Astronomy

On this Earth Day, we reflect on the importance of protecting our planet for future generations. Understanding the Earth system and the complex interactions that shape our planet is paramount for addressing environmental challenges, mitigating climate change, preparing for natural disasters, managing resources sustainably and conserving biodiversity.

Each component of the Earth system – from the atmosphere and oceans to land surfaces and ice sheets – influences and interacts with one another in complex ways. ESA works all-year round to provide satellite data to monitor the health of our planet. Here are 10 examples of how Earth’s systems intertwine and how satellite measurements are key to understanding these complex processes.

An Australian bull ant is the first animal known to use the patterns produced by polarised moonlight to navigate its environment

An Australian bull ant is the first animal known to use the patterns produced by polarised moonlight to navigate its environment

I really can’t believe that the Ingenuity helicopter on Mars took its maiden voyage in April 2021. On the 16th April 2024, engineers at NASA have received the final batch of data from the craft which marks the final task of the team. Ingenuity’s work is not over though as it will remain on the surface collecting data. For the engineers at NASA, they have their sights set on Dragonfly, a new helicopter destined for Titan.

When Ingenuity took off on its maiden voyage it became the first powered craft to achieve flight on an alien world. It has completed 128.8 minutes of flight covering 17 kilometres. It has extra large rotor blades to achieve lift in the thin martian atmosphere and has performed excellently providing guidance and targets for the Perseverance Rover to study close up. 

Ingenuity helicopter

It’s surprising to think that Ingenuity was only ever designed to be a short-lived demonstration mission. Over a period of 30 days, Ingenuity was to perform five experimental test flights and operate over three years. Unfortunately a rather hard landing damaged its rotor blades rendering it unable to fly again. It’s now sat at Airfield Chi in the now named “Valinor Hills” area of Mars. The team gave the region the nickname as a homage to the final residence of the immortals in Lord of the Rings. 

With Ingenuity now unable to fly the team had sent a software update to direct it to continue to collect data even if the Rover is unavailable. This will mean that it will wake each morning, test the (non-flight) systems are operational, take a colour image of the surface and record the temperature. The team believe such long term data could help to inform martian weather studies and help future explorers. This is a long term purpose for Ingenuity and it has the capability to store data for 20 years! If system or battery failure occurs the data will still be securely stored. The only way to retrieve the data though, will be through another autonomous craft or a human visitor of the future. 

The success of Ingenuity paved the way for a new era of planetary exploration. Next up is Dragonfly, a mission to Saturn’s moon Titan. Costing a total of $3.35 billion across its entire lifecycle it will become the fourth mission in NASA’s New Frontiers Program. The probe will be managed by the Marshall Space Flight Centre but behind them is an international team from many different organisations including but not limited to Goddard Space Flight Centre in Maryland; Penn State University in State College, Pennsylvania; Centre National d’Etudes Spatiales in Paris; the German Aerospace Centre in Cologne, Germany; and JAXA (Japan Aerospace Exploration Agency) in Tokyo.

Artist’s concept of Dragonfly soaring over the dunes of Saturn’s moon Titan. Credit: NASA/Johns Hopkins APL/Steve Gribben

Dragonfly is slated to arrive in 2034. It’s mission will be to visit multiple locations, sampling the minerals to search for prebiotic chemical processes. It will also look for chemical signatures that indicate water-based and/or hydrocarbon-based life. Unlike Ingenuity, its rotors are similar size to those you would find on a drone on Earth. The atmosphere is thick and so there is no need for super-sized blades. 

Source : NASA’s Ingenuity Mars Helicopter Team Says Goodbye … for Now and NASA’s Dragonfly Rotorcraft Mission to Saturn’s Moon Titan Confirmed

The post The Ingenuity Team Downloads the Final Data from the Mars Helicopter. The Mission is Over appeared first on Universe Today.

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NASA’s Juno spacecraft came within 1,500 km (930 miles) of the surface of Jupiter’s moon Io in two recent flybys. That’s close enough to reveal new details on the surface of this moon, the most volcanic object in the Solar System. Not only did Juno capture volcanic activity, but scientists were also able to create a visual animation from the data that shows what Io’s 200-km-long lava lake Loki Patera would look like if you could get even closer. There are islands at the center of a magma lake rimmed with hot lava. The lake’s surface is smooth as glass, like obsidian.

“Io is simply littered with volcanoes, and we caught a few of them in action,” said Juno principal investigator Scott Bolton during a news conference at the European Geophysical Union General Assembly in Vienna, Austria. “There is amazing detail showing these crazy islands embedded in the middle of a potentially magma lake rimmed with hot lava. The specular reflection our instruments recorded of the lake suggests parts of Io’s surface are as smooth as glass, reminiscent of volcanically created obsidian glass on Earth.”

This animation is an artist’s concept of Loki Patera, a lava lake on Jupiter’s moon Io, made using data from the JunoCam imager aboard NASA’s Juno spacecraft. With multiple islands in its interior, Loki is a depression filled with magma and rimmed with molten lava. Credit: NASA/JPL-Caltech/SwRI/MSSS

Just imagine if you could stand by the shores of this lake – which would be a stunning view in itself. But then, you could look up and see the giant Jupiter looming in the skies above you.

Juno made the two close flybys of Io in December 2023 and February 2024. Images from Juno’s JunoCam included the first close-up images of the moon’s northern latitudes. Undoubtedly, Io looks like a pizza – which has been the conclusion since our first views of this moon, when Voyager 1 flew through the Jupiter system in March 1979. The mottled and colorful surface comes from the volcanic activity, with hundreds of vents and calderas on the surface that create a variety of features. Volcanic plumes and lava flows across the surface show up in all sorts of colors, from red and yellow to orange and black. Some of the lava “rivers” stretch for hundreds of kilometers.

Io’s sub-Jovian hemisphere is revealed in detail for the first time since Voyager 1 flew through the Jupiter system in March 1979, during the Juno spacecraft’s 58th perijove, or close pass, on February 3, 2024. This image shows Io’s nightside illuminated by sunlight reflected off Jupiter’s cloud tops. Several surface changes are visible include a reshaping of the compound flow field at Kanehekili (center left) and a new lava flow to the east of Kanehekili. This image has a pixel scale of 1.6 km/pixel. Credit : NASA/SwRI/JPL/MSSS/Jason Perry.

Juno scientists were also able to re-create a spectacular feature on Io, a spired mountain that has been nicknamed “The Steeple.” This feature is between 5 and 7 kilometers (3-4.3 miles) in height. It’s hard to comprehend the type of volcanic activity that could have created such a stunning landform.

Created using data collected by the JunoCam imager aboard NASA’s Juno during flybys in December 2023 and February 2024, this animation is an artist’s concept of a feature on the Jovian moon Io that the mission science team nicknamed “Steeple Mountain.” Credit: NASA/JPL-Caltech/SwRI/MSSS

Speaking of volcanic activity, two recent papers have come to a jaw-dropping conclusion about Io: this moon has been erupting since the dawn of the Solar System.

All the volcanic on Io is activity is driven by tidal heating. Io is in an orbital resonance with two other large moons of Jupiter, Europa and Ganymede.

“Every time Ganymede orbits Jupiter once, Europa orbits twice, and Io orbits four times,” explained the authors of a paper published in the Journal of Geophysical Research: Planets, led by Ery Hughes of GNS Science in New Zealand. “This situation causes tidal heating in Io (like how the Moon causes ocean tides on Earth), which causes the volcanism.”

However, scientists haven’t known how long this resonance has been occurring and whether what we observe today is what has always been happening in the Jupiter system. This is because volcanism renews Io’s surface almost constantly, leaving little trace of the past.

Jupiter’s orbital system with the host planet and orbits to scale. Image credit: James Tuttle Keane / Keck Institute for Space Studies

The team of scientists, led by Katherine de Kleer at Caltech and Hughes at GNS Science used the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile observe the sulphur gases in Io’s atmosphere. The isotopes of sulfur were used as a tracer of tidal heating on Io because sulfur is released through volcanism, processed in the atmosphere, and recycled into the mantle. Additionally, some of the sulfur is lost to space, and because of Jupiter’s magnetosphere, a bunch of charged particles whirling around Jupiter that hit Io’s atmosphere continuously.

It turns out that the sulfur that is lost to space on Io is a little bit isotopically lighter than the sulfur that is recycled back into Io’s interior. Because of this, over time, the sulfur remaining on Io gets isotopically heavier and heavier. How much heavier depends on how long volcanism has been taking place.

What the teams found is that tidal heating on Io has been occurring for billions of years.

“The isotopic composition of Io’s inventory of volatile chemical elements, including sulfur and chlorine, reflects its outgassing and mass loss history, and thus records information about its evolution,” the team wrote in the paper published in Science. “These results indicate that Io has been volcanically active for most (or all) of its history, with potentially higher outgassing and mass-loss rates at earlier times.”

Juno continues to makes its way through the Jupiter system. And during Juno’s most recent flyby of Io, on April 9, the spacecraft came within about 16,500 kilometers (10,250 miles) of the moon’s surface. It will perform its 61st flyby of Jupiter on May 12.

JunoCam is a public camera, where members of the public can choose targets for imaging, as well as process all the data.  JunoCam’s raw images are available here for the public to peruse and process into image products. Here you can see the most recent images that have been processed.

Papers: Isotopic Evidence of Long-Lived Volcanism on Io
Using Io’s Sulfur Isotope Cycle to Understand the History of Tidal Heating
Further Reading: NASA, GNS Science

The post Juno Reveals a Giant Lava Lake on Io appeared first on Universe Today.

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It was 1903 that the Wright brothers made the first successful self-propelled flight. Launching themselves to history, they set the foundations for transatlantic flights, supersonic flight and perhaps even the exploration of the Solar System. Now we are on the precipice of travel among the stars but among the many ideas and theories, what is the ultimate and most effective way to explore our nearest stellar neighbours? After all, there are 10,000 stars within a region of 110 light years from Earth so there are plenty to choose from. 

It’s not just the stars that entice us to explore beyond our Solar System. Ever since the first exoplanet discovery in 1992 we have been discovering more and more alien worlds around distant stars. The tally has now reached over 5,500 confirmed exoplanets and they too demand our attention as we reach out among the stars. There have been many ideas and technologies proposed over the past few years but to date, even Proxima Centauri (the nearest star system to our own) remains out of reach. 

In his thesis recently published, lead author Johannes Lebert from the Technische Universität München (TUM) attempts to develop a strategy, based on existing interstellar probe concepts and knowledge of nearby star systems. Lebert was driven by the exoplanet discoveries that continue at pace and the development and interest, both commercially and technically in interstellar probes. Not only does he explore the technologies but he also looks at the returns too. 

Artist’s illustration of HD 104067 b, which is the outermost exoplanet in the HD 104067 system, and responsible for potentially causing massive tidal energy on the innermost exoplanet candidate, TOI-6713.01. (Credit: NASA/JPL-Caltech)

In the strategy developed in the thesis he looks at the two main objectives which are duration of the mission and the returns. By returns he refers to the sum of all rewards provided by the stars explored during the mission and of course be largely scientific.  He considers a multi vehicle approach using several probes which do not return to Earth and are capable of exploring different stars thereby maximising the mission returns. Finally he explores the routing of such a mission to ensure maximum mission returns. Succinctly he calls this his ‘Bi-objective multi- vehicle open routing problem with profits.’

The thesis concludes with several recommendation. First that the use of efficient routing around the stars, a more limited number of probes can be used, limiting reducing fuel costs. This should be balanced by the mission returns which increase faster should more probes be used to explore the same number of stars simultaneously. This does however increase mission costs due to increase fuel costs. Whichever strategy is used, small-scale remotely operated or autonomous craft are far more suited to the need. 

Lebert goes on to explain that higher probe numbers also brings the benefit that probes can be tailored to suit the star systems they are destined to explore. Unlike a smaller number of probes that will have to cater for a greater range of systems.  There is a concept known as the ‘derived scaling law’ which articulates that higher probe numbers do inherit a risk of less efficient deployment.

It’s an interesting read that reminds us that, whilst we are developing the probes, and there are quite a number on the drawing board; Breakthrough Starshot, Interstellar Express, Interstellar Probe, Innovative Interstellar Explorer, Tau Mission to name a few, we do need to consider just how we plan, manage and deploy to maximise the scientific gain. 

Source : Optimal Strategies for the Exploration of Near-by Stars

The post What’s the Most Effective Way to Explore our Nearest Stars? appeared first on Universe Today.

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