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Related Experiment Video

Updated: Jun 24, 2026

Methods for Image-based Surveys of Benthic Macroinvertebrates and Their Habitat Exemplified by the Drop Camera Survey for the Atlantic Sea Scallop

Methods for Image-based Surveys of Benthic Macroinvertebrates and Their Habitat Exemplified by the Drop Camera Survey for the Atlantic Sea Scallop

Published on: July 2, 2018

Oceans on titan?

Science (New York, N.Y.)

|July 1, 1983

Summary

This summary is machine-generated.

Titan

Area of Science:

Planetary Science
Astrobiology

Background:

Titan's atmosphere may contain methane oceans.
Voyager's radio occultation data provides insights into Titan's surface conditions.

Purpose of the Study:

To assess the likelihood of methane oceans on Titan based on atmospheric saturation levels.
To determine conditions under which methane oceans could exist on Titan.

Main Methods:

Analysis of Voyager radio occultation data.
Atmospheric modeling of Titan's near-surface conditions.

Main Results:

Atmospheric methane saturation near 100% is required for methane oceans.
Voyager data suggests low surface humidity, implying land at sounding locations.

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Methods for Image-based Surveys of Benthic Macroinvertebrates and Their Habitat Exemplified by the Drop Camera Survey for the Atlantic Sea Scallop

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The Floating Lab: Standard Operational Procedure for Collecting and Filtering Seawater Samples from Operating Ferries for Environmental DNA Analysis

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Low zonal wind speeds (< 4 cm/s) are necessary for potential low-latitude oceans.

Conclusions:

Methane oceans may exist in unexplored low-latitude regions of Titan.
Specific atmospheric and wind conditions are critical for the presence of surface methane liquid.