SARA measurements of hydrogen flux on the Moon

Although Barabash and his colleagues do not know what is causing the Moon to act as a hydrogen mirror, the discovery paves the way for a new type of picture to be made of the lunar surface. This is because the hydrogen atoms shoot off with speeds of around 200 km/s and so escape without being deflected by the Moon’s weak gravity. Also, because hydrogen is electrically neutral it is not diverted by the magnetic fields in space. So the atoms fly in straight lines from the surface of the Moon, just like photons of light. In principle, each detection can be traced back to its origin and an image of the surface can be made. The areas that emit most hydrogen will show up the brightest.

Sub Kev Atom reflecting Analyser (SARA)

Barabash and his team are currently analysing the data to see if they can make such pictures, in order to look for so-called lunar magnetic anomalies. Whilst the Moon does not generate a global magnetic field, some lunar rocks are magnetised. These generate magnetic bubbles that deflect incoming protons away into surrounding regions. In a hydrogen image, the magnetic rocks will therefore appear dark.

The incoming protons are part of the solar wind, a constant stream of particles given off by the Sun. They collide with every celestial object in the Solar System but are usually stopped by the body’s atmosphere. On bodies without such a natural shield, for example asteroids or the planet Mercury, the solar wind reaches the ground. The SARA team expects that these objects too will reflect many of the incoming protons back into space as hydrogen atoms.

Artist's impression of Chandrayaan-1

This knowledge provides timely advice for the scientists and engineers who are readying ESA’s Bepi-Colombo mission to Mercury. The spacecraft will be carrying two similar instruments to SARA and may find that the inner-most planet is reflecting more hydrogen than the Moon because the solar wind is more concentrated closer to the Sun. In the meantime, the SARA team is combing the lunar data for insight, and puzzling over just why the Moon is so good at reflecting hydrogen.

Notes to Editors:

SARA was one of three instruments that ESA contributed to Chandrayaan-1, the lunar orbiter that finished its mission in August 2009. The instrument was built jointly by scientific groups from Sweden, India, Japan, and Switzerland: Swedish Institute of Space Physics, Kiruna, Sweden; Vikram Sarabhai Space Centre, Trivandrum, India; University of Bern, Switzerland; and Institute of Space and Astronautical Science, Sagamihara, Japan. The instrument is led by Principal Investigators Stanislav Barabash, IRF, Sweden, and Anil Bhardwaj, VSSC, India.

This article reflects findings presented in ‘Extremely high reflection of solar wind protons as neutral hydrogen atoms from regolith in space’, by M. Wieser, S. Barabash, Y. Futaana, M. Holmström, A. Bhardwaj, R. Sridharan, M.B. Dhanya, P. Wurz, A. Schaufelberger and K. Asamura, Planetary and Space Science 2009, doi: 10.1016/j.pss.2009.09.012

Figure 'SARA measurements of hydrogen flux on the Moon' reproduced with permission from Elsevier.

For more information:

Detlef Koschny, ESA Chandrayaan-1 Project Scientist
Email: Detlef.Koschny @ esa.int

Erratum to an earlier version of this article:
How the Moon produces its own water still remains a mystery. The SARA discovery is that the Moon reflects a large fraction of the incoming solar wind protons as hydrogen atoms. What happens with the solar wind protons absorbed by the surface is out of the scope of the SARA investigation.