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Illustration of Crab, Titan's Shadow and Chandra
(Credit: NASA/CXC/M.Weiss)

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Titan Casts Revealing Shadow

Credit: NASA/CXC/Penn State/K.Mori et al.

On January 5, 2003, Titan — Saturn's largest moon and the only moon in the solar system with a thick atmosphere — crossed in front of the Crab Nebula, a bright, extended X-ray source. Titan's transit enabled Chandra to image the one-arcsecond-diameter X-ray shadow cast by the moon (inset). This tiny shadow corresponds to the size of a dime as viewed from about two and a half miles.

The diameter of Titan's shadow was found to be larger than the known diameter of its solid surface. This difference in diameters yields a measurement of about 550 miles (880 kilometers) for the height of the X-ray absorbing region of Titan's atmosphere.

The extent of the upper atmosphere is consistent with, or slightly (10-15%) larger, than that implied by Voyager I observations made at radio, infrared, and ultraviolet wavelengths in 1980. Saturn was about 5% closer to the Sun in 2003, so increased solar heating of Titan may have caused its atmosphere to expand.

Although Titan passes within a few degrees of the Crab Nebula every 30 years, it rarely passes directly in front of it. This may have been the first transit of the Crab Nebula by Titan since the nebula was formed by a supernova that was observed to occur in the year 1054. The next similar conjunction will take place in the year 2267, so this was truly a once in a millennium event.

Fast Facts for Titan:
Credit  NASA/CXC/Penn State/K.Mori et al.
Scale  Image is 16.0 arcsec across.
Category  Solar System
Coordinates (J2000)  RA | Dec
Constellation  null
Observation Dates  January 5, 2003
Observation Time  8 hours
Obs. IDs  4413, 4412, 3727
Color Code  Intensity
Instrument  ACIS
References K. Mori, et al. astro-ph/0403283
Distance Estimate  760 million Miles
Release Date  April 05, 2004