Comet Holmes' close-up
Scientists employed one of the largest CCD cameras to image Comet 17P/Holmes as it fades from view.
November 30, 2007
Provided by the Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts
Comet 17P/Holmes, which dazzled sky watchers with a dramatic outburst that made it visible to the unaided eye, now is fading from sight. However, before it returns to the obscurity from which it came, astronomers at the MMT Observatory took a final look.
On November 4th, Comet 17P/Holmes was about 2nd magnitude and spanned approximately 20 arcminutes on the sky, about 2/3 the size of the Full Moon. Scientists combined separate 20-second exposures through multiple filters to make this full-color view. They used the MMT Observatory's Megacam at Mount Hopkins, Arizona.
Photo by M. Ashby and N. Caldwell (CfA)
In late October, Holmes brightened by a factor of about one million times when it ejected a vast cloud of dust and gas. That cloud expanded over time and now spans more than 870,000 miles, making it larger than the Sun (which is 865,000 miles in diameter).
On November 4, Smithsonian scientists snapped this photo of Comet Holmes using an instrument called Megacam, which is one of the largest CCD cameras in existence. Megacam holds 36 nine-megapixel CCD chips, for a total of more than 300 megapixels.
Separate exposures through three color filters were combined to make this final, full-color image. Individual stars appear as a line of colored dots because the photos were centered on the comet, which moved slightly across the sky.
Currently, Comet Holmes has a total brightness of 3rd magnitude, however its large size on the sky (and resulting low surface brightness) makes it difficult to see without binoculars or a telescope. However, when it was discovered in 1892 it underwent a second bright outburst five months after the first. If Holmes repeats its historical performance, then this comet may offer viewers one more chance to see the show before it bows from the stage.