Dali Chasma

Chasma on Venus
17°36′S 167°00′E / 17.6°S 167°E / -17.6; 167Diameter7,400 kmEponymDali

The Dali and Diana Chasma system consist of deep troughs that extend for 7,400 kilometers (4,600 mi) and are very distinct features on Venus. Those chasma connect the Ovda Regio and Thetis Regio highlands with the large volcanoes at Atla Regio and thus are considered to be the "Scorpion Tail" of Aphrodite Terra. The broad, curving scarp resembles some of Earth's subduction zones where crustal plates are pushed over each other. The radar-bright surface at the highest elevation along the scarp is similar to surfaces in other elevated regions where some metallic mineral such as pyrite (fool's gold) may occur on the surface.[1]

These features are named for the Georgian goddess Dali and the Roman goddess Diana, respectively.

References

  1. ^ Catalog Page for PIA00268
  • v
  • t
  • e
Venus
  • Outline of Venus
Geography
General
Regions
Regio
Terrae
Mountains
and
volcanoes
Plains and
plateaus
Canyons and
valleys
Craters
  • Addams
  • Adivar
  • Agnesi
  • Alcott
  • Ariadne
  • Aurelia
  • Balch
  • Barton
  • Buck
  • Cleopatra
  • Cunitz
  • Danilova
  • De Lalande
  • Dickinson
  • Goeppert-Mayer
  • Golubkina
  • Grimke
  • Gregory
  • Guilbert
  • Isabella
  • Jeanne
  • Maria Celeste
  • Mariko
  • Mead
  • Meitner
  • Merit Ptah
  • Mona Lisa
  • Nanichi
  • Riley
  • Ruth
  • Stefania
  • Wanda
  • Wheatley
  • Yablochkina
Other
Astronomy
General
Transits
Asteroids
Exploration
Past
Current
Planned
Proposed
Proposed
crewed
Other
Related
  • Category
  • Portal
Stub icon

This article about an extraterrestrial geological feature is a stub. You can help Wikipedia by expanding it.

  • v
  • t
  • e