduction to interacting with the XMM-Newton Science Archive results produced from a basic search. For more help and information on using the archive, visit: http://archives.esac.esa.int/xsa/#help

This video provides an introduction to the main search interface of the XMM-Newton Science Archive, used to perform a basic search. For more help or information on using the archive visit: http://archives.esac.esa.int/xsa/#help

Launch of XMM-Newton aboard Ariane 504, December 10 1999.

In this fifth episode of the [email protected] vodcast series Rebecca Barnes will give us a glimpse of the hot, energetic and often violent Universe revealed through X-ray and gamma-ray astronomy, look at ESA missions that detect this hidden light and find out how the science that these missions perform is meticulously planned.

Two of ESA's space observatories, XMM-Newton and Herschel, have combined to create a multi-wavelength view of violent events taking place within the giant galaxy of Centaurus A. The new observations strengthen the view that it may have been created by the cataclysmic collision of two older galaxies. New images taken with the Herschel space observatory with unprecedented resolution at far-infrared wavelengths show that the giant black scar of obscuring dust crossing the centre of Centaurus A all but disappears. ESA's XMM-Newton X-ray observatory recorded the high-energy glow from one of the jets, extending over 12 000 light years away from the galaxy's bright nucleus. XMM-Newton's X-ray view shows not only the way that the jet interacts with the surrounding interstellar matter, but also the galaxy's intensely active nucleus, and its large gaseous halo.

The central region of our Milky Way, the Galactic Bulge, is a rich host of variable high-energy X-ray and gamma-ray sources. Thanks to regular observations by XMM-Newton and Integral observatories over the last ten years, this dynamic environment has been charted in extensive detail, as revealed in this video.

The Eagle Nebula as never seen before. In 1995, the Hubble Space Telescope's 'Pillars of Creation' image of the Eagle Nebula became one of the most iconic images of the 20th century. Now, two of ESA's orbiting observatories, XMM-Newton and Herschel satellites, have shed new light on this enigmatic star-forming region. The ESA Herschel Space Observatory's new image shows the pillars and the wide field of gas and dust around them. Captured in far-infrared wavelengths, the image allows astronomers to see inside the pillars and structures in the region. In parallel, a new multi-energy X-ray image from ESA's XMM-Newton telescope shows those hot young stars responsible for carving the pillars.

ESA's fleet of space telescopes has captured the nearby Andromeda Galaxy, also known as M31, in different wavelengths. Most of these wavelengths are invisible to the eye and each shows a different aspect of the galaxy's nature. Visible light, as seen by optical ground-based telescopes and our eyes, reveals the various stars that shine in the Andromeda Galaxy, yet it is just one small part of the full spectrum of electromagnetic radiation. There are many different wavelengths that are invisible to us but which are revealed by ESA's orbiting telescopes. Starting at the long wavelength end, the Planck spacecraft collects microwaves. These show up particles of incredibly cold dust, at just a few tens of degrees above absolute zero. Slightly higher temperature dust is revealed by the shorter, infrared wavelengths observed by the Herschel space telescope. This dust traces locations in the spiral arms of the Andromeda Galaxy where new stars are being born today. The XMM-Newton telescope detects wavelengths shorter than visible light, collecting ultraviolet and X-rays. These show older stars, many nearing the end of their lives and others that have already exploded, sending shockwaves rolling through space. By monitoring the core of Andromeda since 2002, XMM-Newton has revealed many variable stars, some of which have undergone large stellar detonations known as novae. Ultraviolet wavelengths also display the light from extremely massive stars. These are young stars that will not live long. They exhaust their nuclear fuel and explode as supernovae typically within a few tens of millions of years after they are born. The ultraviolet light is usually absorbed by dust and re-emitted as infrared, so the areas where ultraviolet light is seen directly correspond to relatively clear, dust-free parts of Andromeda. By putting all of these observations together, and seeing Andromeda in its many different colours, astronomers are able to follow the life cycle of the stars.