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LUNAR METEORITE NWA 11273

The lunar surface is fully exposed to outer space due to the absence of the atmosphere. When large asteroids hit the Moon, the collision causes lunar material to lift and disperse. The impact has to be forceful enough in order for lunar rocks to reach the Moon’s escape velocity and make it to outer space. The minimum particle speed required for this to happen is 2.38 km/s. Once the material escapes the Moon’s gravity, rock fragments are captured by the gravitational fields of either the Earth or the Sun. When such fragments fall on the Earth, they are called lunar meteorites.

Collected on Earth by the world's most recognized scientists and renowned collectors from the International Society for Meteoritics and Planetary Science, fragments used are trackable in the World's database of Space Material (Meteoritical Bulletin). Our team consists of meteorite experts, holding university degrees in meteoritic sciences and are classifying space material for the International Space Material Database. 

 

Lunar material inserted inside a glass sphere is museum verified. 

We are honored to have among friends a great scientist who is an active contributor to the meteorite community, an author, and the chief curator of the largest display of space material in the world at the Natural History Museum in Vienna, Dr. Ludovic Ferriere. Between his scientific work and taking care of the international meteorite treasure, Dr. Ferriere also travels the globe in search of new impact craters to be confirmed.

Explore Lunar meteorites in detail.

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MACHINE LEARNING AND AUGMENTED REALITY

We have developed a machine-learning algorithm recognising Spherica and activating augmented reality.

STELLAR THEOREM

Spherica funds curious projects of creative individuals contributing to space research. The power resides in an impact.

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