Moons of Saturn, Part 2 Codexery

Tiger stripes (Enceladus)

Four active fractures on Enceladus with cryovolcanic plumes.

Tiger stripes (Enceladus)

The tiger stripes are four sub-parallel, linear depressions in the south polar region of Saturn's moon Enceladus. They are notable for their elevated surface temperatures and association with present-day cryovolcanism, including a plume of water vapor and ice, methane, carbon dioxide, and nitrogen.

First observed
May 20, 2005
Observed by
Cassini spacecraft's Imaging Science Sub-system (ISS) camera
Number of features
4
Average length
130 kilometers
Average width
2 kilometers
Average depth
500 meters
Ridge height
100 meters
Ridge width
2–4 kilometers
Spacing
approximately 35 kilometers
Surface age estimate
4–100 million years (lunar-like flux) or 0.5–1 million years (constant flux)

Lore & Background

First observed on May 20, 2005, by the Cassini spacecraft's ISS camera, the tiger stripes were seen obliquely during an early flyby. Higher resolution observations on July 14, 2005, revealed them to be low ridges with a central fracture. The Composite Infrared Spectrometer (CIRS) showed elevated surface temperatures, indicating present-day cryovolcanism centered on the stripes. The name 'tiger stripes' is unofficial, based on their distinctive albedo. In November 2006, they were assigned the official names Alexandria Sulcus, Cairo Sulcus, Baghdad Sulcus, and Damascus Sulcus; Baghdad and Damascus sulci are the most active, while Alexandria Sulcus is the least active. The stripes are tectonic fractures, likely fissures in the lithosphere, with hook-shaped bends on the anti-Saturnian hemisphere and bifurcating tips on the sub-Saturnian hemisphere. Virtually no impact craters are found on or near them, suggesting a very young surface age.

Reader's Guide

The tiger stripes are significant as the locus of Enceladus's cryovolcanic activity, confirmed by Cassini's July 14, 2005 flyby. The CIRS instrument measured color temperatures of 113–157 kelvins, far warmer than the expected 68 kelvins, and data from ISS, INMS, CDA, and CIRS showed a plume of water vapor, ice, methane, carbon dioxide, and nitrogen emanating from jets within the stripes. This plume is the source of material for Saturn's E Ring, as confirmed by Cassini's first two close flybys in 2005. The stripes' composition includes coarse-grained crystalline water ice, trapped carbon dioxide ice, and simple organics not found elsewhere on Enceladus. The crystalline ice provides an age constraint of a few decades to a thousand years for surface exposure. The stripes' geologic setting and lack of craters indicate a young surface, with age estimates of 4–100 million years or 0.5–1 million years depending on cratering flux assumptions. The discovery of over 100 geysers and the plume's material suggests a near-surface body of liquid water, though an alternative hypothesis proposes clathrate hydrates as the source.

Did You Know?

More in Moons of Saturn, Part 2 1-24

Spotted an error? Know more?

Reader corrections go straight into our review queue. Suggest an edit · How this site is sourced

Comments

Loading…
Open in the interactive codex →