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Archive for the Spacecraft Design category

March 29, 2018

WFIRST

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NASA Goddard dixit:

“Scheduled to launch in the mid-2020s, the Wide Field Infrared Survey Telescope (WFIRST) will function as Hubble’s wide-eyed cousin. While just as sensitive as Hubble’s cameras, WFIRST’s 300-megapixel Wide Field Instrument will image a sky area 100 times larger. This means a single WFIRST image will hold the equivalent detail of 100 pictures from Hubble.

The mission’s wide field of view will allow it to generate a never-before-seen big picture of the universe, which will help astronomers explore some of the greatest mysteries of the cosmos, like why the expansion of the universe seems to be accelerating. Some scientists attribute the speed-up to dark energy, an unexplained pressure that makes up 68 percent of the total content of the cosmos.

The Wide Field Instrument will also allow WFIRST to measure the matter in hundreds of millions of distant galaxies through a phenomenon dictated by Einstein’s relativity theory. Massive objects like galaxies curve space-time in a way that bends light passing near them, creating a distorted, magnified view of far-off galaxies behind them. WFIRST will paint a broad picture of how matter is structured throughout the universe, allowing scientists to put the governing physics of its assembly to the ultimate test.

WFIRST can use this same light-bending phenomenon to study planets beyond our solar system, known as exoplanets. In a process called microlensing, a foreground star in our galaxy acts as the lens. When its motion randomly aligns with a distant background star, the lens magnifies, brightens and distorts the background star. WFIRST’s microlensing survey will monitor 100 million stars for hundreds of days and is expected to find about 2,500 planets, well targeted at rocky planets in and beyond the region where liquid water may exist.

These results will make WFIRST an ideal companion to missions like NASA’s Kepler and the upcoming Transiting Exoplanet Survey Satellite (TESS), which are designed to study larger planets orbiting closer to their host stars. Together, discoveries from these three missions will help complete the census of planets beyond our solar system. The combined data will also overlap in a critical area known as the habitable zone, the orbiting distance from a host star that would permit a planet’s surface to harbor liquid water — and potentially life.

By pioneering an array of innovative technologies, WFIRST will serve as a multipurpose mission, formulating a big picture of the universe and helping us answer some of the most profound questions in astrophysics, such as how the universe evolved into what we see today, its ultimate fate and whether we are alone. “

Video credit: NASA Goddard

 

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March 27, 2018

The Spica Rocket

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Copenhagen Suborbitals dixit:

“The development of the space capsule which will carry our astronaut up to and above the karman line and into space is progressing.

The space capsule which will be lifted by the Spica rocket to an altitude of over one hundred kilometers, or sixty two miles, will contain all systems necessary to enable it to not only bring the astronaut into space, but also bring him, or her, safely back to earth.”

Video credit: Copenhagen Suborbitals

 

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March 8, 2018

Explorer 1

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NASA dixit:

“Against the backdrop of the 1950s Cold War, after the Soviet Union successfully launched Sputnik, Americans were determined to launch their own Earth-orbiting satellite. Flash back to events leading up to the successful launch of America’s Explorer 1, and the beginnings of America’s Space Age, as told through newsreel and documentary clips of the time.”

Video credit: NASA

 

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March 7, 2018

Ariane 6 Launch Site

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ESA dixit:

“At Europe’s Spaceport in French Guiana, everything is being prepared to accommodate Europe’s newest launcher, Ariane 6. A new launch pad is under construction and the mobile gantry protecting the launcher will soon be visible. The new assembly building dimensions can now be fully seen as the outer shell is almost complete.

Ariane 6 will guarantee Europe’s independent access to space and should consolidate Arianespace’s leading role on the satellites launch market. The first Ariane 6 launch is scheduled for July 2020.”

Video credit: ESA

 

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March 6, 2018

Ariane 6 Vulcain 2.1 Engine Test

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ESA dixit:

“The first hot firing of Ariane 6’s Vulcain 2.1 main engine was performed in January 2018 at the DLR German Aerospace Center test facility in Lampoldshausen, Germany.

The engine, developed by ArianeGroup, has a simplified and more robust nozzle, a gas generator made through additive manufacturing, and an oxygen heater for oxygen tank pressurisation. These features lower the cost of the engine and simplify manufacturing.”

Video credit: Ariane Group

 

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February 28, 2018

Inside Mars

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NASA dixit:

“Even if rovers, balloons, and airplanes continuously move around and near the surface of Mars one day, we should never judge a planet by its cover. Today’s desert-like Martian surface likely hides the presence of water below ground. To “follow the water” to where it is today, we must go beneath the surface of the planet with subsurface explorers. The subsurface of Mars may resemble some of the colder parts of Earth. For example, in Antarctica or Iceland, we know that water is stored in a layer of permafrost and beneath that, as liquid groundwater. Even if the ancient surface water on Mars evaporated, there may still be substantial reservoirs of water, in either liquid or frozen form, in the subsurface.

The very first subsurface exploration of Mars for NASA will be in partnership with the European Space Agency (ESA) in their Mars Express mission. This spacecraft carries a subsurface radar instrument that will use a 40-meter (130-foot) antenna to detect and map subsurface water. Electric signals will be sent down the antenna, creating low-frequency radar waves. The radar waves will penetrate the Martian surface as deep as five kilometers (three miles) and will be reflected back to the spacecraft by different subsurface features, including water. This data will give us a three-dimensional understanding of where and how much water may be distributed in the Martian subsurface.

A lander on Mars Express called Beagle 2 will also carry the first robotic mole. Mimicking the behavior of the small furry earth-bound creatures that burrow into the ground, robotic moles will drill underground by pulverizing rock and soil, avoiding the need for a complex drill stem. Beagle 2’s mole will only have the ability to penetrate less than a meter (less than 3 feet) below the surface.

A much more capable mole is under development in NASA’s technology program. Weighing about 20 kilograms (44 pounds), it will be capable of drilling hundreds of meters (hundreds of yards) into the ground and possibly deeper at a rate of 10-20 meters (33 – 66 feet) a day. Excavated soil would be moved to the back of the mole and a small tube leading to the surface would help alleviate the pressure from the growing mounds of soil. The tube would also send soil samples back to the surface and carry power to the robotic mole. The samples sent up to the surface would be studied for scientific data such as mineral content and oxidation levels of subsurface soil. A mole drilling at the polar cap would study the layers of ice that tell the story of its history, much like the rings of a tree reveal many things from its past. All of this data would provide clues in the search for ancient, or possibly current, life.

Once we know in more detail where the water lies, the next step is to drill in those locations. To get to the zone where frozen water–and possible dormant life–might be present, we will probably need to drill to a depth of 200 meters (656 feet). Liquid groundwater will be even deeper. That’s no easy feat, but it’s critical for understanding the possibility of past or present life on Mars and for confirming that water resources are available for future human explorers.

Deep subsurface access on Mars will have unique challenges. First of all, unlike on Earth, we will not be able to use a drill to go through mud, water, or probably even gas pressure to carry the cuttings away from the bit. We will need new systems for fluidless drilling. Second, we will need an effective means of keeping the hole open while the drilling proceeds. On Earth, this task is normally done with steel casing, which is very heavy. Engineers are actively seeking alternative ways that don’t require us to send heavy equipment to Mars given the expense. Finally, we will have to develop systems that allow the drill to make operational decisions for itself. On Earth, drills can get stuck very quickly, so a Mars robotic drill or subsurface explorer must know how to recognize, avoid, and solve problems on its own.”

Video credit: NASA

 

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