A Look Back at Comet Hale-Bopp
By: Brian Ventrudo, March 25, 2016
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At any particular time, a half-dozen or more comets are visible with a good-sized amateur telescope. But a bright comet is a once-in-a-decade event at best, and a Great Comet, one that grows bright enough to capture wide attention, is rarer still. Recently there have been two Great Comets visible to observers in the southern hemisphere, Comet McNaught in 2007 and Comet Lovejoy in 2011. But it’s been a long drought for stargazers in the northern hemisphere, where no spectacular comet has been seen since 1997 when the mighty Comet C/1995 O1, better known as Comet Hale-Bopp, barreled in from the outer solar system and put on one of the most watched celestial shows in modern history.
Like most newly-observed comets, Hale-Bopp was discovered by accident. On the night of July 23, 1995, the astronomer Alan Hale was visually tracking fainter comets using a telescope in his driveway at his home in New Mexico when he noticed an unexpected smudge near the globular cluster M70 in the constellation Sagittarius. The constellation is chock-a-block with fuzzy deep-sky objects, so Hale took care to make sure the new object was indeed uncharted, and he watched it move against the background stars during the night. Satisfied he had found something interesting, he followed astronomical protocol and sent an email with the position and motion of the object to Brian Marsden at the Central Bureau for Astronomical Telegrams at Harvard, the official center for tracking and announcing transient astronomical events such as comets.
On the same night, Marsden was surprised to receive not an email but an old-fashioned telegram. It came from the amateur stargazer Thomas Bopp in Arizona. Bopp, an auto parts manager who didn’t own a telescope, was out with friends touring Sagittarius with a homemade 17.5″ Dobsonian when he watched the globular cluster M70 drift out of the field of view of the stationary telescope and watched the comet drift in. He also confirmed it was an uncharted object and contacted Western Union to send the word to Harvard. The next morning, the comet was announced to the world.
Astronomers suspected right away that Hale-Bopp was a big one. It had a brightness of magnitude 10.5 when it was discovered by Hale and Bopp between the orbits of Jupiter and Saturn. That’s extremely bright for such a distant comet. Comet Halley, by comparison, was 100 times (five full magnitudes) fainter at the same distance. The new comet also had a resolvable coma which suggested a large and active nucleus. It turned out the nucleus had a diameter of some 60 km, more than six times as large as the nucleus of Halley.
Comet Hale-Bopp followed fast on the tail of another Great Comet, the splendid Comet C/1996 B2 (Hyakutake), which reached peak brightness in 1996. But astronomers were cautious to declare that Hale-Bopp would be an even more spectacular object. They didn’t want to oversell the object and foster disappointment if the comet fizzled.
But the comet did brighten, spectacularly so, during the last months of 1996 and into 1997. It was visible to the unaided eye for an astonishing 18 months, from May 1996 to December 1997, and in March and April of 1997 outshone nearly every star in the sky. It was easily visible even from urban skies and sported its now-famous double tail that stretched 40° across the sky. Even the Great Comet of 1811, a spectacular sight by all accounts, remained visible to the naked eye for just 9 months.
Hale-Bopp made its closest approach to Earth on March 22, 1997 at a distance of 1.32 astronomical units (about 200 million kilometers) and its closest approach to the Sun on April 1, 1997.
This Great Comet of 1997 was perhaps the most observed comet in history by amateur stargazers and by the general public. Scientists did their part, too, and closely examined this immense comet for months and years as it passed Earth and moved again towards the outer solar system. Among the discoveries made by the professionals:
- Dust grains in the unusually dense coma were among the smallest ever observed around any comet
- The comet had a high ratio of deuterium (heavy hydrogen) to regular hydrogen, much higher than the ratio observed in Earth’s oceans, which suggested not all water on Earth came from cometary impacts, and that the comet formed at a temperature of about 25 K in the outer reaches of the early solar system.
- A large abundance of organic molecules was found in the gas and dust of the coma, suggesting the comet, and all comets, might contain the building blocks of simple biologically active molecules
- By observing jets of material ejected by the comet’s nucleus, astronomers measured the rotation rate of the nucleus to be a little less than 12 hours
- In addition to the blue ion tail that pointed away from the Sun, and the white dust tail that followed the orbit of the comet, a third and much fainter tail consisting of neutral sodium atoms extended more than 50 million kilometers from the nucleus between the two brighter tails
Astronomers also found that Comet Hale-Bopp had been this way before, roughly about 4,200 years ago in 2215 B.C. Ancient Egyptian records do indeed indicate a bright “hairy star” may have appeared in the sky at that time. This ancient visit may have been the comet’s first approach to the inner solar system from the distant Oort Cloud. On its most recent visit, the comet’s orbital period was shortened by a gravitational interaction with Jupiter. It will come again to the inner solar system some 2,530 years from now in the year 4525 A.D.
Amazingly, the comet is still visible in very large telescopes. It will likely fade to an unobservable 30th magnitude by 2020.
When will the next Great Comet arrive? No one knows, but it’s been a long drought, at least for us observers north of the equator. The odds suggest it won’t be too much longer.
Note: If you really want to walk down memory lane with Comet Hale-Bopp, have a look at a comprehensive image archive of the comet at this link. This webpage was so popular in 1997 that it received more than a million page views on a single day and clogged the nascent internet.
About the Author
Brian Ventrudo is a writer, scientist, and astronomy educator. He received his first telescope at the age of 5 and completed his first university course in astronomy at the age of 12, eventually receiving a master's degree in the subject. He also holds a Ph.D. in engineering physics from McMaster University. During a twenty-year scientific career, he developed laser systems to detect molecules found in interstellar space and planetary atmospheres, and leveraged his expertise to create laser technology for optical communications networks. Since 2008, Brian has taught astronomy to tens of thousands of stargazers through his websites OneMinuteAstronomer.com and CosmicPursuits.com.
This article is © Brian Ventrudo 2015. All rights reserved.