Earth-like snow, ice features found on Pluto

“Penitentes” — formed by erosion — are bowl-shaped depressions with spires around the edge and indicate presence of an atmosphere.

January 05, 2017 08:40 pm | Updated 08:43 pm IST - TORONTO:

A heart shaped region named Sputnik Planum is seen in enhanced view of the dwarf planet Pluto in an undated image from NASA’s New Horizons spacecraft. The coldest planet in the solar system boasts of “Penitentes” which are formed by erosion and are bowl-shaped depressions with spires around the edge, being several metres high. Scientists say “Penitentes” suggest the presence of an atmosphere is necessary.

A heart shaped region named Sputnik Planum is seen in enhanced view of the dwarf planet Pluto in an undated image from NASA’s New Horizons spacecraft. The coldest planet in the solar system boasts of “Penitentes” which are formed by erosion and are bowl-shaped depressions with spires around the edge, being several metres high. Scientists say “Penitentes” suggest the presence of an atmosphere is necessary.

Scientists have found evidence of Earth-like snow and ice features on Pluto, using a model similar to what meteorologists use to forecast weather on our planet and a computer simulation of the physics of evaporating ices.

“Penitentes” which are formed by erosion, are bowl-shaped depressions with spires around the edge, and are several metres high.

The groundbreaking research, done in collaboration with researchers at NASA and Johns Hopkins University, indicates that these icy features may exist on other planets where environmental conditions are similar.

“The identification of the ridges of Tartarus Dorsa as Penitentes suggests that the presence of an atmosphere is necessary for the formation of penitentes, which would explain why they have not previously been seen on other airless icy satellites or dwarf planets,” said Professor John Moores, from York University in Canada.

May be many in solar system

“But exotic differences in the environment give rise to features with very different scales. This test of our terrestrial models for penitentes suggests that we may find these features elsewhere in the solar system, and in other solar systems, where the conditions are right,” said Prof. Moores. He and his colleagues compared their model to ridges on Pluto imaged by the New Horizons spacecraft in 2015.

Pluto’s ridges are much larger — 500 metres tall and separated by three to five kilometres — as compared to their meter-sized earthly counterparts.

“This gargantuan size is predicted by the same theory that explains the formation of these features on Earth,” said Prof. Moores.

“In fact, we were able to match the size and separation, the direction of the ridges, as well as their age: three pieces of evidence that support our identification of these ridges as penitentes,” he said.

Same laws of nature apply

Prof. Moores said though Pluto’s environment was very different from the Earth — it is much colder, the air much thinner, the sun much dimmer and the snow and ice on the surface are made from methane and nitrogen instead of water — the same laws of nature apply.

The finding was published in the journal Nature .

0 / 0
Sign in to unlock member-only benefits!
  • Access 10 free stories every month
  • Save stories to read later
  • Access to comment on every story
  • Sign-up/manage your newsletter subscriptions with a single click
  • Get notified by email for early access to discounts & offers on our products
Sign in

Comments

Comments have to be in English, and in full sentences. They cannot be abusive or personal. Please abide by our community guidelines for posting your comments.

We have migrated to a new commenting platform. If you are already a registered user of The Hindu and logged in, you may continue to engage with our articles. If you do not have an account please register and login to post comments. Users can access their older comments by logging into their accounts on Vuukle.