Jump to content

Recommended Posts

Posted
Crew-3_say_cheese_card_full.jpg Image:

ESA astronaut Matthias Maurer and his NASA crew mates Raja Chari, Thomas Marshburn and Kayla Barron are all smiles as they arrive at NASA’s Kennedy Space Center in Florida, USA on 26 October 2021.

Collectively, the astronauts make up Crew-3 and will travel to the International Space Station on the SpaceX Crew Dragon spacecraft “Endurance”. The first launch opportunity for Crew-3 is 07:21 CET (06:21 GMT, 02:21 EDT) Sunday 31 October 2021, with a backup date of 3 November. 

The Dragon will dock with the Space Station 22 hours after launch, allowing for a short overlap with the Crew-2 members who are due to depart the Station in the coming week.

With both Matthias and ESA astronaut and current Space Station Commander Thomas Pesquet on board, Europe will have two astronauts resident in space – a rare occurrence.  

The name of Matthias’s mission is “Cosmic Kiss”. This is Matthias’s first mission, and he will be the 600th human to fly to space.

Once in orbit, Matthias will spend around six months living and working in microgravity as he supports more than 35 European experiments and numerous international experiments on board.

Matthias is also certified to perform Extra Vehicular Activity (EVA) in both the Russian Orlan and American EMU spacesuits. He is expected to perform a Russian spacewalk during his mission as part of initial operations for the European Robotic Arm (ERA) that was launched to the Station in July 2021.  

Visit the Cosmic Kiss mission page for more information about Matthias’s mission.

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

  • Similar Topics

    • By NASA
      3 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      Ice cover ebbs and flows through the seasons in the Arctic (left) and the Antarctic (right). Overall, ice cover has declined since scientists started tracking it half a century ago. Download this visualization from NASA’s Scientific Visualization Studio: https://svs.gsfc.nasa.gov/5099Trent Schindler/NASA’s Scientific Visualization Studio Winter sea ice cover in the Arctic was the lowest it’s ever been at its annual peak on March 22, 2025, according to NASA and the National Snow and Ice Data Center (NSIDC) at the University of Colorado, Boulder. At 5.53 million square miles (14.33 million square kilometers), the maximum extent fell below the prior low of 5.56 million square miles (14.41 million square kilometers) in 2017. 
      In the dark and cold of winter, sea ice forms and spreads across Arctic seas. But in recent years, less new ice has been forming, and less multi-year ice has accumulated. This winter continued a downward trend scientists have observed over the past several decades. This year’s peak ice cover was 510,000 square miles (1.32 million square kilometers) below the average levels between 1981 and 2010. 
      In 2025, summer ice in the Antarctic retreated to 764,000 square miles (1.98 million square kilometers) on March 1, tying for the second lowest minimum extent ever recorded. That’s 30% below the 1.10 million square miles (2.84 million square kilometers) that was typical in the Antarctic prior to 2010. Sea ice extent is defined as the total area of the ocean with at least 15% ice concentration.
      The reduction in ice in both polar regions has led to another milestone — the total amount of sea ice on the planet reached an all-time low. Globally, ice coverage in mid-February of this year declined by more than a million square miles (2.5 million square kilometers) from the average before 2010. Altogether, Earth is missing an area of sea ice large enough to cover the entire continental United States east of the Mississippi. 
      “We’re going to come into this next summer season with less ice to begin with,” said Linette Boisvert, an ice scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “It doesn’t bode well for the future.”
      To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
      Observations since 1978 show that ice cover has declined at both poles, leading to a downward trend in the total ice cover over the entire planet. In February 2025, global ice fell to the smallest area ever recorded. Download this visualization from NASA's Scientific Visualization Studio: https://svs.gsfc.nasa.gov/5521Mark Subbaro/NASA's Scientific Visualization Studio Scientists primarily rely on satellites in the Defense Meteorological Satellite Program, which measure Earth’s radiation in the microwave range. This natural radiation is different for open water and for sea ice — with ice cover standing out brightly in microwave-based satellite images. Microwave scanners can also penetrate through cloud cover, allowing for daily global observations. The DMSP data are augmented with historical sources, including data collected between 1978 and 1985 with the Nimbus-7 satellite that was jointly operated by NASA and the National Oceanic and Atmospheric Administration. 
      “It’s not yet clear whether the Southern Hemisphere has entered a new norm with perennially low ice or if the Antarctic is in a passing phase that will revert to prior levels in the years to come,” said Walt Meier, an ice scientist with NSIDC.

      By James Riordon
      NASA’s Earth Science News Team

      Media contact: Elizabeth Vlock
      NASA Headquarters
      Share
      Details
      Last Updated Mar 27, 2025 LocationNASA Goddard Space Flight Center Related Terms
      Earth Earth's Vital Signs General Explore More
      1 min read Arctic Sea Ice Near Historic Low; Antarctic Ice Continues Decline
      This summer, Arctic sea ice decreased to a its minimum extent on September 11, 2024.…
      Article 6 months ago 1 min read Keeping PACE with the Oceans
      NASA can detect tiny organisms, phytoplankton, that affect the color of ocean from space, and…
      Article 9 months ago 1 min read Antarctic Sea Ice Hits Annual Minimum, Second Lowest On Record
      On February 20th, 2024, Antarctic sea ice officially reached its minimum extent for the year.
      Article 1 year ago Keep Exploring Discover More Topics From NASA
      Missions
      Humans in Space
      Climate Change
      Solar System

      View the full article
    • By NASA
      Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions The Solar System The Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets Asteroids, Comets & Meteors The Kuiper Belt The Oort Cloud 4 min read
      Sols 4277-4279: Getting Ready To Say Goodbye to the King!
      Left navigation camera image from Sol 4255, showing “Milestone Peak” on the left, the subject of an RMI in this plan NASA/JPL-Caltech Earth planning date: Friday, Aug. 16, 2024
      It’s time to move on from our “Kings Canyon” drill site, so today’s plan focused on our usual tidy up routine after a drill campaign. First we need to dump out any material in the drill chambers, in an action called “RAGE” – this sounds aggressive but stands for “Rotation to Agitate Granules for Expulsion,” so it’s more of a gentle turning than an angry shaking. This ensures that the drill chambers won’t spill later and we are ready for the next drill campaign – whenever we find a worthy target! Mastcam will document the entire process, and then image the drill bit that was used, making sure it is still in good condition.
      At that point, we are free to use the arm instruments again (no turret movements allowed while there is sample in the drill chamber). So our contact science focuses today on the drill tailings, the pile of ground up rock generated by the drill action. That pile has been sitting there for over two weeks, but luckily it’s not too windy right now and the pile remained more or less intact. MAHLI will image the drill hole and the tailings pile on the first afternoon, APXS will integrate on the tailings on the first night and then MAHLI will image the tailings again on the second day. This post-retract image is just to confirm that APXS did not hit the pile of loose drill fines. As APXS Science Planner today, I worked with RPs to pick out the spot we will focus on and to make sure that we are using the correct sequences to ensure safety of the instrument – but it’s always nice to confirm that we didn’t hit the pile!
      ChemCam has a suite of activities, from LIBS activities close to the rover, to “passive” (non destructive) activities and RMI images (which can be relatively near field or long distance). LIBS on the bedrock target “Marck Lake” will be used to compared with the nearby Kings Canyon target and assess homogeneity across the drill block, while the passive observation of “Red Slate Mountain” will examine a large light toned block about 10 metres away from the rover. ChemCam will also acquire a long distance RMI of loose blocks and boulders about 85 metres away, looking towards “Milestone Peak” (shown in the accompanying image).
      APXS will acquire an overnight “atmospheric” measurement, looking at levels of argon as part of an ongoing campaign. This is paired with ChemCam’s second passive measurement, this time of the sky. We also have monitoring of dust levels, with Mastcam taus of the atmosphere (which atmospheric scientist Alex Innanen talked about here), and a whole host of Navcam dust devil movies, and suprahorizon and zenith movies (which target different parts of the horizon). All of these … and DAN and REMS activities too – our environmental monitoring team is working hard as usual!
      ChemCam has spent the last two weeks or so getting LIBS and passive measurements on “Sam Mack Meadow” – an area of darker toned, sometimes broken up rocks just outside of the current workspace. In fact, ChemCam is getting LIBS on two further targets there in this plan: “Horse Creek Spire” and the somewhat nodular “Kearsarge Pinnacles.” Mastcam will image all of the LIBS targets too. There are some interesting textures here that APXS and MAHLI are keen to sample too, so our next drive is more of a bump to get close enough to allow contact science here too. We will still be able to gaze on the King (Canyon) for another while, so I guess it’s not really goodbye just yet!
      Written by Catherine O’Connell-Cooper, Planetary Geologist at University of New Brunswick
      Share








      Details
      Last Updated Aug 19, 2024 Related Terms
      Blogs Explore More
      2 min read Sols 4275-4276: A Familiar View


      Article


      5 days ago
      2 min read Sols 4273-4274: Prep Rally


      Article


      5 days ago
      2 min read Sols 4270-4272: Sample for SAM


      Article


      1 week ago
      Keep Exploring Discover More Topics From NASA
      Mars


      Mars is the fourth planet from the Sun, and the seventh largest. It’s the only planet we know of inhabited…


      All Mars Resources


      Explore this collection of Mars images, videos, resources, PDFs, and toolkits. Discover valuable content designed to inform, educate, and inspire,…


      Rover Basics


      Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a…


      Mars Exploration: Science Goals


      The key to understanding the past, present or future potential for life on Mars can be found in NASA’s four…

      View the full article
    • By USH
      Stanford Professor Garry Nolanhas been testing the brains of people who say they’ve experienced a UFO encounter as well as he analysis anomalous materials from UFO crashes. 

      Did the people who claimed that they'd had an encounter, especially the pilots, describe any perceivable decrease in neurological capacity? 
      Of the 100 or so patients that we looked at, about a quarter of them died from their injuries. The majority of these patients had symptomology that's basically identical to what's now called Havana syndrome. 
      But Dr. Nolan has also spent the past decade analyzing anomalous materials From UFO crashes 
      One of the materials from the so called Ubatuba event, a UFO event in Brazil, has extraordinarily altered isotope ratios of magnesium. 
      What that means is that if you find a metal where the isotope ratios are changed far beyond what is normally found in nature, then that material has likely been engineered, the material is downstream of a process that caused them to be altered. Someone did it. The questions are who… and why? 
      Speaking to Vice’s Motherboard, Nolan opened up about his work and revealed what sparked his interest in UAP. Learn more at: Vice Motherboard
        View the full article
  • Check out these Videos

×
×
  • Create New...