“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.”
“ICESat-2 (Ice, Cloud, and land Elevation Satellite 2), part of NASA’s Earth Observing System, is a planned satellite mission for measuring ice sheet elevation, sea ice freeboard as well as land topography and vegetation characteristics. ICESat-2 is a planned follow-on to the ICESat mission. It will be launched in 2018 from Vandenberg Air Force Base in California into a near-circular, near-polar orbit with an altitude of approximately 496 km. It is being designed to operate for 3 years, and will carry enough propellant for 7 years.
The ICESat-2 mission is designed to provide elevation data needed to determine ice sheet mass balance as well as vegetation canopy information. It will provide topography measurements of cities, lakes and reservoirs, oceans and land surfaces around the globe, in addition to the polar-specific coverage.
The ICESat-2 project is being managed by NASA Goddard Space Flight Center. The sole instrument is being designed and built by NASA Goddard Space Flight Center, and the bus is being provided by Orbital ATK. The satellite will launch on a Delta II rocket provided by United Launch Alliance. As of November 2017 this is the last planned launch of the Delta ll launch vehicle.
The sole instrument on ICESat-2 will be the Advanced Topographic Laser Altimeter System (ATLAS), a space-based LIDAR. ATLAS will time the flight of laser photons from the satellite to Earth and back; computer programs will use the travel time from multiple pulses to determine elevation. The ATLAS laser will emit visible laser pulses at 532 nm wavelength. The laser is being developed and built by Fibertek, Inc. As ICESat-2 orbits, the ATLAS will generate six beams arranged in three pairs, with the pairs 3.3 km apart, in order to better determine the surface’s slope and provide more ground coverage. ATLAS will take elevation measurements every 70 cm along the satellite’s ground path. The laser will fire at a rate of 10 kHz. Each pulse sends out about 20 trillion photons, almost all of which are dispersed or deflected as the pulse travels to Earth’s surface and bounces back to the satellite. About a dozen photons from each pulse return to the instrument and are collected in a beryllium telescope.”
Music: “Cristal Delight,” Fred Dubois, Killer Tracks
Ryan Fitzgibbons (USRA): Lead Producer
Kate Ramsayer (Telophase Corp.): Lead Writer
Ryan Fitzgibbons (USRA): Writer
Ryan Fitzgibbons (USRA): Lead Animator
Adriana Manrique Gutierrez (USRA): Animator
Thorsten Markus (NASA/GSFC): Lead Scientist
Thomas A. Neumann Ph.D. (NASA/GSFC): Lead Scientist
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