Skip to main content

Can a Venus Lander Survive Longer Than a Few Minutes?

Sending a lander to Venus presents several huge engineering problems. Granted, we’d get a break from the nail-biting entry, descent and landing, since Venus’ atmosphere is so thick, a lander would settle gently to the surface like a stone settles in water — no sky cranes or retrorockets required.

But the rest of the endeavor is fraught with challenges. The average temperature at the surface is 455 degrees C (850 F), hot enough to melt lead. The mix of chemicals that make up the atmosphere, such as sulfuric acid, is corrosive to most metals. And the crushing atmospheric pressure is roughly equivalent to being 1,500 meters (5,000 ft) under water. These extreme environmental conditions are where metals and electronics go to die; therefore, the few Venus lander missions that have made it to the surface — like the Soviet Venera missions — only lasted two hours or less. Any future landers or rovers will need to have nearly super-hero-type characteristics to endure on the surface of Earth’s evil twin.

But there’s one additional challenge that might be close to being solved: creating batteries that can operate long enough in Venus’ hellish conditions to make a lander mission worth the effort.

NASA is working with a company called Advanced Thermal Batteries, Inc. (ATB) and together they created the first battery that has demonstrated the capability to operate at Venus’ temperatures for an entire Venus solar day, which is approximately 120 Earth-days.

Test battery hardware: High temperature thermal batteries adapted for the Venus surface. Image Credit: Dr. Michael Barclay, Advanced Thermal Batteries, Inc.

The battery is based on short-lived thermal battery systems used for powering smart missiles, The battery contains 17 individual cells and uses specifically designed chemistry and structural materials While the battery is still in development, engineers are encouraged that tests conducted demonstrate that these types of batteries are capable of operating in harsh environments like on Venus. Additionally, this advanced type of battery technology may provide a new energy storage device for future exploration in harsh environments across the Solar System.

“This recent battery technology demonstration, with improved architecture and low self-discharge electrochemistry, is a huge accomplishment that many may have not thought possible,” said Dr. Kevin Wepasnick, ATB Project Engineer, in a NASA press release.

Batteries appear to be the only solution for powering a Venus lander. Solar panels are not viable due to surface light levels being comparable to an overcast day on Earth, and current solar panel designs would not withstand the high surface pressures. A radioisotope thermoelectric generator (RTG) requires bringing a heat source to the surface of Venus, and since heat management is already a major mission challenge, this method is not a good option.

But on Venus, thermal batteries can utilize the ambient atmospheric conditions to heat a special high-temperature electrolyte that is solid and inert at standard room temperature. Additionally, they can remain operational without the need for pyrotechnics or thermal insulation.

NASA says this new battery approach has demonstrated high-temperature operation for unprecedented periods of time, and lays the foundation for a new paradigm in battery technology and for Venus landers.

Conceptual image of Long-Lived In situ Solar System Explorer (LLISSE) on the Venus compared to larger traditional landers. Image Credit: John Wrbanek, NASA GRC.

The work on the new type of thermal battery is part of ongoing work at NASA Glenn Research Center to develop a small Venus lander called the Long-Lived In situ Solar System Explorer (LLISSE). The program uses the latest advances in high-temperature systems and a novel concept of operations to allow operations on the surface of Venus for 60 days or longer while the lander collects science data and transmits it to a Venus orbiter.

LLISSE is intended to be approximately 10 kg (22 lbs) and carry a suite of small sensors to measure winds, radiance, temperature, pressure, and abundances of key atmospheric chemical constituents. LLISSE will be a complete system with electronics, communications, and instrumentation—all of which will require a battery to operate.

ATB says they expect that a complete prototype Venus battery system will be demonstrated in the next 18 months.

Read more about the new battery here.

The post Can a Venus Lander Survive Longer Than a Few Minutes? appeared first on Universe Today.



from Universe Today https://ift.tt/BF4WPVu
via IFTTT

Comments

Popular posts from this blog

Researchers Match Up 12 Meteorites with the Near-Earth Asteroids They Came From

Every day meteoroids blast through our planet’s atmosphere to hit the ground as meteorites. A team of researchers in Italy traced twelve of them to progenitor asteroids that orbit in near-Earth space. Scientists treasure meteorites because they reveal information about their parent bodies. In an arXiv paper, two Italian researchers—Albino Carbognani and Marco Fenucci—analyze the characteristics of the parent bodies of 20 selected meteorites. They were able to track all but eight back to their parent asteroids. Based on their work, the pair says at least a quarter of meteorites come from collisions that happened in near-Earth space and not in the Main Belt. Meteorites from Near-Earth Asteroids: How They Got Here Many meteorites are chondritic, similar to asteroids in the Main Belt (or came from it). In their paper, the authors point out that progenitor meteoroids (including many that fall to Earth and become meteorites) formed millions of years ago following collisions between main-...

JWST Takes a Detailed Look at Jupiter’s Moon Ganymede

Nature doesn’t conform to our ideas of neatly-contained categories. Many things in nature blur the lines we try to draw around them. That’s true of Jupiter’s moon Ganymede, the largest moon in the Solar System. The JWST took a closer look at Ganymede, the moon that’s kind of like a planet, to understand its surface better. Ganymede is basically a planet, except it doesn’t orbit the Sun. If it did orbit the Sun instead of Jupiter, it would be indistinguishable from a planet. It has a differentiated internal structure with a molten core that produces a magnetic field. It has a silicon mantle much like Earth’s, and has a complex icy crust with a deep ocean submerged beneath it. It has an atmosphere, though it’s thin. It’s also larger than Mercury, and almost as large as Mars. According to the authors of a new study, it’s an archetype of a water world. But even with all this knowledge of the huge moon, there are details yet to be revealed. This is especially true of its complex surface...

The Ultraviolet Habitable Zone Sets a Time Limit on the Formation of Life

The field of extrasolar planet studies has grown exponentially in the past twenty years. Thanks to missions like Kepler, the Transiting Exoplanet Survey Satellite (TESS), and other dedicated observatories, astronomers have confirmed 5,690 exoplanets in 4,243 star systems . With so many planets and systems available for study, scientists have been forced to reconsider many previously-held notions about planet formation and evolution and what conditions are necessary for life. In the latter case, scientists have been rethinking the concept of the Circumsolar Habitable Zone (CHZ). By definition, a CHZ is the region around a star where an orbiting planet would be warm enough to maintain liquid water on its surface. As stars evolve with time, their radiance and heat will increase or decrease depending on their mass , altering the boundaries of the CHZ. In a recent study , a team of astronomers from the Italian National Institute of Astrophysics (INAF) considered how the evolution of star...