OrbitalHub

NASA dixit:

“NASA’s Parker Solar Probe is in the midst of intense environmental testing at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, in preparation for its journey to the Sun. These tests simulate the noise and shaking the spacecraft will experience during its launch from Cape Canaveral, Florida, scheduled for 2018.

Parker Solar Probe’s integration and testing team must check over the spacecraft and systems to make sure everything is still in optimal working condition after experiencing these rigorous conditions – including a check of the solar arrays, which will provide electrical power to the spacecraft.

Parker Solar Probe will explore the Sun’s outer atmosphere and make critical observations that will answer decades-old questions about the physics of stars. The resulting data will also help improve how we forecast major eruptions on the Sun and subsequent space weather events that can impact life on Earth, as well as satellites and astronauts in space. The mission is named for Eugene N. Parker, whose profound insights into solar physics and processes have helped shape the field of heliophysics.”

Joy Ng (USRA): Producer

Sarah Frazier (ADNET SYSTEMS): Writer

Lee Hobson (APL): Videographer

Music credit: ‘Push Away’ by Andrew Michael Britton [PRS], David Stephen Goldsmith [PRS], Mikey Rowe [PRS] from Killer Tracks.

Video credit: NASA’s Goddard Space Flight Center

Planetary Resources dixit:

“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.”

Video credit: Planetary Resources

Planetary Resources dixit:

“Asteroid mining is the key to our future expansion into space.

Planetary Resources is conducting the first commercial exploration of resources on near Earth asteroids.

The first resource that we’re interested in is water. Water, when you break it down into the elements Hydrogen and Oxygen, is rocket fuel – currently the best way to get around the Solar System.

In much the same way that the economic activity on Earth is enabled by fossil fuels, in space, we will have a water-based economy. The Earth’s gravity well is so deep that the cost of bringing propellant from Earth to fuel that economy in space will be prohibitive.”

Read more about how asteroid mining is the key to our future expansion into space.

Video credit: Planetary Resources

ESA dixit:

“[This is a] Video showing a test of the mechanisms steering the four solar electric propulsion thrusters on BepiColombo’s Mercury Transfer Module (speeded up by 20 times). The module will use a combination of electric propulsion and multiple gravity assists at Earth, Venus and Mercury to carry BepiColombo’s two scientificorbiters – ESA’s Mercury Planetary Orbiter and Japan’s Mercury Magnetospheric Orbiter – to the innermost planet in our Solar System.

The test is designed to demonstrate that the mechanisms can reach their full steering range. The thruster mechanisms control the steering of the spacecraft during the long thrust arcs of the 7.2 year cruise to Mercury and as such are used for navigation, attitude control, and reaction wheel off-loading. Together with the onboard software, the mechanisms will update the direction of the thrust vector every five minutes relative to the spacecraft’s evolving centre of gravity. The thrusters will be fired for several months at a time between the gravity assist flybys.

This particular test was conducted in April 2017, before the spacecraft was put into the composite stack configuration. The same test will be repeated again later in the year to verify performance after the stack level vibration test campaign.”

Video credit: ESA

ESA dixit:

“The high performance of ESA’s new generation ‘Planetary and Asteroid Natural scene Generation Utility’ or Pangu software enables real-time testing of both landing algorithms and hardware. Entry, descent and landing on a planetary body is an extremely risky move: decelerating from orbital velocities of multiple km per second down to zero, at just the right moment to put down softly on an unknown surface, while avoiding craters, boulders and other unpredictable hazards.

But Pangu can generate realistic images of planets and asteroids on a real-time basis, as if approaching a landing site during an actual mission. This allows the testing of landing algorithms, or dedicated microprocessors or entire landing cameras or other hardware ‘in the loop’ – plugged directly into the simulation – or run thousands of simulations one after the other on a ‘Monte Carlo’ basis, to test all eventualities.

Seen here is a Pangu recreation of the Mars Curiosity’s rover’s approach to Mars, using original telemetry, and then a view of Mars moon Phobos. This is followed by another recreation the Japanese Hayabusa probe’s encounter with the rubble-strewn Itokawa near-Earth asteroid, and finally a telemetry-based recreation of the field of view of the New Horizons mission as it performed its rapid flyby of Pluto.

This new generation of Pangu was developed for ESA by the University of Dundee in Scotland.”

Video credit: ESA

NASA dixit:

“February 21, 2017. NASA’s Cassini spacecraft captured these remarkable views of a propeller feature in Saturn’s A ring. These are the sharpest images taken of a propeller so far, and show an unprecedented level of detail. The propeller is nicknamed “Santos-Dumont,” after the pioneering Brazilian-French aviator. This observation was Cassini’s first targeted flyby of a propeller. The views show the object from vantage points on opposite sides of the rings. The top image looks toward the rings’ sunlit side, while the bottom image shows the unilluminated side, where sunlight filters through the backlit ring.

The two images are reprojected at the same scale (0.13 mile or 207 meters per pixel) in order to facilitate comparison. Cassini scientists have been tracking the orbit of this object for the past decade, tracing the effect that the ring has upon it. Now, as Cassini has moved in close to the ring as part of its ring-grazing orbits, it was able to obtain this extreme close-up view of the propeller, enabling researchers to examine its effects on the ring. These views, and others like them, will inform models and studies in new ways going forward.

Like a frosted window, Saturn’s rings look different depending on whether they are seen fully sunlit or backlit. On the lit side, the rings look darker where there is less material to reflect sunlight. On the unlit side, some regions look darker because there is less material, but other regions look dark because there is so much material that the ring becomes opaque. Observing the same propeller on both the lit and unlit sides allows scientists to gather richer information about how the moonlet affects the ring. For example, in the unlit-side view, the broad, dark band through the middle of the propeller seems to be a combination of both empty and opaque regions. The propeller’s central moonlet would only be a couple of pixels across in these images, and may not actually be resolved here. The lit-side image shows that a bright, narrow band of material connects the moonlet directly to the larger ring, in agreement with dynamical models. That same thin band of material may also be obscuring the moonlet from view. Lengthwise along the propeller is a gap in the ring that the moonlet has pried open. The gap appears dark on both the lit and unlit sides. Flanking the gap near the moonlet are regions of enhanced density, which appear bright on the lit side and more mottled on the unlit side.

One benefit of the high resolution of these images is that, for the first time, wavy edges are clearly visible in the gap. These waves are also expected from dynamical models, and they emphasize that the gap must be sharp-edged. Furthermore, the distance between the wave crests tells scientists the width of the gap (1.2 miles or 2 kilometers), which in turn reveals the mass of the central moonlet. From these measurements, Cassini imaging scientists deduce that the moonlet’s mass is comparable to that of a snowball about 0.6 mile (1 kilometer) wide.”

Image credit: NASA/JPL-Caltech/Space Science Institute