When it was formed, the young proto-Earth was hot and probably circled around the sun in a very dry zone where water evaporated and was blown into space by the solar wind. According to one theory, our blue planet came to its great oceans through watery celestial bodies that hit the earth. As spectral analyses of comet tails have shown, it was most likely not comets.
This is because in their ice, the ratio of hydrogen with two protons in its nucleus, deuterium (D), to hydrogen with one proton in its nucleus (H) is usually different from that on Earth. On the other hand, the water trapped in certain meteorites – i.e. in fragments of asteroids that have hit the Earth – is almost exactly the same as terrestrial water. Such C-class asteroids are highly carbonaceous and come from the outer part of the asteroid belt that orbits the sun between Mars and Jupiter. Ryugu is one of them.
Prof. Frank Brenker, geoscientist at Goethe University, will examine the Ryugu sample together with his colleague Dr. Beverly Tkalcec. He explains: “There are very good scientific arguments that the D/H ratio we find in meteorites is indeed similar to that of asteroids in space. Nevertheless, we cannot rule out water vapour contamination on Earth: after all, 90 percent of an asteroid evaporates when it passes through the atmosphere, and even if it hits a dry desert, the meteorite can absorb water until it is found, for example from early morning fog. With the Ryugu sample we will finally get certainty on this issue”.
To this end, from the middle of next year, the Frankfurt researchers will examine and screen Ryugu samples for their chemical composition at the particle accelerators ESRF in Grenoble and DESY in Hamburg. Later in the year, Ryugu samples will be cut with the help of a focused ion beam and will be examined with a transmission electron microscope at Goethe University. Tkalcec and Brenker want to determine the exact geological history of the asteroid. In order to be able to assess the measured values for the water, but also the organic compounds that occur, it is immensely important to understand all the processes that led to their formation in the first place. The temperature achieved by the asteroid is just as important here as the circumstances of the formation of water-containing minerals, and the influence of impacts on the surface of the asteroid.
The building blocks for life on Earth may also come from carbon-rich asteroids such as Ryugu, since sugars and components of proteins (amino acids) and the hereditary molecule DNA (nucleobases), which could have been formed from inorganic substances under suitable conditions, have already been found in meteorites. For this reason as well, numerous scientific teams from all over the world will be working on the analysis of the Ryugu samples.
Images for download:
- Prof. Dr. Frank Brenker, Institute für Geosciences, Goethe University Frankfurt. Credit: Jürgen Lecher for Goethe University. https://www.uni-frankfurt.de/95132289
- Prof. Dr. Frank Brenker, Institute für Geosciences, Goethe University Frankfurt. Credit: personal photo. https://www.uni-frankfurt.de/95132407
- Dr. Beverley Tkalcec, Institute für Geosciences, Goethe University Frankfurt. Credit: personal photo. https://www.uni-frankfurt.de/95132444
- Landing of space probe Hayabusa 2 on the asteroid Ryugu for the collection of samples. Illustration: Akihiro Ikeshita für JAXA. https://www.hayabusa2.jaxa.jp/en/galleries/cg/pages/touchdown1.html
- The asteroid Ryugu from a distance of 20 kilometres, photographed by the probe Hayabusa 2. Credit: JAXA, University of Tokyo, Kochi University, Rikkyo University, Nagoya University, Chiba Institute of Technology, Meiji University, University of Aizu and AIST.
- Hayabusa 2 passes by Earth: On its return, the probe flew past Earth on its way to another mission and sent a capsule containing the Ryugu sample to Earth. The capsule landed in the Australian desert on Saturday, 5 December 2020. Illustration: Akihiro Ikeshita for JAXA.
Prof. Dr. Frank Brenker
Institute for Geosciences – Nanoscience