The Earth is protected from solar wind and cosmic rays by the Earth's magnetic field. On the night side of the earth, the side opposite the Sun, the Earth’s magnetic field is extended like a comet tail and makes a space like a streamer (magnetosphere). At the center of the magnetosphere, there is an area which exists as a sheet-like structure of hot plasma.
A joint group of researchers from the Institute of Space and Astronautical Science and Nagoya University, led by Professor TERADA Kentaro at the Graduate School of Science, Osaka University, by using the Magnetic field and Plasma experiment/Plasma energy Angle and Composition experiment (MAP-PACE) on SELENE (Selenological and Engineering Explorer), known in Japan as the spacecraft "Kaguya," succeeded in observing that oxygen from the gravisphere of Earth was transported to the Moon 380,000 km away by solar activity.
This group examined plasma data of MAP-PACE 100 km above the Moon’s surface and discovered that high-energy oxygen ions (O+) appeared only when the Moon and Kaguya crossed the plasma sheet.
It had been known that oxygen ions flowed out from the polar regions into space; however, this group succeeded in observing that they were transported as “Earth wind” to the surface of the Moon, a world first.
O+ ions detected by this group had a high energy of 1-10 keV. These O+ ions can be implanted into a depth of tens of nanometers of a metal particle. This is a very important finding in understanding the complicated isotopic composition of oxygen on the lunar regolith, which has long been a mystery. Through their observation, this group demonstrated the possibility that components that lack 16O, which is a stable isotope of oxygen and is observed in the ozone layer, a region of Earth's stratosphere, were transported to the Moon surface as “Earth wind” and implanted into a depth of tens of nanometers on the surface of lunar soils.
Oxygen, which is vital to sustaining life and makes up about 20 percent of the Earth’s atmosphere, has been produced from photosynthesis of plants during the last 2 to 3 billion years. Discoveries like the one by this group will not only encourage researchers’ spirit of seeking truth, but will also have a great impact on the views of nature and science of the general public.
For five days of each lunar orbit, the Moon is shielded from solar wind bombardment by the Earth’s magnetosphere, which is filled with terrestrial ions. Although the possibility of the presence of terrestrial nitrogen and noble gases in lunar soil has been discussed based on their isotopic composition, complicated oxygen isotope fractionation in lunar metal (particularly the provenance of a 16O-poor component) remains an enigma. Here, we report observations from the Japanese spacecraft Kaguya of significant numbers of 1–10 keV O+ ions, seen only when the Moon was in the Earth’s plasma sheet. Considering the penetration depth into metal of O+ ions with such energy, and the 16O-poor mass-independent fractionation of the Earth’s upper atmosphere, we conclude that biogenic terrestrial oxygen has been transported to the Moon by the Earth wind (at least 2.6 × 104 ions cm−2 s−1) and implanted into the surface of the lunar regolith, at around tens of nanometres in depth. We suggest the possibility that the Earth’s atmosphere of billions of years ago may be preserved on the present-day lunar surface.
Figure 1. Photo by courtesy of Osaka University/NASA
To learn more about this research, please view the full research report entitled “Biogenic oxygen from Earth transported to the Moon by a wind of magnetospheric ions” at of the Nature Astronomy website.