Io tagged posts

By staring into the hellish landscape of Jupiter’s moon Io – the most volcanically active location in the solar system – Cornell University astronomers have been able to study a fundamental process in planetary formation and evolution: tidal heating.

“Tidal heating plays an important role in the heating and orbital evolution of celestial bodies,” said Alex Hayes, professor of astronomy.

“It provides the warmth necessary to form and sustain subsurface oceans in the moons around giant planets like Jupi...

New radio images from the Atacama Large Millimeter/submillimeter Array (ALMA) show for the first time the direct effect of volcanic activity on the atmosphere of Jupiter’s moon Io.

Io is the most volcanically active moon in our solar system. It hosts more than 400 active volcanoes, spewing out sulfur gases that give Io its yellow-white-orange-red colors when they freeze out on its surface.

Although it is extremely thin — about a billion times thinner than Earth’s atmosphere — Io has an atmosphere that can teach us about Io’s volcanic activity and provide us a window into the exotic moon’s interior and what is happening below its colorful crust.

Previous research has sh...

Cartilage template formation via engineered extracellular matrix. Credit: Syam Nukavarapu/UConn Photo

A team of UConn Health researchers has designed a novel, hybrid hydrogel system to help address some of the challenges in repairing bone in the event of injury. There are over 200 bones in an adult human skeleton, ranging in size from a couple of millimeters in length to well over a foot. How these bones form and how they are repaired if injured varies, and has posed a challenge for many researchers in the field of regenerative medicine.

Two processes involved with human skeletal development help all the bones in our body form and grow. These processes are called intramembranous and endochondral ossification, IO and EO respectively...

An artist’s rendering depicts Io’s volcanic plumes creating the atmosphere in sunlight. Credit: Image courtesy of Southwest Research Institute

Research reveals freezing effects of Jupiter’s shadow on moon’s volcanic gases. A study led by SwRI’s Constantine Tsang concluded that Io’s thin atmosphere, which consists primarily of sulfur dioxide (SO2) gas emitted from volcanoes, collapses as the SO2 freezes onto the surface as ice when Io is shaded by Jupiter. When the moon moves out of eclipse and ice warms, the atmosphere reforms through sublimation, where ice converts directly to gas. “This research is the first time scientists have observed this phenomenon directly, improving our understanding of this geologically active moon,” said Tsang, SwRI’s Space Science and Engineering Division.

The ...