OrbitalHub

NASA dixit:

“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.”

Credits Video: NASA

ESA dixit:

“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

ESA dixit:

“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.”

Credits Video: ESA/NASA/Roscosmos

ESA dixit:

“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.”

Credits Video:ESA

ESA dixit:

“This is an animated view of the 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. “

Credits Video: ESA / Gaia / DPAC / 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

NASA dixit:

“On June 11, NASA’s Fermi Gamma-ray Space Telescope celebrated a decade of using gamma rays, the highest-energy form of light in the cosmos, to study black holes, neutron stars, and other extreme cosmic objects and events. Fermi’s main instrument, the Large Area Telescope (LAT), has observed more than 5,000 individual gamma-ray sources.

In 1949, Enrico Fermi — an Italian-American pioneer in high-energy physics and Nobel laureate for whom the mission was named — suggested that cosmic rays, particles traveling at nearly the speed of light, could be propelled by supernova shock waves. In 2013, Fermi’s LAT used gamma rays to prove these stellar remnants are at least one source of the speedy particles. Fermi’s all-sky map, produced by the LAT, has revealed two massive structures extending above and below the plane of the Milky Way. These two “bubbles” span 50,000 light-years and were probably produced by the supermassive black hole at the center of the galaxy only a few million years ago.

The Gamma-ray Burst Monitor (GBM), Fermi’s secondary instrument, can see the entire sky at any instant, except the portion blocked by Earth. The satellite has observed over 2,300 gamma-ray bursts, the most luminous events in the universe. Gamma-ray bursts occur when massive stars collapse or neutron stars or black holes merge and drive jets of particles at nearly the speed of light. In those jets, matter travels at different speeds and collides, emitting gamma rays.

On August 17, 2017, Fermi detected a gamma-ray burst from a powerful explosion in the constellation Hydra. At almost the same time, the National Science Foundation’s Laser Interferometer Gravitational-wave Observatory detected ripples in space-time from the same event, the merger of two neutron stars. This was the first time light and gravitational waves were detected from the same source. Scientists also used another gamma-ray burst detected by Fermi to confirm Einstein’s theory that space-time is smooth and continuous. “

Credits Music: “Unseen Husband” from Killer Tracks

Credits Video: NASA’s Goddard Space Flight Center