[Wikipedia] Toulouse Observatory
The Toulouse Observatory (French: Observatoire de Toulouse) is located in Toulouse, France and was established in 1733.
It was founded by l'Académie des Sciences, Inscriptions et Belles-Lettres de Toulouse (Academy of Science, Inscriptions and the Humanities of Toulouse). It was moved 1841 and again in 1981.
In 1987, Genevieve Soucail of the Toulouse Observatory and her collaborators presented data of a blue ring-like structure in Abell 370 and proposed a gravitational lensing interpretation
In the 1990s the observatory worked on MEGACAM with several other institutions.
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Ariane 5, Cité de l'espace, Toulouse, Midi-Pyrénées, France, Europe
Ariane 5 is a European rocket that is a part of the Ariane rocket family, an expendable launch system used to deliver payloads into geostationary transfer orbit (GTO) or low Earth orbit (LEO). Ariane 5 rockets are manufactured under the authority of the European Space Agency (ESA) and the Centre National d'Etudes Spatiales (CNES). Airbus Defence and Space is the prime contractor for the vehicles, leading a consortium of sub-contractors. Ariane 5 is operated and marketed by Arianespace as part of the Ariane programme. Astrium builds the rockets in Europe and Arianespace launches them from the Guiana Space Centre in French Guiana. Ariane 5 succeeded Ariane 4, but was not derived from it directly. Ariane 5 has been refined since the first launch in successive versions, G, G+, GS, ECA, and most recently, ES. ESA originally designed Ariane 5 to launch the Hermes spaceplane, and thus intended it to be human rated from the beginning. Two satellites can be mounted using a SYLDA carrier (SYstème de Lancement Double Ariane). Three main satellites are possible depending on size using SPELTRA (Structure Porteuse Externe Lancement TRiple Ariane). Up to eight secondary payloads, usually small experiment packages or minisatellites, can be carried with an ASAP (Ariane Structure for Auxiliary Payloads) platform. By mid-2007, Arianespace has ordered a total of 99 Ariane 5 launchers from Astrium. The first batch ordered in 1995 consisted of 14 launchers, while the second—P2—batch ordered in 1999 consisted of 20 launchers. A third—PA—batch consisting of 25 ECA and 5 ES launchers was ordered in 2004. The latest batch ordered in mid-2007 consist of another 35 ECA launchers. Through these orders, the Ariane 5 will be the workhorse of Arianespace at least through 2015. Ariane 5's first test flight (Ariane 5 Flight 501) on 4 June 1996 failed, with the rocket self-destructing 37 seconds after launch because of a malfunction in the control software. A data conversion from 64-bit floating point value to 16-bit signed integer value to be stored in a variable representing horizontal bias caused a processor trap (operand error) because the floating point value was too large to be represented by a 16-bit signed integer. The software was originally written for the Ariane 4 where efficiency considerations (the computer running the software had an 80% maximum workload requirement) led to four variables being protected with a handler while three others, including the horizontal bias variable, were left unprotected because it was thought that they were physically limited or that there was a large margin of error. The software, written in Ada, was included in the Ariane 5 through the reuse of an entire Ariane 4 subsystem despite the fact that the particular software containing the bug, which was just a part of the subsystem, was not required by the Ariane 5 because it has a different preparation sequence than the Ariane 4. The second test flight (L502, on 30 October 1997) was a partial failure. The Vulcain nozzle caused a roll problem, leading to premature shutdown of the core stage. The upper stage operated successfully, but it could not reach the intended orbit.
A subsequent test flight (L503, on 21 October 1998) proved successful and the first commercial launch (L504) occurred on 10 December 1999 with the launch of the XMM-Newton X-ray observatory satellite. Another partial failure occurred on 12 July 2001, with the delivery of two satellites into an incorrect orbit, at only half the height of the intended GTO. The ESA Artemis telecommunications satellite was able to reach its intended orbit on 31 January 2003, through the use of its experimental ion propulsion system. The next launch did not occur until 1 March 2002, when the Envisat environmental satellite successfully reached an orbit 800 km above the Earth in the 11th launch. At 8111 kg, it was the heaviest single payload until the launch of the first ATV on March 9, 2008 (19,360 kg). The first launch of the ECA variant on 11 December 2002 ended in failure when a main booster problem caused the rocket to veer off-course, forcing its self-destruction three minutes into the flight. Its payload of two communications satellites (Stentor and Hot Bird 7), valued at about EUR 630 million, was lost in the ocean. The fault was determined to have been caused by a leak in coolant pipes allowing the nozzle to overheat. After this failure, Arianespace SA delayed the expected January 2003 launch for the Rosetta mission to 26 February 2004, but this was again delayed to early March 2004 due to a minor fault in the foam that protects the cryogenic tanks on the Ariane 5. As of April 2014, the failure of the first ECA launch was the last failure of an Ariane 5; since then, all subsequent launches have been successful, with 59 consecutive successes that stretch back to 9 April 2003 with the launch of INSAT-3A and Galaxy 12 satellites.
Toulouse (France) : Itinéraire de visite touristique par vue aérienne de la ville en 3D
aircitytour.com, l'itinéraire de vos visites touristiques et culturelles en vidéo en 3D (visite virtuelle). D'autres visites sont disponibles sur aircitytour.com
Visite virtuelle de la ville de Toulouse (France), par vue aérienne en 3D, à partir du logiciel Google Earth.
Détail de la visite par lieux :
- Cité de l'espace
- Musée Georges-Labit
- Jardin des Plantes
- Grand Rond
- Jardin Royal
- Quai des Savoirs
- Muséum de Toulouse
- Les Bateaux Toulousains
- Cathédrale Saint-Étienne de Toulouse
- Musée Paul-Dupuy
- Hôtel du Vieux-Raisin
- Église Notre-Dame de la Dalbade
- Prairie des Filtres
- Musée de l’Affiche de Toulouse
- Jardin Raymond VI
- Les Abattoirs
- Le Château d'eau
- Hôtel-Dieu Saint-Jacques
- Pont-Neuf de Toulouse
- Pont Saint-Pierre de Toulouse
- The Daurade
- Basilique de la Daurade
- Hôtel d'Assézat
- Musée des Augustins de Toulouse
- La Ruche
- Musée des Compagnons du Tour de France
- Musée du Vieux Toulouse
- Hôtel de Bernuy
- Ensemble conventuel des Jacobins
- Église Saint-Pierre des Chartreux de Toulouse
- Place du Capitole
- Capitole de Toulouse
- Square Charles-de-Gaulle
- Donjon du Capitole
- Église Notre-Dame du Taur
- Chapelle des Carmélites de Toulouse
- Musée Saint-Raymond, Musée des Antiques de Toulouse
- Basilique Saint-Sernin de Toulouse
- Observatoire de Toulouse
- Jardin Compans-Caffarelli
- Amphithéâtre romain de Purpan-Ancely
- Ailes Anciennes Toulouse
- Aeroscopia
Police tells Police Practice Observatory to leave, GiletsJaunes YV Toulouse, 11/01/20, live3 cut 13
Police in Toulouse know the French police observers. They have their own vests, allways, not as protesters, and they make scientific reports. These are now also send away by the police. Democracy in France...
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aeroscopia museum Toulouse, France
프랑스 남부 툴루즈에 위치한 에어로스코피아(aerocopia) 입니다.
에어로스코피아는 2015년 1월에 개장한 프랑스 항공 박물관 입니다.
프랑스가 에어버스와 관련이 있어서 에어버스와 관련된 비행기들 및 자료가 전시되고 있습니다.
aeroscopia museum Toulouse, France
XMM-Newton, Cité de l'espace, Toulouse, Midi-Pyrénées, France, Europe
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 114,000 kilometres (71,000 mi) from Earth, while the perigee is only 7,000 kilometres (4,300 mi). 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 Feb 2000. The original mission lifetime was two years, but it has now been extended for further observations until at least 2010, and again until 2012, and technically the observatory could operate until beyond 2018. Observations are managed and archived at the European Space Astronomy Centre (formerly known as VILSPA) 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. The European satellite XMM-Newton, built under contract to ESA by a consortium of 35 European companies with Astrium as prime contractor, by far excels its predecessor, the Astrium-built ROSAT satellite. The satellite weighs 3,800 kilograms (8,400 lb), is 10 metres (33 ft) long and 16 metres (52 ft) in span with its solar arrays deployed. It holds three X-ray telescopes, developed by Media Lario of Italy, each of which contains 58 Wolter-type concentric mirrors. The combined collecting area is 4,425 cm2 (686 sq in) at 1.5 KeV to 1,740 cm2 (270 sq in) at 8 KeV. The three European Photon Imaging Cameras (EPIC) are sensitive over the energy range 0.2 keV to 12 keV. Other instruments onboard are two reflection grating spectrometers which are sensitive below ~2 keV, and a 30 centimetres (12 in) diameter Ritchey-Chretien optical/UV telescope. Each telescope consists of 58 600 mm-long shells, with diameters from 306 to 700 millimetres, and thickness linearly dependent on the diameter increasing from 470 µm at the small shells to 1070 µm at the large one; the fully assembled telescope has gaps of about one millimetre between the shells. The shells are made by electroforming onto a highly polished aluminium mandrel, starting with a 250 nm layer of vapour-deposited gold that becomes the reflecting surface, then the nickel support; the mandrels are reusable but a different one is needed for each shell. The electroforming deposits nickel at a rate of 10 µm per hour. The mandrels were manufactured at Carl Zeiss AG, and the electroforming and final assembly performed at Media Lario; Kayser-Threde also played a role. The shells are glued into grooves in an Inconel spider, which keeps them aligned to within the five-micron tolerance required to get adequate X-ray resolution. It was used to discover the 10 billion light years from Earth galaxy cluster XMMXCS 2215-1738. The object SCP 06F6, discovered by the Hubble Space Telescope (HST) in February 2006, was then observed by XMM Newton in early August 2006, and appeared to show an X-ray glow around it two orders of magnitude more luminous than that of supernovae. In June 2011, a team from the University of Geneva, Switzerland, reported XMM-Newton seeing a flare that lasted four hours at a peak intensity of 10,000 times the normal rate, from an observation of Supergiant Fast X-Ray Transient IGR J18410-0535, where a blue supergiant star shed a plume of matter that was partly ingested by the smaller neutron star with the accompanying X-ray emissions. In February 2014, different analyses have extracted from the spectrum of X-ray emissions observed by XMM-Newton, a monochromatic signal around 3.5 keV. This signal is coming from different galaxy cluster and several scenarios of dark matter can justify such a line. We can cite for example a 3.5 keV candidate annihilating into 2 photons, or a 7 keV dark matter particle decaying into photon and neutrino. In any case, it would be a warm dark matter which could be motivated also by other astrophysical observations (core galactic profiles and missing of small structures around the milky way).
Le planétarium
Le planétarium de l'Espace des sciences, à Rennes. Chaque séance est pilotée en direct et commentée par un médiateur, qui adapte son discours au thème, au public et à l'actualité astronomique. Un voyage fantastique, aux confins de l'Univers, entre l'infiniment grand et l'infiniment petit ! Réalisation Vincent Melcion.
Police Practice Observatory is send away Gilets Jaunes protest Toulouse live cut7, 2-11-2019, acte51
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This work can be used, but not abused – if you feel the need to steal it, at least have the decency to put up links to our youtube channel
and facebook page
(Not because I want to get rich from this, but because I need to live and we want to keep the information free for people, we all work for free and because I take the fucking risks in the street to provide this information for free, for the people)
And since I am actually really poor because of doing this, you can support me and keep me going. If I do get rich from this, I will share it with the other workers, but far from that, hahahahaha.
If you like my work, please leave a tip so I can continue
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Juut Muijs gas sprayed from CLOSE up with can Medics help her Act 48 , Toulouse, France 12102019
Yellow Vests protest , Act 48, today is the national call in Toulouse
Juut get sprayd from upclose, medics needed, could not open eyes for a while.
Today still hurts, but non the less she went on filming.
Please Subscribe! and ask others, when we have 1000+ subscribers we can do more technically, plus people do not hAve to get a notification, simply do not tap or click the bell icon Thanks in advance!
Reporting in English – Dutch and German possible too!
Subscribe to our youtube channel while you are at it. Click the bell. And you will be notified every time we go live.
This work can be used, but not abused – if you feel the need to steal it, at least have the decency to put up links to our youtube channel
and facebook page
(Not because I want to get rich from this, but because I need to live and we want to keep the information free for people, we all work for free and because I take the fucking risks in the street to provide this information for free, for the people)
And since I am actually really poor because of doing this, you can support me and keep me going. If I do get rich from this, I will share it with the other workers, but far from that, hahahahaha.
If you like my work, please leave a tip so I can continue
PayPal: info@unusuals.eu
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@juutmuijs
2018 IPS Toulouse
메타스페이스
We miss IPS Toulouse 2018 already. See you guys again 2020.
2018 IPS Conference에 다녀왔습니다! ^0^~/
(IPS, International Planetarium Society)
ECLA 2016 - Olivier Berné, Université de Toulouse/CNRS (France)
Interview with Olivier Berné, from the Université de Toulouse/CNRS (France).
European Conference on Laboratory Astrophysics ECLA2016: Gas on the Rocks, November 21 - 25, 2016, CSIC, Madrid, Spain
More information in the #ECLA2016 Press Room:
Suicidal Tendencies - Live in Toulouse 2017
Suicidal Tendencies - Live in Toulouse 2017
MOPA Interview (Toulouse - 12.08.2010) pt.3
Interview de Tristan Mocquet (piano) à la Halle aux Grains de Toulouse le 12 Août 2010. Troisième partie.
DaveyDanceBlog -139- Toulouse
Davey Dance-BLOG. A project started while traveling Europe during Spring 2007. Armed only with an ipod and a Canon, Davey picks a location and a pop song. Then Davey records an improvised dance.
Featuring the song La Vie en Rose by Louis Armstorng
(dedicated to my friend Camille Billops for suggesting to slow it down a bit, and to the PS on their recent political victory. ROSE! )
Rosangela e Rosane na igreja de Toulouse
Rosangela e Rosane na igreja de Toulouse
Marche de nuit féministe à Toulouse - 25 novembre 2017
Le 25 novembre 2017 une marche de nuit en mixité choisie contre les violences sexistes défilait bruyamment dans les rues de Toulouse. Nous étions nombreu.ses à occuper l'espace public plusieurs heures durant, avec une batucada splendide et des slogans déters, tels que «Nous sommes fortes, nous sommes fières, et féministes et radicales et en colère ! », « Ta main sur mon cul, mon poing dans ta gueule ! », « Contre le patriarcat je me lève et je me bat ! Contre les violences sexistes, je résiste et je persiste ! », « Fière, vénère, pas prête à s'taire ! , etc.
L'ambiance était puissante et énergisante, une marche magnifique, marquée notamment par une chorale (et d'autres un peu plus improvisées ^^) qui, pour ma part, m'a fait découvrir de superbes chansons féministes.
Malheureusement, des policiers de la bac (majoritairement) ainsi que des crs nous ont suivis de très près durant tout le long du parcours. Dès le début ce fut tendu, ils avaient clairement envie d'arrêter des personnes, pointant des gens du doigt et animés par une attitude clairement agressive.
Des tags ainsi que des stickers ont été apposés à différents endroits afin de délivrer des messages politiques. Après l'un d'entre eux, les crs et la bac ont tenté d'interpeller une personne de façon violente (coups de matraques et gazages à bout portant), une solidarité était très clairement présente, protégeant les personnes en danger. Mais malgré cela 2 personnes ont été arrêtées et placées en garde à vue cette nuit là.
(Arrêter des personnes qui manifestent contre les violences sexistes mais laisser en liberté des agresseurs/violeurs dont on sait qu'ils sont dangereux ?)
Arrivé.es à la fin du parcours autorisé, à Jean Jaures, le cortège à continué toujours dans la même lancée dans le grand boulevard (l'accès à Jean Jaures même était impossible au vu du nombre de camion de crs garés pour faire barrage). Les crs et la bac ont rapidement tout fait pour que nous quittions le boulevard, tentant tout d'abord d'arracher une banderole, puis en tirant une grenade lacrymogène dans la foule. Malgré cela la marche a continué dans ce lieu très passant, au milieu des bars remplis de monde, et toujours avec des slogans pleins d'entrain (la batucada était quant à elle partie).
Mais très peu de temps après, les crs et bacceux sont venus bloquer le boulevard notamment en tirant de nouveau une grenade lacrymo dans la foule. Le cortège se dirige alors naturellement vers un axe moins passant, continuant à se faire entendre. Pour faire rapide, la marche s'est terminée par une dispersion choisie à un moment donné critique.
Malgré tout, une très belle marche, une énergie géniale.
A bas le patriarcat, à bas les violences sexistes, de grosses pensées et un gros soutien à tou.tes les survivant.es de violences sexistes en tout genre.
En espérant que cette vidéo puisse un peu vous relater ce moment fort.
Toulouse Acte 39 : les Gilets jaunes descendent dans la rue
Le 10 août c'est jaune à Toulouse ! En plein été les jaunes sont toujours là pour la justice sociale fiscale et climatique !
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#GiletsJaunes #Toulouse #Acte39
Toulouse gunfire
Walking into town we happen upon the action
Devendra - i feel like a child - Toulouse