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Reading: Researchers Discover Water on Large Asteroids Iris and Massalia
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Space

Researchers Discover Water on Large Asteroids Iris and Massalia

Highlights

  • SOFIA telescope data shows asteroids Iris and Massalia have water.

  • Dr. Anicia Arredondo's study reveals water bound to asteroid minerals.

  • James Webb Telescope to further research Solar System's water distribution.

NEWSLINKER
Last updated: 13 February, 2024 - 4:46 pm 4:46 pm
NEWSLINKER 1 year ago
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Innovative astronomical research has revealed the presence of water molecules on two of the Solar System’s larger asteroids, challenging previous assumptions about dry celestial bodies in our cosmic backyard. The Stratospheric Observatory for Infrared Astronomy (SOFIA) telescope’s data was instrumental in this finding, which suggests that asteroids could play a vital role in our understanding of water distribution in space.

Contents
Orbital Giants Harbor WaterWater Presence Beyond Earthly Boundaries

Orbital Giants Harbor Water

Among the vast array of asteroids, Iris and Massalia stand out not only for their considerable size but also for their now-confirmed water content. These celestial bodies, part of the millions populating the asteroid belt, are significant due to their specific orbital characteristics. Iris, with its 199 km diameter, completes an orbit every 3.7 years, while the slightly smaller Massalia boasts a similar orbit. The study’s conclusions about their water content mark a significant advancement in astrophysical studies.

Water Presence Beyond Earthly Boundaries

While SOFIA has ceased operations, its legacy continues through discoveries like the detection of water on Iris and Massalia. Renowned for its prior revelation of water on the Moon’s surface, the infrared telescope has once again underscored its scientific value. SOFIA’s data, captured through its Faint Object InfraRed Camera (FORCAST), has been crucial in identifying water signatures on these asteroids, likening their water content to that discovered on the lunar surface.

The significant finding, spearheaded by Dr. Anicia Arredondo, aligns the water volume on these asteroids with lunar measurements. The spectral data indicates that water molecules are bound within minerals on the asteroids’ surface, suggesting that such celestial bodies could be more than just arid rocks drifting through space.

Analysis of additional, fainter asteroids such as Parthenope and Melpomene was inconclusive, likely due to FORCAST’s limited sensitivity. This underlines the need for more powerful observational tools to further study the water content on smaller space rocks.

The research team now turns its attention to the James Webb Space Telescope, with its superior optics and sensitivity, to delve deeper into the mysteries of water in our Solar System. This cutting-edge telescope promises to enhance our comprehension of water’s role in the cosmos and its potential connection to extraterrestrial life.

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