“The Arkyd-6 spacecraft not only tests our core technologies, but also tests how we work together as a team. In this video, our Director of Systems Engineering Brian Douglas describes the design and engineering philosophies that worked really well for us when building Arkyd-6.
Using components that were not originally designed for space, innovating where it makes sense, and having a single owner from a hardware’s inception to its operation are some philosophies that we will continue to build upon as we design the Arkyd-301 spacecraft. ​”
“The mission of the Bigelow Expandable Activity Module (BEAM) on the International Space Station has been, well, expanded. After more than a year and a half on orbit providing performance data on expandable habitat technologies, NASA and Bigelow Aerospace have reached agreement to extend the life of the privately-owned module. For a minimum of three more years, BEAM will be a more operational element of the station used in crew activities and on board storage, allowing time to gather more data on the technology’s structural integrity, thermal stability, and resistance to space debris, radiation and microbial growth.”
“Built in compliance with the 6U CubeSat standard, the Arkyd-6 (A6) includes the core technology that will be used in the company’s asteroid exploration program including a mid-wave infrared sensor, second-generation avionics, power systems, communications, and attitude determination and control systems.
The A6 instrument is a broadband imager spanning 3 to 5 microns within the infrared region of the electromagnetic spectrum. This region is sensitive to the presence of water – including that in hydrated minerals – and thermal energy, allowing it to be used as a tool to search for water on Earth and beyond. In support of our deep space exploration efforts, A6 is a part of Planetary Resources’ research and development work to create an instrument capable of detecting water on near-Earth asteroids.”
“A team from NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is developing a new, third-generation facility science instrument for the Stratospheric Observatory for Infrared Astronomy, SOFIA.
The High Resolution Mid-InfrarEd Spectrometer (HIRMES), is a spectrometer optimized to detect neutral atomic oxygen, water, as well as normal and deuterated (or “heavy”) hydrogen molecules at infrared wavelengths between 25 and 122 microns (a micron is one-millionth of a meter). These wavelengths are key to determining how water vapor, ice, and oxygen combine at different times during planet formation, and will enable new observations of how these elements combine with dust to form the mass that may one day become a planet.
HIRMES will provide scientists with a unique opportunity to study this aspect of planetary formation, as SOFIA is currently the only NASA observatory capable of accessing these mid-infrared wavelengths. Infrared wavelengths between 28 and 112 microns do not reach ground-based telescopes because water vapor and carbon dioxide in the Earth’s atmosphere block this energy. SOFIA is able to access this part of the electromagnetic spectrum by flying between 39,000 feet and 45,000 feet, above more than 99 percent of this water vapor.”
Francis Reddy (Syneren Technologies): Science Writer
Rob Andreoli (AIMM): Videographer
John Caldwell (AIMM): Videographer
Scott Wiessinger (USRA): Animator
Music credit: “Sparkle Shimmer” and “The Orion Arm”, both from Killer Tracks.
“Though the Webb telescope will focus on stars and galaxies approximately 13.5 billion light-years away, its sight goes through a similar process as you would if you underwent laser vision correction surgery to be able to focus on an object 10 feet across the room. In orbit at Earth’s second Lagrange point (L2), far from the help of a terrestrial doctor, Webb will use its near-infrared camera (NIRCam) instrument to help align its primary mirror segments about 40 days after launch, once they have unfolded from their unaligned stowed position and cooled to their operating temperatures.
Laser vision correction surgery reshapes the cornea of the eye to remove imperfections that cause vision problems like nearsightedness. The cornea is the surface of the eye; it helps focus rays of light on the retina at the back of the eye, and though it appears to be uniform and smooth, it can be misshapen and pockmarked with dents, dimples, and other imperfections that can affect a person’s sight. The relative positioning of Webb’s primary mirror segments after launch will be the equivalent of these corneal imperfections, and engineers on Earth will need to make corrections to the mirrors’ positions to bring them into alignment, ensuring they will produce sharp, focused images.”
“This timelapse video shows Sentinel-5P satellite, from final preparations to liftoff on a Rockot launcher, from the Plesetsk Cosmodrome in northern Russia, on 13 October 2017.
The Sentinels are a fleet of satellites designed to deliver the wealth of data and imagery that are central to the European Commission’s Copernicus programme. This unique environmental monitoring programme is providing a step change in the way we view and manage our environment, understand and tackle the effects of climate change and safeguard everyday lives.
Sentinel-5 Precursor – also known as Sentinel-5P – is the first Copernicus mission dedicated to monitoring our atmosphere. The satellite carries the state-of-the-art Tropomi instrument to map a multitude of trace gases such as nitrogen dioxide, ozone, formaldehyde, sulphur dioxide, methane, carbon monoxide and aerosols – all of which affect the air we breathe and therefore our health, and our climate.
With a swath width of 2600 km, it will map the entire planet every day. Information from this new mission will be used through the Copernicus Atmosphere Monitoring Service for air quality forecasts and for decision-making. The mission will also contribute to services such as volcanic ash monitoring for aviation safety and for services that warn of high levels of UV radiation, which can cause skin damage. In addition, scientists will also use the data to improve our knowledge of important processes in the atmosphere related to the climate and to the formation of holes in the ozone layer.
Sentinel-5P was developed to reduce data gaps between the Envisat satellite – in particular the Sciamachy instrument – and the launch of Sentinel-5, and to complement GOME-2 on MetOp. In the future, both the geostationary Sentinel-4 and polar-orbiting Sentinel-5 missions will monitor the composition of the atmosphere for Copernicus Atmosphere Services. Both missions will be carried on meteorological satellites operated by Eumetsat. Until then, the Sentinel-5P mission will play a key role in monitoring and tracking air pollution.”
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