“This is a 360° animated view of the entire sky. 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. “
Credits Video: ESA/Gaia/DPAC, CC BY SA 3.0 IGO/Gaia Data Processing and Analysis Consortium (DPAC); Gaia Sky; S. Jordan/T. Sagristà , Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Germany
“Though close to home, the space immediately around Earth is full of hidden secrets and invisible processes. In a new discovery reported in the journal Nature, scientists working with NASA’s Magnetospheric Multiscale spacecraft — MMS — have uncovered a new type of magnetic event in our near-Earth environment by using an innovative technique to squeeze extra information out of the data.
Magnetic reconnection is one of the most important processes in the space — filled with charged particles known as plasma — around Earth. This fundamental process dissipates magnetic energy and propels charged particles, both of which contribute to a dynamic space weather system that scientists want to better understand, and even someday predict, as we do terrestrial weather. Reconnection occurs when crossed magnetic field lines snap, explosively flinging away nearby particles at high speeds. The new discovery found reconnection where it has never been seen before — in turbulent plasma. “
Credits Music: “Think Tank” and “Natural Time Cycles” by Laurent Dury from Killer Tracks
Credits Video: NASA’s Goddard Space Flight Center/Tai Phan (University of California, Berkeley): Lead Scientist/James Drake (University of Maryland): Scientist/Michael Shay (University of Delaware): Scientist/Jonathan Eastwood (Imperial College London): Scientist/Joy Ng (USRA): Producer/Mara Johnson-Groh (Wyle Information Systems): Writer/Tom Bridgman (GST): Data Visualizer/Lisa Poje (Freelance): Lead Animator/Josh Masters (USRA): Lead Animator/Walt Feimer (KBRwyle): Animator/Brian Monroe (USRA): Animator/Joy Ng (USRA): Animator/Mary P. Hrybyk-Keith (TRAX International Corporation): Graphic Designer/Colby Haggerty (University of Chicago): Visualizer/Ashley Michini (University of Pennsylvania): Visualizer/Tulasi Parashar (University of Delaware): Visualizer/Aaron E. Lepsch (ADNET Systems Inc.): Technical Support
“NASA’s remotely-piloted Ikhana aircraft, based at the agency’s Armstrong Flight Research Center in Edwards, California, successfully flew its first mission in the National Airspace System without a safety chase aircraft. This historic flight moves the United States one step closer to normalizing unmanned aircraft operations in the airspace used by commercial and private pilots.
Flying these large remotely-piloted aircraft over the United States opens the doors to all types of services, from monitoring and fighting forest fires, to providing new emergency search and rescue operations. The technology in this aircraft could, at some point, be scaled down for use in other general aviation aircraft.
Flights of large craft like Ikhana, have traditionally required a safety chase aircraft to follow the unmanned aircraft as it travels through the same airspace used by commercial aircraft. The Ikhana flew in accordance with the Federal Aviation Administration’s (FAA) Technical Standard Order 211 — Detect and Avoid Systems — and Technical Standard Order 212 — Air-to-Air Radar for Traffic Surveillance.
The FAA granted NASA special permission to conduct this flight under the authority of a Certificate of Waiver or Authorization on March 30. The certificate permitted Ikhana’s pilot to rely on the latest Detect and Avoid technology, enabling the remote pilot on the ground to see and avoid other aircraft during the flight.
NASA successfully worked with its industry partners to develop a standard for Detect and Avoid technologies, complied with the requirements of the FAA Technical Standard Orders, and garnered flight approval from the FAA.
The Ikhana aircraft was equipped with detect and avoid technologies, including an airborne radar developed by General Atomics Aeronautical Systems, Inc., a Honeywell Traffic Alert and Collision Avoidance System, a Detect and Avoid Fusion Tracker, and an Automatic Dependent Surveillance-Broadcast capability – a surveillance technology where the aircraft determines its position via satellite navigation and periodically broadcasts this information so other aircraft can track it.”
“These are the last images taken by Rosetta’s high resolution OSIRIS camera during the mission’s final hours at Comet 67P/Churyumov-Gerasimenko. As it moved closer towards the surface it scanned across an ancient pit and sent back images showing what would become its final resting place.”
Credits Video: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA – CC BY-SA 4.0/D. C. Jimeno and M. P. Ayucar
“The launch lasts less than ten minutes whereby the Soyuz spacecraft is propelled 1640 km and gains 210 km altitude. Every second for nine minutes, the spacecraft accelerates 50 km/h on average as the rocket’s boosters burn their fuel and are discarded.
The astronauts, from left to right, are NASA astronaut Serena Auñón-Chancellor, Roscosmos commander Sergei Prokopyev, and ESA astronaut and flight engineer Alexander Gerst launched in the Soyuz MS-09 spacecraft from the Baikonur cosmodrome in Kazakhstan to the International Space Station on 6 June 2018.
Hunched in their Sokol flight suits that offer protection in case of fire or depressurisation, the trio stay in the crew capsule of the Soyuz – the only module that is also designed to survive a return to Earth. The bags above their heads contain supplies for the International Space Station as every bit of space is used.
During a Soyuz launch astronauts typically experience forces of up to 4g – having to work while being pressed into their seats with a force that is four times more than the gravity felt on Earth. The Soyuz commander uses a stick to press buttons as they are too far away from the control panel.
The fluffy toys above the astronauts’ heads are mascots and good luck charms but also serve as a simple but effective test to see when the spacecraft is in orbit: when they start to float the spacecraft is weightless and orbiting Earth. Above Sergei is the mascot for the 2018 FIFA soccer World Cup held in Russia. Alexander took German children television icon “Die Maus” with him.
The launch went as planned as the 50-m tall Soyuz rocket propelled the astronauts to their cruising speed of around 28 800 km/h. For this launch the astronauts took 34 orbits of Earth over two days to arrive at their destination spending their time in the cramped orbital module of the Soyuz that is no larger than a car. With limited communications and living space the astronauts had time to adapt to weightlessness and reflect on their mission ahead. They aligned their spacecraft with the International Space Station and approached the orbital outpost for docking on 8 June 2018.
Alexander is a returning visitor to the International Space Station, the first of ESA’s 2009 class of astronauts to be sent into space for a second time. During the second part of his mission Alexander will take over as commander of the International Space Station, only the second time an ESA astronaut will take on this role so far.”
“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.”
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