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Important notice about reduced STEREO science operations

Observing Comet Elenin

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Comet Elenin as seen by HI1-B on Aug. 6, 2011.

As Comet Elenin passed to within just 7 million kilometers of the STEREO (Behind) spacecraft, NASA rolled the spacecraft to take a look at it (Aug. 1, 2011) with its wide angle HI-2 instrument. Though the observation lasted only a little over an hour, the fuzzy looking comet can be seen moving across a small portion of the sky. STEREO will be taking these one-hour observations every day through August 12. The comet is seen by the HI-2 telescope between August 1-5, and by the higher resolution HI-1 telescope between August 6-12. From August 15 onward, the comet enters the HI-1 telescope's nominal field of view, at which time we should enjoy continuous viewing of the comet. Over time, we expect the comet to be visible in the SOHO C3 coronagraph on September 23 for six days and possibly STEREO's COR2 coronagraph as well between August 20 and September 1. The closest the comet will come to Earth is 0.23 AU (Astronomical Units), or approximately 34-million kilometers, so it poses no threat to us. We will attempt to keep this page updated with the latest observations.

Single frames showing the comet are available, together with the regular synoptic images, as part of the SECCHI image gallery.

We do expect the comet to appear to become significantly brighter over the next few days as it gets closer to the Sun-spacecraft line as a consequence of a process known as foward-scattering. STEREO-B, which is far from Earth, happens to see this "back-lighting" effect as a consequence of its location relative to the comet, and is not indicative of a sudden change in the comet itself.

Russian astronomer Leonid Elenin discovered the comet last December at International Scientific Optical Network's robotic observatory near Mayhill, New Mexico.

From Earth, presently the comet is a faint smudge of light in deep sky exposures. By late August comet Elenin could be visible to the naked eye as a dim "fuzzy star" with a tail.


Last Revised: September 05, 2014 17:32:36 UTC
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