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== Comets == Forward scattering can make a back-lit comet appear significantly brighter because the dust and [[ice crystal]]s are reflecting and enhancing the apparent brightness of the comet by scattering that light towards the observer.<ref name="scattering">{{cite web |title=Comet Elenin as seen by STEREO-B, and what we think is going to happen next... |publisher=Sungrazing Comets |url=https://sungrazer.nrl.navy.mil/index.php?p=Elenin |access-date=2011-08-05 |archive-date=2011-09-26 |archive-url=https://web.archive.org/web/20110926203659/http://sungrazer.nrl.navy.mil/index.php?p=Elenin |url-status=live }}</ref> Comets studied forward-scattering in visible-thermal photometry include [[Comet Skjellerup–Maristany|C/1927 X1 (Skjellerup–Maristany)]], [[Comet West|C/1975 V1 (West)]], and C/1980 Y1 (Bradfield).<ref name=Marcus2007>{{cite journal |last=Marcus |first=Joseph C. |title=Forward-Scattering Enhancement of Comet Brightness. I. Background and Model |journal=International Comet Quarterly |volume=29 |issue=2 |pages=39–66 |year=2007 |bibcode=2007ICQ....29...39M}}</ref> Comets studied forward-scattering in [[Solar and Heliospheric Observatory|SOHO]] non-thermal C3 [[coronograph]] photometry include [[96P/Machholz]] and C/2004 F4 (Bradfield).<ref name=Marcus2007/> The brightness of the [[great comet]]s [[C/2006 P1]] (McNaught) and [[Comet Skjellerup–Maristany]] near [[perihelion]] were enhanced by forward scattering.<ref name="fscat">{{Cite journal |url = http://www.icq.eps.harvard.edu/marcus_icq29_119.pdf |bibcode = 2007ICQ....29..119M |title = Forward-Scattering Enhancement of Comet Brightness. II. The Light Curve of C/2006 P1 |journal = International Comet Quarterly |volume = 29 |first = Joseph N. |last = Marcus |date = October 2007 |pages = 119–130 |url-status = dead |archive-url = https://web.archive.org/web/20110708051321/http://www.icq.eps.harvard.edu/marcus_icq29_119.pdf |archive-date = 2011-07-08 }}</ref>
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