'Comets of the Centuries': 500 Years of the Greatest Comets Ever Seen

Comet ISON by Waldemar Skorupa
German amateur astronomer Waldemar Skorupa captured this spectacular photo of Comet ISON from Kahler Asten, in Germany, on Nov. 16, 2013. (Image credit: Waldemar Skorupa (Kahler Asten, Germany) )

When Comet ISON was discovered and a preliminary orbit for it was worked out, it was initially announced that it could be the "comet of the century."

Of course, the 21st century is only 12 years old (from 2001) and ISON turned out to be a dud. But out there in the far recesses of space there is certainly some unknown comet worthy of such an honorific title that will ultimately put on a unique and memorable show sometime during this century. 

Take note that four of these five dazzlers appeared in the latter half of their century and that the average time between appearances amounts to 97 years. Considering that Comet Ikeya-Seki passed by in 1965, the next prospective "Comet of the Century" might not appear — according to our small sampling — until maybe 2029 at the earliest … and maybe not even until the next century (in 2103!). [Incredible Photos of Comet ISON]

By Nov. 8, it was reported by Japanese observers as a "broom star," appearing "as bright as the moon" with a white tail spanning over 60 degrees (your clenched fist held at arm's length measures 10 degrees). The famous astronomer Tycho Brahe first saw the comet as a reflection in his garden fish pond on Nov. 13, and likened its brightness to Venus. The comet was still as bright as zero magnitude inDecember before it finally dropped below the limit of naked-eye visibility on Jan. 26, 1578. (Magnitude is a measure of a celestial object's brightness, with smaller numbers corresponding to brighter objects.)

The German astronomer Gottfried Kirch became the first person to ever discover a comet with a telescope when he sighted this comet on Nov. 14, 1680, when it was at fourth magnitude. By Dec. 2, it already had a 15-degree tail and had reached second magnitude (as bright as Polaris, the North Star).  On Dec. 18, it was at perihelion (the closest point to the sun in its orbit) coming to within 128,000 miles (206,000 km) of the sun's surface.

At least one report (from Albany, NY) indicates that the comet was visible in the daytime. Several days later it could be seen in the evening twilight sky with a tail stretching straight up from a second-magnitude head from the southwest horizon for 70 to 90 degrees. By Jan. 10, 1681, the tail had shrunk to 55 degrees and by the Jan. 23 it measured "only" 30 degrees, with its head having faded to fourth magnitude. It remained visible to the naked eye until early February 1681.

By Sept. 14, it became visible in broad daylight, and when it arrived at perihelion on Dec. 17, it passed at a distance of only 264,000 miles (425,000 km) from the sun's surface. On that day, some observers described the comet's silvery radiance as scarcely fainter than the limb of the Sun, suggesting a magnitude somewhere between -15 and -20 (the latter magnitude would register nearly 1,000 times brighter than the full moon!). The following day, observers in Cordoba, Argentina, described the comet as a "blazing star" near the sun.

The nucleus also broke into at least four separate parts. In the days and weeks that followed, the comet became visible in the morning sky as an immense object sporting a brilliant tail. Today, some comet historians consider it a "Super Comet," far above the run of even great comets. [See Amazing Stargazer Photos of Comets from 2013]

The comet was then visible as a brilliant object within a degree or two of the sun, and wherever the sky was clear, the comet could be seen by observers merely by blocking out the sun with their hands. From Japan, the homeland of the observers who discovered it, Ikeya-Seki was described as appearing "10 times brighter than the full moon," corresponding to a magnitude of minus 15. Also at that time, the nucleus was observed to break into two or three pieces.

ISON fizzled, so we continue to wait…

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, the Farmer's Almanac and other publications, and he is also an on-camera meteorologist for News 12 Westchester, N.Y. Follow us @Spacedotcom, Facebook and Google+.

Joe Rao
Skywatching Columnist

Joe Rao is Space.com's skywatching columnist, as well as a veteran meteorologist and eclipse chaser who also serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky & Telescope and other publications. Joe is an 8-time Emmy-nominated meteorologist who served the Putnam Valley region of New York for over 21 years. You can find him on Twitter and YouTube tracking lunar and solar eclipses, meteor showers and more. To find out Joe's latest project, visit him on Twitter.