Tag: Solar System

  • Juice fully integrated

    Juice fully integrated

    ESA’s Juice mission has entered its final phase of development, with the spacecraft moving to an @Airbus Defence and Space facility in Toulouse, France, for the next round of testing. The spacecraft has been fully integrated, and these tests will be done in full flight configuration, as Juice is scheduled for launch from Europe’s Spaceport in Kourou, French Guiana, in April 2023.

    The Juice mission is a perfect example of collaboration between several national space agencies and European industry. Its objective is to explore the gas giant Jupiter, its environment, and three of its moons: Europa, Callisto and Ganymede. By studying this planetary system, ESA hopes to learn more about the icy worlds around Jupiter and the origins and possibility of life in our Universe

    Learn more about Juice: https://bit.ly/JuiceESAScience

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  • Can you spot the solar hedgehog? 🦔 #shorts

    Can you spot the solar hedgehog? 🦔 #shorts

    Solar Orbiter is a space mission of international collaboration between ESA and @NASA.

    Solar Orbiter’s closest approach to the Sun, known as perihelion, took place on 26 March. The spacecraft was inside the orbit of Mercury, at about one-third the distance from the Sun to the Earth, and its heatshield was reaching around 500°C. But it dissipated that heat with its innovative technology to keep the spacecraft safe and functioning.

    Learn more: http://bit.ly/SolarOrbiterESA

    #SolarOrbiter
    #TheSunUpClose

  • Juice’s journey and Jupiter system tour

    Juice’s journey and Jupiter system tour

    ESA’s Jupiter Icy Moons Explorer, Juice, is set to embark on an eight-year cruise to Jupiter starting April 2023. The mission will investigate the emergence of habitable worlds around gas giants and the Jupiter system as an archetype for the numerous giant planets now known to orbit other stars.

    This animation depicts Juice’s journey to Jupiter and highlights from its foreseen tour of the giant planet and its large ocean-bearing moons. It depicts Juice’s journey from leaving Earth’s surface in a launch window 5–25 April 2023 and performing multiple gravity assist flybys in the inner Solar System, to arrival at Jupiter (July 2031), flybys of the Jovian moons Europa, Callisto and Ganymede, orbital insertion at Ganymede (December 2034), and eventual impact on this moon’s surface (late 2035).

    An Ariane 5 will lift Juice into space from Europe’s Spaceport in Kourou. A series of gravity assist flybys of Earth, the Earth-Moon system and Venus will set the spacecraft on course for its July 2031 arrival at Jupiter. These flybys are shown here in order – Earth-Moon (August 2024), Venus (August 2025), Earth (September 2026, January 2029) – interspersed by Juice’s continuing orbits around the Sun. Juice’s flyby of the Earth-Moon system, known as a Lunar-Earth gravity assist (LEGA), is a world first: by performing this manoeuvre – a gravity assist flyby of the Moon followed just 1.5 days later by one of Earth – Juice will save a significant amount of propellant on its journey.

    Juice will start its science mission about six months prior to entering orbit around Jupiter, making observations as it approaches its destination. Once in the Jovian system, a gravity assist flyby of Jupiter’s largest moon Ganymede – also the largest moon in the Solar System – will help Juice enter orbit around Jupiter, where the spacecraft will spend four years observing the gas giant and three of its moons: Ganymede, Callisto and Europa.

    Juice will make two flybys of Europa (July 2032), which has strong evidence for an ocean of liquid water under its icy shell. Juice will look at the moon’s active zones, its surface composition and geology, search for pockets of liquid water under the surface, and study the plasma environment around Europa, also exploring the moon’s tiny atmosphere and hunting for plumes of water vapour (as have been previously detected erupting to space).

    A sequence of Callisto flybys will be used to study this ancient, cratered world that may too harbour a subsurface ocean, also changing the angle of Juice’s orbit with respect to Jupiter’s equator, making it possible to explore Jupiter’s higher latitudes (2032–2034).

    A sequence of Ganymede and Callisto flybys will adjust Juice’s orbit – properly orienting it while minimising the amount of propellant expended – so that it can enter orbit around Ganymede in December 2034, making it the first spacecraft to orbit another planet’s moon. Juice’s initial elliptical orbit will be followed by a 5000 km-altitude circular orbit, and later a 500 km-altitude circular orbit.

    Ganymede is the only moon in the Solar System to have a magnetosphere. Juice will investigate this phenomenon and the moon’s internal magnetic field, and explore how its plasma environment interacts with that of Jupiter. Juice will also study Ganymede’s atmosphere, surface, subsurface, interior and internal ocean, investigating the moon as not only a planetary object but also a possible habitat.

    Over time, Juice’s orbit around Ganymede will naturally decay due to lack of propellant, and it will make a grazing impact onto the surface (late 2035).

    The Juice launch itself will be a historical milestone for more reasons than one. It will be the final launch for Ariane 5, ending the launcher’s nearly three-decade run as one of the world’s most successful heavy-lift rockets. Its duties are being taken over by Ariane 6.

    Learn more about Juice: https://bit.ly/JuiceESAScience

    Credit: ESA/Lightcurve Films/R. Andres

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  • Artemis: crawling towards launch

    Artemis: crawling towards launch

    One of the many milestones in the leadup to the launch of Artemis is its rollout: this is when a crawler will carry the SLS rocket with Orion and ESM from the Vehicle Assembly Building to launchpad 39B. @NASA’s John Giles gives us a tour of the crawler and explains the adaptations made to this “wonderful piece of machinery” since it was first built for the Apollo programme in the 1960s. ESA is playing a key role in NASA’s Artemis programme, which will bring astronauts back to the Moon. The European Service Module – or ESM – will provide propulsion, power and thermal control for the Orion spacecraft.

    Learn more: https://bit.ly/Artemis1ESA

    Video credits: European Space Agency
    Thumbnail image credits: NASA/Leif Heimbold

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  • European push to the Moon

    European push to the Moon

    The European Space Agency is playing a vital role in humankind’s return to the Moon. In a few months @NASA will launch Artemis I from the Kennedy Space Center. The uncrewed mission will carry NASA’s Orion spacecraft incorporating ESA’s European Service Module (ESM-1), built and tested by Airbus Bremen, in Germany, with the help of 10 European nations. ESM-1’s main engine and 32 thrusters will propel Orion into orbit around the Moon and return it to Earth.

    As Artemis I prepares for launch, the second European Service Module (ESM-2) is about to ship to the US with ESM-3 also currently under construction. The second Artemis mission, however, has a crucial difference: it will carry four astronauts for a lunar flyby. ESM-2 will provide propulsion, power, oxygen, water and life support as well as controlling the temperature in the orbiting crew module. ESM-3 will go one step further and put the first person on the Moon for 50 years.

    Learn more about Orion: https://bit.ly/ESAsOrion

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    We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.

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  • Earth views from space – 1 hour long in 4K!

    Earth views from space – 1 hour long in 4K!

    Watch over one hour of our planet, seen from the International Space Station, in 4K resolution. This compilation was made from video taken by ESA astronauts, mostly by Thomas Pesquet during his first mission, Proxima, and ESA astronaut Alexander Gerst on his second mission, Horizons, as well as footage from Samantha Cristoforetti’s Futura mission and Paolo Nespoli’s Vita mission.

    Flying 400 km above our amazing planet Earth, the Space Station travels at 28 800 km/h to stay in orbit. The videos are in real time and not sped up or edited. Most of the scenes were filmed in the European-built Cupola module, the Space Station’s observatory.

    On 21 April 2001, the first ESA astronaut Umberto Guidoni arrived at the Space Station. Since then, the Space Station has grown immensely, as have the number of Europeans to have worked in it, together with the science experiments performed in orbit.

    Europe contributes around 8% of the running costs of the International Space Station, but has built a large part of the structure, including ESA’s Columbus laboratory, the Cupola observatory, the Tranquillity and Harmony modules, as well as the computers that collect data and provide navigation, communications and operations for the Russian segment.

    ESA also provided the Space Station with supplies and boosted its orbit through five Automated Transfer Vehicles, the heaviest and most versatile Space Station supply ferry. This programme evolved into the European Service Modules that ESA is supplying for @NASA’s Artemis programme, taking humans forward to the Moon and thus continuing the exemplary international collaboration beyond Earth’s orbit.

    Since Umberto’s mission, there have been 26 further ESA astronaut missions to the International Space Station, with astronauts flying to Station on either the Russian Soyuz or US Space Shuttle spacecraft.

    Thomas Pesquet’s second mission, Alpha, is the 28th mission for ESA, with ESA astronaut Matthias Maurer already lined up for his first flight later this year, and ESA astronaut Samantha Cristoforetti scheduled for the 30th ESA International Space Station mission in 2022.

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  • Drop tests for touchdown on Mars

    Drop tests for touchdown on Mars

    The ExoMars team have performed important parachute drop tests as crucial preparation for a safe touchdown on Mars in 2023. The European Rosalind Franklin rover will search for signs of past life beneath the surface of Mars with its unique two metre drill and onboard laboratory. The Russian surface science platform Kazachok will study the environment at the landing site. Landing on Mars is always a challenging endeavour and all possible parameters are taken into account.

    More information on ExoMars: http://www.esa.int/exomars

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  • Sound of a close Venus flyby #shorts

    Sound of a close Venus flyby #shorts

    A sonification of data recorded by the Italian Spring Accelerometer (ISA) aboard the BepiColombo Mercury Planetary Orbiter spacecraft during the flyby of Venus on 10 August 2021. The accelerometer data was converted to frequency to be made audible to the human ear. The resulting sound is rich with interesting effects due to the planet’s gravity acting on the spacecraft structure, the response of the spacecraft to the rapid temperature changes, and the change in reaction wheel velocity as they work hard to compensate for these effects.

    The audio has been matched to the timing that the images seen in this movie were captured, in the moments after closest approach.

    Read more: https://www.esa.int/Science_Exploration/Space_Science/Sights_and_sounds_of_a_Venus_flyby

    Credit:
    Images: ESA/BepiColombo/MTM, CC BY-SA 3.0 IGO
    Audio: ESA/BepiColombo/ISA/ASI-INAF, CC BY-SA 3.0 IGO

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  • BepiColombo’s close Venus encounter

    BepiColombo’s close Venus encounter

    A stunning sequence of 89 images taken by the monitoring cameras on board the European-Japanese BepiColombo mission to Mercury, as the spacecraft made a close approach of Venus on 10 August 2021.

    The sequence includes images from all three Monitoring Cameras (MCAM) onboard the Mercury Transfer Module, which provides black-and-white snapshots in 1024 x 1024 pixel resolution. It is not possible to image with the high-resolution camera suite during the cruise phase. The images have been lightly processed to enhance contrast and use the full dynamic range. A small amount of optical vignetting is seen in the corners of some of the images.

    The first image is from MCAM 1, and was taken at 13:41:02 UTC, prior to close approach. As such, the spacecraft was still on the nightside of the planet, but the dayside can just be seen creeping into view. Part of the spacecraft’s solar array can also be seen.

    The second image was taken by MCAM 2 at 13:51:56 UTC, two seconds after closest approach. With the Venus surface just 552 km away, the planet fills the entire field of view. The camera is not able to image detail of the planet’s atmosphere. The image also captures the Mercury Planetary Orbiter’s medium gain antenna and magnetometer boom.

    The rest of the sequence is from MCAM 3, while the spacecraft was pointed at Venus, and then as it slews away and gradually recedes from view, covering the time period 13:53:56 UTC on 10 August until 12:21:26 UTC on 11 August. The high gain antenna of the Mercury Planetary Orbiter is also seen changing orientation as it points towards Earth.

    The music accompanying the compilation was composed especially for the occasion, by @Anna Phoebe.

    The images were captured during the second of two Venus flybys, and the third of nine flybys overall. The flybys are gravity assist manoeuvres needed to help steer the spacecraft on course for Mercury. During its seven-year cruise to the smallest and innermost planet of the Solar System, BepiColombo makes one flyby at Earth, two at Venus and six at Mercury in order to approach the orbit around Mercury. Its first Mercury flyby will take place 1-2 October 2021 from a distance of just 200 km.

    BepiColombo, which comprises ESA’s Mercury Planetary Orbiter and the Mercury Magnetospheric Orbiter of @JAXA | 宇宙航空研究開発機構, is scheduled to reach its target orbit around the smallest and innermost planet of the Solar System in 2025. The spacecraft will separate and enter into their respective orbits before starting their science mission in early 2026 .

    Credit: ESA/BepiColombo/MTM, CC BY-SA 3.0 IGO

    Music composed by Anna Phoebe, with additional soundscapes by Mark McCaughrean

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  • Exoplanet Types: Worlds Beyond Our Solar System

    Exoplanet Types: Worlds Beyond Our Solar System

    When we describe different types of exoplanets – planets outside our solar system – what do we mean by “hot Jupiters,” “warm Neptunes,” and “super-Earths”? Since we’re still surveying and learning about the variety of worlds out there among the stars, it’s sometimes helpful to refer to characteristics they share with planets we’re familiar with in our own planetary system.

    Credit: NASA/JPL-Caltech

  • What Is an Exoplanet?

    What Is an Exoplanet?

    Exoplanets – planets outside our solar system – are everywhere. But why do we study them? What makes them so interesting? At NASA, we’re surveying and studying exoplanets to learn all about their weirdness, their variety, and all the fascinating things they can tell us about how planets form and develop.

    Credit: NASA/JPL-Caltech

  • See the European Service Modules taking humankind forward to the Moon

    See the European Service Modules taking humankind forward to the Moon

    From the @Airbus integration halls in Bremen, Germany, this replay of a live event shows a sneak peek of the two European Service Modules that will power astronauts to the Moon and back as part of @NASA’s Orion spacecraft.

    Orion is NASA’s next exploration spacecraft to send astronauts farther into space than ever before, beyond the Moon to asteroids and even Mars.

    ESA has contracted and is overseeing the development of the European Service Module, the part of the Orion spacecraft that provides air, electricity and propulsion. Much like a train engine pulls passenger carriages and supplies power, the European Service Module will power the Orion crew module to its destination and back to Earth.

    The programme includes Andreas Hammer, Head of @Airbus Defence and Space Exploration showing the European Service Modules in production, ESA Director General Jan Wörner announcing future developments, a statement by ESA’s head of European Service Module programme Philippe Deloo, a statement by Airbus head of European Service Module programme Didier Radola, a Moon missions overview with ESA astronaut Alexander Gerst and ESA’s head of Space Transportation Nico Dettmann on how ESA is building Orion with industry.

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  • Artemis I – European Service Module perspective

    Artemis I – European Service Module perspective

    The Orion spacecraft with European Service Module will fly farther from Earth than any human-rated vehicle has ever flown before. This video gives an overview of the first mission – without astronauts – for Artemis, focussing on ESA’s European Service Module that powers the spacecraft.

    The spacecraft will perform a flyby of the Moon, using lunar gravity to gain speed and propel itself 70 000 km beyond the Moon, almost half a million km from Earth – further than any human has ever travelled.

    On its return journey, Orion will do another flyby of the Moon before heading back to Earth.
    The total trip will take around 20 days, ending with a splashdown in the Pacific Ocean without the European Service Module – it separates and burns up harmlessly in the atmosphere.

    The second Artemis mission will have a similar flight plan but with astronauts. The third Artemis mission will see astronauts taken to the lunar surface.

    The European Service Module is ESA’s contribution to NASA’s Orion spacecraft that will send astronauts to the Moon and beyond. It provides electricity, water, oxygen and nitrogen as well as keeping the spacecraft at the right temperature and on course.

    The European Service Module has 33 thrusters, 11 km of electrical wiring, four propellant and two pressure tanks that all work together to supply propulsion and everything needed to keep astronauts alive far from Earth – there is no room for error.

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  • Meet the Experts: Designing space missions

    Meet the Experts: Designing space missions

    Space missions are complex and require input from many specialists. The Concurrent Design Facility (CDF) is where most of ESA missions are conceived and conceptually designed. In this episode of Meet the Experts, Massimo Bandecchi, the founding father of ESA’s CDF, explains Concurrent Design (CD) and some of the missions studied using this methodology.

    Find more episodes in the series: https://www.esa.int/Education/Expedition_Home/12_-_18_years_old

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  • Comets | Meet the experts

    Comets | Meet the experts

    Comets are small objects of loosely packed ice and dust. Sometimes oddly shaped, they can tell us much about the formation of our Solar System. Cometary scientist Charlotte Götz discusses comets, their formation and their study in this week’s episode of Meet the Experts.

    Find more episodes in the series here: https://www.esa.int/Education/Expedition_Home/12_-_18_years_old

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  • 13 things you need to know about space

    13 things you need to know about space

    Here at ESA, the European Space Agency, space is our business. It’s a place we explore, heading outwards while also looking back, to improve life on our own blue planet. Why go out there? Because space is useful and valuable; because it’s the place we all live. That’s why ESA does what we do: because Earth is only the start. Here’s what you need to know about the stuff that surrounds us.

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    We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related.

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  • #EZScience: Preparing to Launch the Perseverance Rover to Mars

    #EZScience: Preparing to Launch the Perseverance Rover to Mars

    In this “On the Go” episode of #EZScience, we’re on the scene at Kennedy Space Center with the rocket that will take the Perseverance rover and the Ingenuity helicopter to Mars.

    ABOUT THE SERIES: In our #EZScience video series with the National Air and Space Museum, NASA’s associate administrator for science Dr. Thomas Zurbuchen and Museum director Dr. Ellen Stofan talk about the latest in planetary science and exploration.

    Learn more about the series: https://www.nasa.gov/ezscience

  • Flight over the Mars 2020 Perseverance rover landing site

    Flight over the Mars 2020 Perseverance rover landing site

    This video shows Jezero crater, the landing site of the @NASA Mars 2020 Perseverance rover on the Red Planet, based on images from ESA’s Mars Express mission. The planned landing area is marked with an orange ellipse.

    Scheduled for launch from Cape Canaveral, Florida on 30 July 2020 on board an Atlas V rocket, the Perseverance rover will land on 18 February 2021 in Jezero crater.

    An impact crater with a diameter of about 45 km, Jezero is located at the rim of the giant Isidis impact basin. Morphological evidence suggests that the crater once hosted a lake, some 3.5 billion years ago.

    Jezero possesses an inlet- and an outlet channel. The inlet channel discharges into a fan-delta deposit, containing water-rich minerals such as smectite clays. Scientists believe that the lake was relatively long lived because the delta may have required 1 to 10 million years to reach its thickness and size. Other studies conclude that the lake did not experience periods of important water-level fluctuations and that it was formed by a continuous surface runoff. This makes Jezero crater to a prime target for the search for potential signs of microbial life, because organic molecules are very well preserved in river deltas and lake sediments.

    A recent study of the ancient lakeshores, diverse minerals and violent volcanism of Jezero crater based on data from ESA’s Mars Express mission is available here: https://bit.ly/MarsExpressHelpsUncoverTheSecretsOfPerseveranceLandingSite

    The animation was created using an image mosaic made from four single orbit observations obtained by the High Resolution Stereo Camera (HRSC) on Mars Express between 2004 and 2008. The mosaic combines data from the HRSC nadir and colour channels; the nadir channel is aligned perpendicular to the surface of Mars, as if looking straight down at the surface. The mosaic image was then combined with topography information from the stereo channels of HRSC to generate a three-dimensional landscape, which was then recorded from different perspectives, as with a movie camera, to render the flight shown in the video.

    Copyright:
    Animation: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO
    Music: Björn Schreiner
    Soundtrack logo: Alicia Neesemann

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  • From Comet NEOWISE to Comet Interceptor

    From Comet NEOWISE to Comet Interceptor

    Discovered in March 2020, Comet NEOWISE became visible to the naked eye in July, gifting observers in the northern hemisphere with one of the most scenic comets in over 20 years. The comet, which is on an almost parabolic orbit and had its closest approach to the Sun, or perihelion, in early July, reaches its closest point to Earth on 22–23 July, before zipping back towards the outer Solar System.

    In this video, ESA Research Fellows Rachana Bhatawdekar and Sandor Kruk share their experience and explain how to observe and image the comet in the sky. Next, ESA Research Fellow Charlotte Götz tells us more about comets and their tails, and how ESA’s future Comet Interceptor mission, to be launched in 2028, is going to wait for such a ‘great’ comet that has not been discovered yet. The spacecraft will sit in a parking orbit around the Lagrange point L2, 1.5 million kilometres away from Earth, until an interesting ‘pristine’ comet visits the inner Solar System. It will then intersect the comet’s orbit to study its nucleus, gases, dust, and plasma environment.

    Jump to the different segments of the video:
    00:00 – 1:22 – How to see comet NEOWISE
    1:23 – 2:42 – How to take a picture of comet NEOWISE
    2:43 – 6:17 – Comets and Comet Interceptor

    More about Comet Interceptor https://bit.ly/ESAsMissionToInterceptAComet

    Image credits: Rachana Bhatawdekar, Sandor Kruk, Mark McCaughrean, Kai Noeske (2020)
    Thumbnail image: Courtesy Mark McCaughrean, 12 July 2020 (Wassenaar, The Netherlands)

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  • Solar Orbiter first images revealed

    Solar Orbiter first images revealed

    ESA’s Solar Orbiter spacecraft has sent back its first images of the Sun. At 77 million kilometres from the surface, this is the closest a camera has ever flown to our nearest star. The pictures reveal features on the Sun’s exterior that have never been seen in detail before.

    Launched on 10 February 2020, the spacecraft completed its commissioning phase and first close-approach to the Sun in mid-June. Since then, science teams have been processing and examining this early data.

    The spacecraft is currently in its cruise phase, on its way to Venus, but will eventually get even closer to the Sun.

    Learn more: https://bit.ly/SolarOrbitersFirstImages

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  • Solar Orbiter sees ‘campfires’ on the Sun

    Solar Orbiter sees ‘campfires’ on the Sun

    The first images from ESA’s Solar Orbiter, captured around the spacecraft’s first close pass of the Sun, some 77 million kilometres from its surface, are already exceeding expectations revealing interesting new phenomena on our parent star.

    This animation shows a series of close-up views captured by the Extreme Ultraviolet Imager (EUI) at wavelengths of 17 nanometers, showing the upper atmosphere of the Sun, or corona, with a temperature of around 1 million degrees.

    These images reveal a multitude of small flaring loops, erupting bright spots and dark, moving fibrils. A ubiquitous feature of the solar surface, uncovered for the first time by these images, have been called ‘campfires’. They are omnipresent minuature eruptions that could be contributing to the high temperatures of the solar corona and the origin of the solar wind.

    Captured on 30 May 2020, when Solar Orbiter was roughly halfway between the Earth and the Sun, these are the closest views of the Sun ever taken, allowing EUI to see features in the solar corona of only 400 km across. As the mission continues, Solar Orbiter will go closer to the Sun and this will increase the instrument’s resolving power by a factor of two at closest approach.

    The colour on this image has been artificially added because the original wavelength detected by the instrument is invisible to the human eye.

    The circle in the lower left corner indicates the size of Earth for scale.

    The extended grey shape visible at times moving across the field (00:00-00:25; 01:00-01:28; 01:50-02:00; 02:52-03:27) is not a solar feature but is caused by a sensor artefact.

    Solar Orbiter is a space mission of international collaboration between ESA and NASA.

    Learn more: https://bit.ly/SolarOrbitersFirstImages

    Credit: Solar Orbiter/EUI Team (ESA & NASA); CSL, IAS, MPS, PMOD/WRC, ROB, UCL/MSSL

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  • Closer than ever: Solar Orbiter’s first views of the Sun

    Closer than ever: Solar Orbiter’s first views of the Sun

    The first images from ESA’s Solar Orbiter are already exceeding expectations and revealing interesting new phenomena on the Sun.

    This animation combines a series of views captured with several remote-sensing instruments on Solar Orbiter between 30 May and 21 June 2020, when the spacecraft was roughly halfway between the Earth and the Sun ¬– closer to the Sun than any other solar telescope has ever been before.

    The red and yellow images were taken with the Extreme Ultraviolet Imager (EUI) in the extreme ultraviolet region of the electromagnetic spectrum, at wavelengths of 30 and 17 nanometers, respectively.

    The close-up views by EUI show the upper atmosphere of the Sun, or corona, with a temperature of around 1 million degrees. With the power to see features in the solar corona of only 400 km across, these images reveal a multitude of small flaring loops, erupting bright spots and dark, moving fibrils. A ubiquitous feature of the solar surface, uncovered for the first time by these images, have been called ‘campfires’. They are omnipresent minuature eruptions that could be contributing to the high temperatures of the solar corona and the origin of the solar wind.

    The EUI images are followed by three views based on data from the Polarimetric and Helioseismic Imager (PHI) instrument. The blue and red view is a ‘tachogram’ of the Sun, showing the line of sight velocity of the Sun, with the blue side turning to us and the red side turning away. The following view is a magnetogram, or a map of magnetic propertied for the whole Sun, featuring a large magnetically active region in the lower right-hand quadrant of the Sun. The yellow-orange view is a visible light image and represents what we would see with the naked eye: there are no sunspots visible because the Sun is displaying only low levels of magnetic activity at the moment.

    On larger scales, the Metis coronograph blocks out the dazzling light from the solar surface, bringing the fainter corona into view. Metis observes the corona simultaneously in visible light (shown in green) and ultraviolet light (shown in red) for the first time with unprecedented temporal coverage and spatial resolution. These images reveal the two bright equatorial streamers and fainter polar regions that are characteristic of the solar corona during times of minimal magnetic activity.

    On even grander scales, the Heliospheric Imager (SoloHI) telescope takes images of the solar wind – the stream of charged particles constantly released by the Sun into outer space – by capturing the light scattered by electrons in the wind. The first-light image from SoloHI is shown at the end, as a mosaic of four separate images from the instrument’s four separate detectors. In this view, the Sun is located to the right of the frame, and its light is blocked by a series of baffles; the last baffle is in the field of view on the right-hand side and is illuminated by reflections from the solar array. The partial ellipse visible on the right is the zodiacal light, created by sunlight reflecting off the dust particles that are orbiting the Sun. The signal from the solar wind outflow is faint compared to the much brighter zodiacal light signal, but the SoloHI team has developed techniques to reveal it. Planet Mercury is also visible as a small bright dot near the lower edge of the upper left tile.

    Solar Orbiter is a space mission of international collaboration between ESA and NASA.

    Learn more: https://bit.ly/SolarOrbitersFirstImages

    Credit: Solar Orbiter/EUI Team; PHI Team; Metis Team; SoloHI Team /ESA & NASA

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  • We Persevere

    We Persevere

    NASA’s next Mars rover has a name – Perseverance. Like every exploration mission before, our rover is going to face challenges, and it’s going to make amazing discoveries. 

    The time at hand is hard. We have already surmounted many obstacles on our way to Red Planet, but as humans we will not give up. We will always persevere.

    Targeted for launch in July 2020, NASA’s Mars Perseverance rover will search for signs of habitable conditions on Mars in the ancient past and for signs of past microbial life itself.

    Learn more about the mission: https://mars.nasa.gov/mars2020/

    Produced by brother
    Directed by Theodore Melfi
    Narrated by Octavia Spencer

    Music Credit: RONE – MOTION III
    Composed and produced by Erwan Castex
    Arranged by Romain Allender
    Performed by Rone, Vanessa Wagner & Les siècles Orchestra
    iF3073 – ℗ & © 2018 InFiné
    Published by InFiné Éditions / Warner Chappell Music Publishing

  • Meet the NASA Psyche team who will map Psyche’s elemental composition

    Meet the NASA Psyche team who will map Psyche’s elemental composition

    Meet the team designing and building the Psyche mission’s gamma ray and neutron spectrometer. This instrument on the spacecraft will detect, measure, and map Psyche’s elemental composition. It is mounted on a 6-foot (2-meter) boom to distance the sensors from background radiation created by energetic particles interacting with the spacecraft and to provide an unobstructed field of view. The team is based at the Applied Physics Laboratory at Johns Hopkins University and is led by Principal Investigator David Lawrence. 

    Learn more: https://psyche.asu.edu/mission/instruments-science-investigations/

  • What You Need to Know About Astrobiology – The Search for Life in the Universe!

    What You Need to Know About Astrobiology – The Search for Life in the Universe!

    How did life begin on Earth? Does life exist beyond our home planet? How do we search for it?

    These are the really tough questions astrobiologists want to answer by studying life as we know it.

    Here’s what you need to know about our search for life in the cosmos: https://www.nasa.gov/content/the-search-for-life

  • “It can be done.” – an Earth Day message

    “It can be done.” – an Earth Day message

    In summer 2018, ESA joined with the musician Vangelis and the family of scientist Prof. Stephen Hawking to beam a message marking his passing to the nearest black hole. On 22 April 2020, Earth Day, we’re transmitting this poignant message to all of planet Earth – as a message of hope, to say that, by working together, we can overcome this crisis and others facing humankind.

    The message reads:

    “I am very aware of the preciousness of time. Seize the moment. Act now.

    “I have spent my life travelling across the Universe inside my mind. Through theoretical physics I have sought to answer some of the great questions but there are other challenges, other big questions which must be answered, and these will also need a new generation who are interested, engaged and with an understanding of science.

    “How will we feed an ever-growing population, provide clean water, generate renewable energy, prevent and cure disease and slow down global climate change?

    “I hope that science and technology will provide the answers to these questions, but it will take people, human beings with knowledge and understanding to implement the solution.

    “One of the great revelations of the space age has been a perspective that has given humanity on ourselves. When we see the Earth from space we see ourselves as a whole; we see the unity and not the divisions. It is such a simple image, with a compelling message: one planet, one human race.

    “We are here together, and we need to live together with tolerance and respect. We must become global citizens.

    “I have been enormously privileged through my work to be able to contribute to our understanding of the Universe. But it would be an empty Universe indeed, if it were not for the people I love and who love me.

    “We are all time travellers journeying together into the future. But let us work together to make that future a place we want to visit. Be brave, be determined, overcome the odds. It can be done.

    “It can be done.”

    Text and narration: Prof. Stephen Hawking (© The Estate of Stephen Hawking)

    Music: The Stephen Hawking Tribute by Vangelis (composed, arranged, produced and performed by Vangelis) 2018

    Images:
    ISS – ESA/NASA
    Sentinel images – contain modified Copernicus Sentinel data/ESA, CC BY-SA 3.0 IGO
    Stock footage – Pexels.com, Pixabay, Bedrijfsfilmspecialist.nl
    COVID-19 testing – ©Governor Tom Wolf/Wikimedia Commons, CC-BY 2.0
    Sentinel 2 animation – ©ESA/ATG Medialab
    Earthrise – NASA
    Rosetta Earth 2009 – ESA/Rosetta/MPS for OSIRIS team/M. McCaughrean
    BepiColombo launch – ©ESA/CNES/Arianespace
    Black hole – ©EHT Collaboration, CC BY 4.0
    LHA 120-N150 – ©ESA/Hubble, NASA, Digitized Sky Survey 2, CC BY 4.0, D. De Martin
    BepiColombo Earth flyby ©ESA/BepiColombo/MTM, CC BY-SA 3.0 IGO

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  • Zoom past Earth with BepiColombo in virtual reality simulation

    Zoom past Earth with BepiColombo in virtual reality simulation

    With a simple Google Cardboard-style virtual reality (VR) viewer, you can experience how it feels to be a spacecraft hurtling past Earth. This 360-degree VR simulation of a flyby manoeuvre performed by ESA’s Mercury-bound BepiColombo spacecraft takes you on a trip past Earth at the distance of only 12 700 km, closer than the orbit of Europe’s navigational satellites Galileo.

    The simulation displays the field of view of two of BepiColombo’s science instruments (MERTIS and PHEBUS) and two of its three MCAM selfie cameras during the gravity-assist flyby at Earth on 10 April 2020.

    The simulation was created using the SPICE software developed by NASA’s Jet Propulsion Laboratory and data generated by the European Space and Astronomy Centre (ESAC)in Spain.

    BepiColombo, a joint mission of ESA and the Japan Aerospace Exploration Agency (JAXA), is on a seven-year cruise to Mercury, the smallest and innermost planet of the Solar System. Launched in October 2018, BepiColombo follows an intricate trajectory that involves nine gravity-assist flyby manoeuvres. In addition to the flyby at Earth, BepiColombo will perform two flybys at Venus and six at Mercury, its target planet. The manoeuvres slow down the spacecraft as it needs to constantly brake against the gravitational pull of the Sun in order to be able to enter the correct orbit around Mercury in 2025, ahead of commencing science operations in early 2026.

    Credit: ESA SPICE Service/RHEA Group.

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  • Lagrange mission to provide solar warning

    Lagrange mission to provide solar warning

    Earth’s magnetic field protects life on Earth from the intense radiation and titanic amounts of energetic material our Sun blasts in every direction. However, astronauts and satellites in space, future explorers travelling to the Moon and Mars, and infrastructure on Earth such as power grids and communication systems remain vulnerable to these violent outbursts.

    For this reason, ESA is planning to send a satellite to monitor the ‘side’ of our Sun, from a gravitationally stable position known as the fifth Lagrange point. From here, the Lagrange satellite will detect potentially hazardous solar events before they come into view from Earth, giving us advance knowledge of their speed, direction and chance of impact.

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  • Solar Orbiter launch highlights

    Solar Orbiter launch highlights

    Highlights from the preparation and liftoff of ESA’s Sun-exploring mission Solar Orbiter.

    Solar Orbiter lofted to space aboard the US Atlas V 411 rocket from NASA’s spaceport in Cape Canaveral, Florida at 04:03 GMT (05:03 CET) on 10 February 2020.

    An ESA-led mission with strong NASA participation, Solar Orbiter carries a set of ten instruments for imaging the surface of the Sun and studying the environment in its vicinity. The spacecraft will travel around the Sun on an elliptical orbit that will take it as close as 42 million km away from the Sun’s surface, about a quarter of the distance between the Sun and Earth. The orbit will allow Solar Orbiter to see some of the never-before-imaged regions of the Sun, including the poles, and shed new light on what gives rise to solar wind, which can affect infrastructure on Earth.

    More about Solar Orbiter: https://www.esa.int/solarorbiter

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  • Solar Orbiter liftoff

    Solar Orbiter liftoff

    ESA’s new Sun-exploring mission Solar Orbiter lofted to space aboard the US Atlas V 411 rocket from NASA’s spaceport in Cape Canaveral, Florida at 04:03 GMT (05:03 CET) on 10 February 2020.

    Solar Orbiter, an ESA-led mission with strong NASA participation, carries a set of ten instruments for imaging the surface of the Sun and studying the environment in its vicinity. The spacecraft will travel around the Sun on an elliptical orbit that will take it as close as 42 million km away from the Sun’s surface, about a quarter of the distance between the Sun and Earth. The orbit will allow Solar Orbiter to see some of the never-before-imaged regions of the Sun, including the poles, and shed new light on what gives rise to solar wind, which can affect infrastructure on Earth.

    More about Solar Orbiter: https://www.esa.int/solarorbiter

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  • Solar Orbiter launch preparations

    Solar Orbiter launch preparations

    ESA’s Solar Orbiter satellite in a cleanroom at the Astrotech payload processing facility near Kennedy Space Centre, Florida. The spacecraft is seen being mounted onto the payload adaptor ring and encapsulated into a fairing, which will protect the satellite and the rocket upper stage during the turbulent ascent through Earth’s atmosphere.

    Learn more about Solar Orbiter: http://bit.ly/ESASolarOrbiter

    The video was created with support from Airbus/Astrotech/ULA/NASA

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  • ESA’s missions to the Sun

    ESA’s missions to the Sun

    ESA’s new Sun-explorer, Solar Orbiter, will capture close-up images of never before seen regions of our parent star, including the poles, and study the electromagnetic environment in its vicinity. The cutting-edge spacecraft will get as close as 42 million kilometres away from the Sun, about a quarter of the distance between the Sun and Earth, and face scorching temperatures of up to 500°C.

    ESA has a long history of studying the Sun from space. Since the launch of Ulysses in 1990, the agency has led or cooperated on several Sun-exploring missions including SOHO, the Cluster quartet and Proba-2.

    Learn more about the Sun: http://bit.ly/LivingWithAStar

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  • Solar Orbiter operations simulations

    Solar Orbiter operations simulations

    ESA’s Solar Orbiter is getting ready for its launch on an Atlas V rocket provided by NASA and operated by United Launch Alliance from Cape Canaveral, Florida.

    Once in space, and over the course of several years, the spacecraft will repeatedly use the gravity of Venus and Earth to raise its orbit above the poles of the Sun, providing new perspectives on our star, including the first images of the Sun’s polar regions.

    All these operations will be controlled from the European Space Operations Centre (ESOC), Germany, where a dedicated team is currently working on simulations of the first moments in orbit, after separation from the launcher, but also all the delicate manoeuvres of the journey that will make Solar Orbiter mission possible.

    Learn more Solar Orbiter: http://bit.ly/ESASolarOrbiter

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  • Solar Orbiter – the Sun close-up

    Solar Orbiter – the Sun close-up

    ESA’s mission to the Sun, Solar Orbiter, is due for launch on an Atlas V 411 from Cape Canaveral, Florida on 9 February 23:03 EST / 04:03 GMT / 05:03 CET on 10 Feb.
     
    Equipped with a suite of ten scientific instruments, Solar Orbiter will capture the first images of the Sun’s poles and make detailed observations of solar activity. Its specially designed heatshield is capable of enduring temperatures of more than 500ºC.

    Solar Orbiter is a space mission of international collaboration between ESA and NASA. The spacecraft has been developed by Airbus.

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  • Forward to the Moon with ESA

    Forward to the Moon with ESA

    The first flight of the Artemis programme, which will see humans return to the Moon, is scheduled to begin soon. The lunar spacecraft consists of NASA’s Orion crew module and the European Service Module, or ESM. Developed by ESA and building on technology from its Automated Transfer Vehicle (ATV), the ESM will provide propulsion, life support, environmental control and electrical power to Orion. The Artemis 1 spacecraft modules are undergoing thermal vacuum and electromagnetic interference tests in the world’s largest space simulation vacuum chamber at the Glenn Research Centre’s Plum Brook Station in Sandusky, Ohio, USA.

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  • Solar Orbiter

    Solar Orbiter

    Engineers have completed their testing of ESA’s Solar Orbiter spacecraft in preparation for launch early next year.

    Equipped with a suite of ten instruments, Solar Orbiter will capture the closest ever pictures of our star, the first images of its poles, and make detailed observations of solar activity. Its specially designed heatshield is capable of enduring temperatures of more than 500 degrees Celsius.

    Over the past year, Solar Orbiter has been undergoing a series of rigorous tests at the IABG test centre near Munich, Germany. The spacecraft is due to be packed into an Antonov cargo plane on 31 October for shipping to Florida. Launch on an Atlas 5 rocket from Cape Canaveral, is planned for February 2020.

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  • ExoMars progress update

    ExoMars progress update

    ExoMars 2020 has passed a number of milestones. The European carrier module was delivered in March. The European rover, which contains nine instruments, has been assembled by Airbus UK and is under environmental testing in Toulouse. It should be integrated with the spacecraft by the end of the year. The spacecraft is now in the Thales Alenia Space test facilities in Cannes to start the environmental and performance verification test campaign that will last until February 2020.

    However, there remain some important challenges ahead for the parachute system of the descent module. Recent balloon high-altitude drop tests were unsuccessful. As a result, the next and final two drop tests, scheduled between January and March 2020, must be fully successful otherwise the mission cannot launch in 2020.

    The joint ESA and Russian mission consists of four elements: a carrier module to propel the spacecraft to Mars, a descent module, a surface science platform and the Rosalind Franklin rover, which will use its drill up to depths of two meters to search for signs of life.

    More information on ExoMars: http://www.esa.int/exomars

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  • Latest from Rosetta

    Latest from Rosetta

    Three years after the Rosetta mission officially ended in 2016, scientists met at ESA’s ESTEC facility in The Netherlands to discuss the latest findings at the final Science Working Team (SWT) meeting.

    From the launch in 2004, to its arrival at comet 67P in 2014, Rosetta has been an emotional and inspiring mission. Its findings have furthered our understanding of comets and changed our perceptions of how the Solar System formed.

    The mission produced an enormous amount of data which will keep many scientists busy for years. The OSIRIS camera, for example, took 100 000 images. These are archived – with the analysis of images recently providing further insight into the comet’s activity.

    Rosetta’s legacy of cometary science and data is not just continuing to produce more work, however, it’s also inspiring the next generation of scientists. Some began working on Rosetta as students and are now taking their experience forward onto ESA’s future Comet Interceptor mission.

    Further insight into the comet’s activity: http://bit.ly/CometCollapsingCliffsAndBouncingBoulders

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  • This is ESA

    This is ESA

    ESA is the only space agency in the world that covers the whole range of space activities. We’re exploring our Solar System and unlocking the secrets of the Universe. We’re monitoring space and protecting our planetary environment. We’re making space accessible and developing the technologies for the future, and we’re also using space to benefit citizens and meet future challenges on Earth.

    In November 2019, European ministers in charge of space activities will gather at the Space19+ conference in Seville, Spain, to decide on ESA’s vision for the future of Europe in space. Space19+ will be an opportunity to direct Europe’s ‘next generation’ ambitions in space, and address the challenges facing not only the European space sector but also European society as a whole.

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  • Hera: Our planetary defence mission

    Hera: Our planetary defence mission

    Hera will show us things we’ve never seen before. Astrophysicist and Queen guitarist Brian May tells the story of our mission that would be humanity’s first-ever spacecraft to visit a double asteroid.

    The asteroid system – named Didymos – is typical of the thousands that pose an impact risk to our planet, and even the smaller of the two would be big enough to destroy an entire city if it were to collide with Earth.

    Hera will help us to find out if it would be possible to deflect such an asteroid on a collision course with Earth. The mission will revolutionise our understanding of asteroids and how to protect ourselves from them, and therefore could be crucial for saving our planet.

    First, NASA will crash its DART spacecraft into the smaller asteroid – known as Didymoon – before Hera comes in to map the resulting impact crater and measure the asteroid’s mass. Hera will carry two CubeSats on board, which will be able to fly much closer to the asteroid’s surface, carrying out crucial scientific studies, before touching down. Hera’s up-close observations will turn asteroid deflection into a well-understood planetary defence technique.

    The Hera mission will be presented to our Space19+ meeting this November, where Europe’s space ministers will take a final decision on flying the mission, as part of the Agency’s broader planetary defence initiatives that aim to protect European and world citizens.

    Learn more about Hera: http://bit.ly/ESAHera

    Copyright: ESA – Science Office

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