Euclid space mission to map the “dark Universe” embarks on epic journey

A European mission to explore how gravity, dark energy and dark matter has shaped the Universe has launched following £37 million UK Space Agency funding.

The Euclid space telescope will map the “dark Universe” by observing billions of galaxies out to 10 billion lightyears, across more than a third of the sky, to gather data on how its structure has formed over its cosmic history.

Led by the European Space Agency (ESA) and a consortium of 2,000 scientists across 16 countries, Euclid will spend six years venturing through space with two scientific instruments: a UK-built visible imager (VIS) that will become one of the largest cameras ever sent into space, and a near infrared spectrometer and photometer, developed in France.

Secretary of State for Science and Technology Chloe Smith said: “The launch of the Euclid mission is a truly significant moment. Backed by £37 million in UK funding and supported by our remarkable scientific talent and expertise, the mission will launch one of the largest cameras ever into space to look out across our universe.

“The mission will gain unparalleled insight into the mysteries of how the Universe was formed, delivering ground-breaking discoveries that will redefine what we know about space.”

Dr Paul Bate, Chief Executive of the UK Space Agency, said: “Watching the launch of Euclid, I feel inspired by the years of hard work from thousands of people that go into space science missions, and the fundamental importance of discovery – how we set out to understand and explore the Universe.

“The UK Space Agency’s £37 million investment in Euclid has supported world-class science on this journey, from the development of the ground segment to the build of the crucial visible imager instrument, which will help humanity begin to uncover the mysteries of dark matter and dark energy.”

The Euclid spacecraft being loaded into the SpaceX Falcon 9 fairing ahead of launch, on 27 June 2023. Credit: SpaceX.

Euclid took off on board a SpaceX spacecraft from Cape Canaveral in Florida at 4.12pm (BST) on 1 July.

The UK Space Agency’s funding goes back to 2010, up to 2024, and is divided between teams at University College London, The Open University, University of Cambridge, University of Edinburgh, University of Oxford, University of Portsmouth and Durham University.

All these institutions have contributed to the development and implementation of the Euclid UK Science Ground Segment (UKSGS), which runs the Euclid data analysis. Led by the University of Edinburgh, which hosts Euclid’s UK Science Data Centre (SDC-UK), the UKSGS will process hundreds of petabytes of data over the next six years to produce maps of the galaxies and dark matter of the Universe.

The wider Euclid Consortium includes experts from 300 organisations across 13 European countries, the US, Canada and Japan.

The Science and Technology Facilities Council (STFC) also contributed to design and development work on Euclid instrumentation and provided funding to UK astronomy teams who will analyse the data returned from the mission, including studies on the physics responsible for the observed accelerated expansion of the Universe.

Executive Chair at STFC Professor Mark Thomson said: “Euclid will answer some of the biggest and most profound questions we have about the Universe and dark energy. Congratulations to everyone involved in the design, construction and launch of Euclid – we are opening a new window on the cosmos.

“This is a fantastic example of close collaboration between scientists, engineers, technicians, and astronomers across Europe working together to tackle some of the biggest questions in science.”

Research funded by the UK Space Agency

University College London (MSSL and P&A) – Design, build and testing of Euclid’s VIS optical camera (£20.5 million)

UCL researchers have led on designing, building and testing the VIS optical camera, one of Euclid’s two instruments, working with teams at Open University as well as in France, Italy and Switzerland.

The core electronics for the instrument, including its complex array of 36 CCDs (that convert photons into electrons), were built at UCL’s Mullard Space Science Laboratory.

The camera, one of the largest ever sent into space, will take high resolution, panoramic images of a large swathe of the Universe, going back 10 billion years and covering a third of the night sky.

Professor Benjamin Joachimi (UCL Physics & Astronomy) is also playing a key role in the ground-based part of the mission (the ground segment), converting Euclid’s raw data into statistical summaries that can be compared to our current theoretical models of the universe.

Professor Mark Cropper, leader of the VIS camera team at UCL Mullard Space Science Laboratory, said: “The VIS instrument will image a large swathe of the distant Universe with almost the fine resolution of the Hubble Space Telescope, observing more of the Universe in one day than Hubble did in 25 years.

“The data will allow us to infer the distribution of dark matter across the Universe more precisely than ever before. The galaxies being imaged are up to 10 billion years old so we will also see how dark matter has evolved over most of the Universe’s history. The Universe on this scale has not yet been seen in this level of detail.”

Professor Tom Kitching, one of four science co-ordinators for Euclid, said: “The puzzles we hope to address are fundamental. Are our models of the Universe correct?

“What is dark energy? Is it vacuum energy – the energy of virtual particles popping in and out of existence in empty space? Is it a new particle field that we didn’t expect? Or it may be Einstein’s theory of gravity that is wrong.

“Whatever the answer, a revolution in physics is almost guaranteed.”

University of Edinburgh (£8.9 million)

Edinburgh has been involved in the design and build of Euclid from its earliest days –  leading the Euclid gravitational lensing data analysis, the UK Data Science Analysis and host to the UK’s Euclid Science Data Centre which will process hundreds of petabytes of data throughout the mission.

Professor Andy Taylor, leader of the gravitational lensing analysis for Euclid, the UK’s Euclid Science Data Analysis and SDC-UK, said: “This is a very exciting time for astronomy, and cosmology in particular.

“Euclid is designed to answer some of the biggest questions we have about the Universe. It has been a lot of hard work by many scientists to get here, but the results could change how we understand nature.

Professor Alkistis Pourtsidou, leader of Euclid’s nonlinear modelling team said: “Euclid is going to provide a very large and very detailed 3D map of the Universe, across the sky and along time.

“This map is a remarkable achievement combining state-of-the-art science and engineering. We want to extract the maximum amount of information from it and use it to figure out how nature works at the most fundamental level.

Dr Alex Hall, deputy leader of the gravitational lensing science working group, said: With the launch of Euclid begins an astronomical observing campaign that is amongst the most ambitious ever attempted.

“By imaging over a billion galaxies, Euclid will allow us to make a map of dark matter with unprecedented precision that will answer fundamental questions about our Universe. The next few years are going to be very exciting, and it is a privilege to be part of this incredible project.”

University of Oxford – Developing lensing signal measurement and correction for the effects of telescope and detectors on the data (£2.1 million)

Oxford’s Department of Physics has played a significant role in the lensing data analysis. As well as contributing to the development of the method used to measure the lensing signal, the team have specialised in correcting for the effects that the telescope and imaging detectors have on the data.

No telescope system is perfect – there is always some blurring and distortion of the images – and Oxford’s role has been not only to build the software models but also to devise ways of calibrating those models using dedicated in-orbit data from Euclid. These are crucial steps that allow the lensing measurements to be used to explore the dark side of our Universe.

Professor Lance Miller, leader of the work at the University of Oxford, said: “This is an incredibly exciting time.

“This space mission is the result of years of work and for us here in Oxford, that work continues as we put the finishing touches to the software that will be analysing some of the first Euclid data sent back to Earth, from August onwards.

“I have been working on Euclid since its inception, so to have reached this major milestone today is extraordinary. It is fantastic to be part of a mission that could play a fundamental role in our understanding of the Universe.

University of Portsmouth – Writing code for data analysis (£1.8 million)

The University of Portsmouth’s team, led by Ernest Rutherford Fellow, Dr Seshadri Nadathur, has been working with the wider European team, writing code that will help analyse data from the spacecraft.

Dr Seshadri Nadathur, from Portsmouth’s Institute of Cosmology and Gravitation, said: “Galaxies are not randomly scattered around the sky – instead there are patterns in their positions that are relics of correlations created at the time of the Big Bang, shaped over billions of years by the interplay of gravity pulling galaxies together and the expansion of the Universe driving them apart.

“By measuring and understanding these patterns in the maps Euclid will provide, we will learn about the mysterious force of dark energy that seems to be driving the Universe to expand ever faster.

“The team at Portsmouth has been busy developing and testing software that builds the maps and allows them to correct for any spurious patterns in the galaxy positions that arise purely due to variations in the performance of the telescope and instruments, so that we can isolate the true cosmological patterns we are interested in.”

Durham University – Building Euclid tolerance to radiation and supercomputer mock data (£1.3 million)

Professor Richard Massey, of Durham University’s Centre for Extragalactic Astronomy/Institute for Computational Cosmology, is a founder of the Euclid mission and has been developing its design and science goals for 20 years.

Work from a team of international researchers has included making Euclid’s camera more tolerant to the high radiation environment in which it will need to survive above the Earth’s atmosphere, learning from our experience with the Hubble Space Telescope.

As well as leading on Euclid’s radiation monitoring and mitigation strategy, Durham has used supercomputer simulation capabilities to create mock data to train Euclid’s analysis software, which will be compared against the spacecraft’s real observations.

Professor Richard Massey said: “When exploring any wild new frontier, the first step is to map the land. Euclid will make the largest ever map (with a tiny ‘you are here’ at the centre) and will show the invisible Universe.

“By revealing where dark matter and dark energy hide, we hope to take the second step – to discover what they are and trigger a gold rush of new science about how they behave.

“Euclid is like the Hubble Space Telescope, but with a wide-angle view. It will let astronomers stand back and see the sweeping vista of the Universe – but with the same high-resolution detail.

“Exploring and mapping new frontiers is the most human thing possible. Helping shape our next look into the dark has been a privilege.

“It has taken 20 years to make Euclid’s technology possible, engineer its details, and navigate the politics of competing against other proposed missions that would all discover amazing things. That rocket carries the sense of exploration and lifetimes’ work of thousands of scientists and engineers.”

The Open University – Developing and testing VIS detectors (£1.2 million)

The Open University’s Centre for Electronic Imaging (CEI) has been involved in developing the detectors for the VIS instrument and testing how they will perform in the harsh radiation environment in space.

The team will continue to monitor the detectors during the mission, to help mitigate the effects of the damage caused by high energy particles outside the Earth’s protective atmosphere, allowing Euclid to return the best possible science for the mission lifetime.

Dr Jesper Skottfelt, CEI Fellow at The Open University, said: “After 15 years of CEI involvement in the Euclid mission, it is exciting to see the spacecraft being launched.

“Our study of the VIS detectors has led to the development of new techniques to correct the effects of radiation damage which will enhance science return for this and future space missions.

“We look forward to seeing the progress Euclid will deliver towards answering some of the most fundamental questions we have about our Universe.

University of Cambridge – Developing astrometric calibration pipeline for Euclid image data (£870,000)

The University of Cambridge’s Institute of Astronomy (IoA) team has been involved in Euclid since 2010, supporting development of the astrometric calibration pipeline for the optical image data from Euclid, ensuring that the positions of the billions of sources to be imaged by Euclid can be determined to exquisite accuracy.

Nicholas Walton, leader of the IoA Euclid team and a Director of Research at the University of Cambridge, said: Dark energy and dark matter fundamentally govern the formation and evolution of our Universe.

“The Euclid mission will finally uncover the mysteries of how these ‘dark’ forces have shaped the cosmos that we see today, from life here on Earth, to our Sun, our Milky Way, our nearby galaxy neighbours, and the wider Universe beyond.”

Jupiter icy moon explorer begins journey to discover new worlds

The mission will study Jupiter’s moons for potential habitability for life

The Jupiter icy moons mission (JUICE) has taken off on its journey to study Jupiter, our largest planet, and investigate whether some of its icy moons are home to conditions that could support life.

Funded by the UK Space Agency, the UK leads on one of the 10 science instruments on board the European Space Agency’s Jupiter Icy Moons Explorer (JUICE) and has contributed to the development of two more.

Blasting off from Kourou in French Guiana at 1:14pm BST on Friday 14 April, JUICE will spend eight years travelling to the Jupiter system. On the way, it will perform fly-bys of Earth and Venus, using the gravitational fields of the planets to generate enough speed to reach Jupiter. One of these will be the first ever lunar-Earth gravity assist manoeuvre.

Secretary of State for Science, Innovation and Technology, Michelle Donelan, said: “The UK Space Agency has invested around £9 million in the JUICE mission to explore Jupiter and its moons. UK tech on the spacecraft illustrates how our world class universities and research institutions are unlocking deep space exploration.

“I want the UK’s space sector to continue thriving and encourage STEM learning for the next generation. It’s important that we push the boundaries of science, innovation and technology across the country to support the jobs of the future.”

On arrival in 2031, JUICE will circle Jupiter and fly past moons Ganymede, Europa and Callisto, making observations and taking measurements, studying the Jovian system as an archetype for gas giants elsewhere in the universe.

Finally in December 2034, JUICE will transfer into orbit around Ganymede, becoming the first spacecraft ever to orbit a moon other than Earth’s. While up close and personal with Ganymede, the mission will investigate the giant ocean that scientists believe hides under its icy crust, seeking evidence of habitability.

Dr Caroline Harper, Head of Space Science at the UK Space Agency, said: “The launch of JUICE marks years of hard work and collaboration by scientists, engineers and space agencies all over the world, but the journey is far from over.

“We look forward to following the spacecraft as it makes its eight-year trip to Jupiter and then as it studies the planet and its moons, using specialised UK-developed science instruments.

“We have a large community of research experts in the UK who are eagerly awaiting the data that JUICE will provide. With this information we hope to discover more about the nature of gas giants in space, and their icy moons, bringing us another step closer to understanding the evolution of the Universe.”

Ariane 5 rocket launching
JUICE lifting off. Credit: ESA – M. Pédoussaut

The UK Space Agency invested £9 million into the JUICE science payload, by supporting three critical instruments on board, which are:

  • J-MAG (UK-led magnetometer) – Development led by Imperial College London with radiation-hardness and mechanical design contributed by the University of Leicester.
  • JANUS (Italian-led optical camera system) – Imaging sensors developed by Teledyne-e2v in the UK, then tested, calibrated and characterised by Open University.
  • PEP (Swedish-led particle environment package) – Solid-state detectors provided by University College London and radiation design for instrument suite contributed by Aberystwyth University.

Principal Investigator for the J-MAG instrument at Imperial College London, Professor Michele Dougherty, has been involved in JUICE since well before it was selected by ESA in 2014 as the first Large Class mission in its Cosmic Vision Science Programme.

Professor Michele Dougherty, Head of the Department of Physics at Imperial College London, said: “With our instrument’s measurements, we are almost looking inside these worlds.

“What we’re doing, however, is extremely difficult, as the signals we’re trying to detect are extremely small. It’s like trying to find lots of needles in a haystack, and those needles are changing shape and colour all the time. But we think the results are going to be spectacular.

“Space missions are long and slow, so launch only marks the halfway point of this one – because we first started thinking about it 15 years ago, and we’ll be getting the last data in 15 years’ time. But I can’t wait for launch to happen because that’s the next milestone for us – we’ll be on our way to Jupiter.

JUICE is a collaboration between ESA, NASA and the space agencies of Japan and Israel and will consider two key themes from ESA’s Cosmic Vision 2015 – 2025: What are the conditions for planet formation and the emergence of life? And how does the Solar System work?

After taking off on an Ariane 5 launch vehicle from Kourou in French Guiana it is expected to arrive at Jupiter in July 2031 and complete 35 icy moon flybys before arriving at Ganymede – the largest of Jupiter’s moons – by December 2034.

JUICE will spend its eight-year voyage productively; it will pass by Venus to test and calibrate its instruments, gather data and take advantage of the gravity assist to save on fuel. Meanwhile, scientists on the ground will work on finalising software and data modelling in time for arrival at Jupiter.

Chiaki Crews, Research Fellow at the Open University, said: “The JUICE mission aims to answer many exciting questions, including whether the ocean worlds beneath the surfaces of Jupiter’s icy moons could potentially harbour life. One of the many instruments needed to make detailed scientific observations to help answer such questions is a camera.

“Our team at the Open University has spent several years testing and optimising a new image sensor for JUICE’s scientific camera, JANUS. A large part of our work was to irradiate test sensors with high doses of radiation, just like it is expected to experience during the JUICE mission lifetime, to check that JANUS will still be able to take images without too much degradation.

“We are now very much looking forward to watching the launch, albeit we’ll have to wait patiently for several more years before we’ll see the first images sent back from Jupiter’s moons.”

Professor Geraint Jones at University College London’s Mullard Space Science Laboratory, said: “It’s fantastic to see JUICE, carrying the PEP instrument that we contributed to, nearing its launch. We look forward to seeing data from our sensors on the ‘soup’ of ions, electrons and atoms surrounding Jupiter and its moons.

“This data will help us, for instance, to understand how particles around Jupiter reach such high energies – energies that could be fatal for an astronaut. We are excited that the mission will shed new light on worlds that could potentially host life.”

Professor Emma Bunce, Director of the Institute for Space at the University of Leicester, said: “The JUICE mission represents the next logical step in our exploration of potentially habitable worlds in the outer solar system. The JUICE spacecraft will do that via multiple flybys of Europa, Ganymede and Callisto, and eventually from a dedicated orbit at Ganymede towards the end of the mission.

“After many years of hard work from science, engineering, and industry teams, we are so excited that the JUICE mission is finally ready to launch and start its long journey to the Jupiter system. We will patiently await the incredible data that we expect to receive from 2031, and we are confident that it will absolutely be worth the wait!”

Professor Manuel Grande, Head of Solar System Physics at Aberystwyth University’s Department of Physics, said: “The major challenge when visiting the icy moons of Jupiter, in particular Europa, is the extreme radiation environment which would interfere with the spacecraft’s instrumentation and swamp any readings.

“The innovative design of the shielding, which was pioneered at Aberystwyth, makes it possible to avoid the effects of radiation on readings and allow for the detection of organic molecules in the neighbourhood of Europa, which is perhaps the most likely site for life in our Solar System after our own Earth.”

Daniel Waller, Vice-President at Teledyne e2v, said: “The launch of JUICE with the JANUS optical camera onboard marks a milestone in this important mission. This is our second complementary metal-oxide-semiconductor sensor from our facility in Chelmsford to fly in space in recent months.

“This sensor will give us sight of both the icy moons and the environment of Jupiter, increasing our understanding of other planets in our solar system.”

UK celebrates successful launch of James Webb Space Telescope

The once-in-a-generation James Webb Space Telescope launched on Christmas Day, with scientists and engineers across the UK playing a vital role in the mission.

The telescope, known as ‘Webb’, blasted off from the Arianespace spaceport in French Guiana on 25 December 2021 at 12:20 pm – the culmination of decades of scientific collaboration.

The mission is led by NASA, the European Space Agency (ESA) and the Canadian Space Agency, with the UK playing a major role by leading the European consortium, which designed, built and tested one of the four main science instruments, working closely with partners in the US.

Science Minister George Freeman said: “Today is a monumental milestone for international and UK space science: the Webb Space Telescope will allow us to go further and deeper to explore and discover our planetary universe.

“The project draws heavily on the world-class expertise of top UK scientists and engineers who were able to deliver vital pieces of this complex and powerful telescope.

“Being at the heart of this international project showcases the innovative talent of the UK’s world-leading scientists and engineers, and emphasises our position as a global science powerhouse.”

Seeing the Universe

The telescope is set to redefine our understanding of the cosmos and unveil some of the secrets of the distant Universe.

Webb will peer through dusty clouds in space to allow scientists to determine how the first galaxies were formed and will see our own solar system in whole new ways and in never-before-seen detail.

Scientists and engineers in the UK were crucial to the development and launch of the Mid-Infrared Instrument (MIRI), which will be able to see the faint light from the most distant stars, effectively looking further back in time than ever before, and to peer through dust and gas to spot stars being born.

JWST’s Mid Infrared Instrument (MIRI), for which the UK leads the European Consortium. Credit: STFC RAL Space

The MIRI development has been funded by the UK Space Agency and the Science and Technology Facilities Council, part of UK Research and Innovation, and ESA.

Caroline Harper, Head of Space Science at the UK Space Agency, said: “Webb is set to re-write the text books on astronomy, showing us things about the universe we have never been able to see before.  I am excited to see the fascinating discoveries the spacecraft makes as it reveals the evolution of the universe.

“The UK has played a crucial role in this once-in-a-generation mission, developing the Mid-Infrared Instrument, which will examine the physical and chemical properties of objects in the early universe in greater detail than ever.

“This has been a fantastic example of academic-industry partnership, showcasing the skills and expertise of our scientists and engineers.”

Webb in the UK

MIRI will deliver a host of capabilities, boasting a spectrograph to break up light into its constituent wavelengths, a coronagraph to block starlight and look at fainter objects next to stars, and a camera to take pictures.

MIRI was designed, built, and tested by a European Consortium of 10 member countries led by the UK, in partnership with the US. The European contribution is led by Professor Gillian Wright MBE of STFC’s UK Astronomy Technology Centre (UKATC), and includes STFC RAL Space, University of Leicester, and Airbus UK.

The UK’s lead role in the instrument involves taking responsibility for the overall design, science performance, and the mechanical, thermal and optical design, along with the assembly, integration, testing and calibration software.

The UK (UK Space Agency since 2011 and STFC) has invested almost £20 million in the development phase of MIRI and has continued to support essential post-delivery testing, integration, calibration and characterisation activities by the UK MIRI team.

Intégration EPC au BIL, le 06/11/2021. | EPC integration at BIL. 11/06/2021.

Professor Gillian Wright, European Principal Investigator for MIRI and Director of UKATC, said: “To see Webb launch, with MIRI on board, after more than two decades is a seminal moment.

“MIRI is a special instrument, for the breadth of its science, the team that built it, and being the coolest instrument on Webb. The MIRI team rose to the challenges and brought some exquisite engineering solutions to make it a reality.

“The Webb mission as a whole is an amazing technological breakthrough in scale and complexity, and this extends to the instruments, including MIRI.   With the launch, all of us are excitedly anticipating the first MIRI data and the new view of the universe we will have.”

What’s next for Webb

Credit: NASA

Although Webb has successfully launched, its journey is only just beginning.

The giant mirror for the telescope had to be launched as 18 segments folded inside the launch vehicle and it must be unfolded, and all the segments perfectly aligned, in space. A huge sunshield the size of a tennis court is needed to keep the instruments cold enough to work and this must also be unfurled in space.

Webb will then go on a month-long journey to its destination, a million miles from Earth.

In the six months after launch, the observatory commissioning will take place – with first results expected in the summer of 2022.

NASA’s Perseverance: seeking life on Mars

Less than a day after NASA’s Mars 2020 Perseverance rover successfully landed on the surface of Mars, engineers and scientists at the agency’s Jet Propulsion Laboratory in Southern California were hard at work, awaiting the next transmissions from Perseverance.

As data gradually came in, relayed by several spacecraft orbiting the Red Planet, the Perseverance team were relieved to see the rover’s health reports, which showed everything appeared to be working as expected.

Adding to the excitement was a high-resolution image taken during the rover’s landing. While NASA’s Mars Curiosity rover sent back a stop-motion movie of its descent, Perseverance’s cameras are intended to capture video of its touchdown and this new still image was taken from that footage, which is still being relayed to Earth and processed.

Unlike with past rovers, the majority of Perseverance’s cameras capture images in color. After landing, two of the Hazard Cameras (Hazcams) captured views from the front and rear of the rover, showing one of its wheels in the Martian dirt (above).

Perseverance got a close-up from NASA’s eye in the sky, as well: NASA’s Mars Reconnaissance. Orbiter, which used a special high-resolution camera to capture the spacecraft sailing into Jezero Crater, with its parachute trailing behind. The High Resolution Camera Experiment (HiRISE) camera did the same for Curiosity in 2012. JPL leads the orbiter’s mission, while the HiRISE instrument is led by the University of Arizona.

Several pyrotechnic charges are expected to fire later on Friday, releasing Perseverance’s mast (the “head” of the rover) from where it is fixed on the rover’s deck.

The Navigation Cameras (Navcams), which are used for driving, share space on the mast with two science cameras: the zoomable Mastcam-Z and a laser instrument called SuperCam. The mast is scheduled to be raised Saturday, Feb. 20, after which the Navcams are expected to take panoramas of the rover’s deck and its surroundings.

In the days to come, engineers will pore over the rover’s system data, updating its software and beginning to test its various instruments.

In the following weeks, Perseverance will test its robotic arm and take its first, short drive. It will be at least one or two months until Perseverance will find a flat location to drop off Ingenuity, the mini-helicopter attached to the rover’s belly, and even longer before it finally hits the road, beginning its science mission and searching for its first sample of Martian rock and sediment.

More About the Mission

A primary objective for Perseverance’s mission on Mars is astrobiology research, including the search for signs of ancient microbial life. The rover will characterize the planet’s geology and past climate and be the first mission to collect and cache Martian rock and regolith, paving the way for human exploration of the Red Planet.

Subsequent NASA missions, in cooperation with ESA (European Space Agency), will send spacecraft to Mars to collect these cached samples from the surface and return them to Earth for in-depth analysis.

The Mars 2020 Perseverance mission is part of NASA’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.

JPL, a division of Caltech in Pasadena, California, manages the Mars 2020 Perseverance mission and the Ingenuity Mars Helicopter technology demonstration for NASA.

For more about Perseverance, go to:

https://mars.nasa.gov/mars2020/

and

https://nasa.gov/perseverance

Images: NASA

The song of Mars: sounds from The Red Planet

A UK instrument has captured the first sounds ever recorded directly from Mars.

The NASA InSight lander, which is supported by the UK Space Agency, has recorded a haunting, low rumble caused by vibrations from the wind. These vibrations were detected by an ultra-sensitive seismometer, developed in the UK, and an air pressure sensor sitting on the lander’s deck. Continue reading The song of Mars: sounds from The Red Planet

Next stop Mars: InSight to study earthquakes on the Red Planet

A new mission to Mars involving UK science will be the first to study the heart of the Red Planet and measure ‘Marsquakes’ from its surface. The NASA InSight mission, which stands for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, launched from California aboard a United Launch Alliance Atlas V rocket at 12.05pm (BST) yesterday (above). Continue reading Next stop Mars: InSight to study earthquakes on the Red Planet