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Haraiya

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description Haraiya Overview

Haraiya is a howardite meteorite that fell in the state of Uttar Pradesh, India. Howardites are a group of achondritic meteorites formed from the surface regolith of asteroid 4 Vesta. Haraiya is characterized as a polymict breccia, meaning it is composed of mixed fragments of both eucrite and diogenite rocks that were lithified together. This composition provides scientists with a comprehensive sample of the diverse crustal lithologies present on Vesta, offering valuable data for understanding the volcanic and impact history of large differentiated asteroids.

help Haraiya FAQ

Why is Haraiya classified as a howardite rather than an ordinary chondrite?

Haraiya is an achondritic breccia made from mixed fragments of differentiated asteroid material, not a chondrite containing primitive chondrules. Howardites are associated with the surface of asteroid 4 Vesta.

What does polymict breccia mean in the case of Haraiya?

Polymict means that Haraiya contains many different rock fragments cemented together in one meteorite. That mixture reflects regolith material repeatedly broken up and redeposited on 4 Vesta's surface.

How does Haraiya relate to eucrites and diogenites?

Howardites such as Haraiya commonly contain fragments related to both eucrites and diogenites. Together, these meteorites form the HED group, which is linked to 4 Vesta.

Where did Haraiya fall?

Haraiya fell in the Indian state of Uttar Pradesh. Its observed fall location is important because it distinguishes the meteorite from many finds recovered later from deserts.

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