© 1985, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112
On February 9, 1986, the most famous comet of all time will make the closest approach to the Sun in its current 76-year trip around our star. For a few months, before and after that date, the comet will be visible from our vantage point on the Earth — but, alas, not as well as it was in 1910. We begin the inaugural issue of The Universe in the Classroom with an in-depth look at Comet Halley (pronounced to rhyme with "Sally'') and its upcoming "not-so-close encounter'' with the Earth.
According to our modern theories, comets are frozen debris, left over from the formation of the solar system. We believe there is a vast "cloud'' of icy pieces in the outer regions of the solar system, far beyond the orbit of Pluto. While most of these will never leave their distant orbits, a few are disturbed in their motion and come into the inner solar system, revealing themselves to us.
These comets then move around the solar system in huge elongated orbits, which means they spend most of their time far away from the Sun. Out there a comet remains frozen and is invisible to even our best telescopes. But as a comet's path brings it closer and closer to the Sun, the heat begins to evaporate the ices and release some of the dust particles trapped within them.
The freed gas and dust particles form a cloud or "halo'' around the iceberg which astronomers call a coma. A comet's coma can get as large as 100,000 km across as the comet nears the Sun, and the glowing gases of the coma produce the "fuzzy patch'' appearance we associate with comets.
Not all the material liberated from the comet iceberg remains in the coma. A flow of high speed particles from the Sun (which astronomers call the "solar wind'') pushes on the gas particles in the coma and sweeps them into a long "tail'' pointing away from the Sun. In addition, the dust particles in the outer coma are pushed into a gently curving dust tail by the pressure of the Sun's radiation.
Comet tails can stretch out for more than 10 million kilometers. Yet they contain so few particles in total that the material in a com- et tail could easily fit into an average suitcase and leave enough room for a change of clothes.
Some comets, on the other hand, have had their orbits altered by the gravitational pull of the giant outer planets — Jupiter, Saturn, Uranus, and Neptune. These "short-period comets'' — of which about 100 are known — mostly stay within the region of the planets and can thus grace our skies much more regularly.
Comet Halley is a fine example of a short-period comet, taking about 76 years to make one orbit around the Sun. At its closest point (perihelion), the comet is only 88 million kilometers from the Sun (about 60% of the Earth's distance from our star.) At its most distant point (aphelion), Halley is 5.2 billion kilometers from the Sun and thus beyond the orbit of Neptune.
Why is the comet named Halley?
The coma and tail of a comet, indicated on a photograph of Halley's Comet taken on May 8, 1910. (Mt. Wilson Observatory photograph.)
Is Comet Halley on target for its rendezvous with the inner solar system?
On October 16, 1982, a team of astronomers led by David Jewett and G. Edward Danielson recovered Comet Halley using the 200-inch telescope on Palomar Mountain in Southern California. Since the comet at that time was about fifty million times fainter than the faintest objects our eyes can see, they had to use not only the largest American telescope but also special electronic equipment which had been developed for the upcoming Space Telescope.
When they found the comet, it was about 1.6 billion kilometers from the Sun, still beyond the orbit of Saturn. This recovery beats the previous record for finding Comet Halley by over two years! The comet was almost exactly where astronomers predicted it would be and right on time for its closest pass to the Sun on February 9, 1985.
On its way in toward the Sun, Comet Halley will pass closest to the Earth on November 27, 1985, at a distance of 93 million kilometers. On its outward journey, the comet will come within 48 million kilometers of us on April 11,1986. In 1910, however, the closest approach was within 24 million kilometers and we passed through one part of the comet's tail. Therefore, the comet will look a lot fainter this time around and some astronomers predict that in the bright skies of most cities it may well be invisible to the naked eye.
To make things a bit more complicated, the comet's orbit is tilted when compared to the orbits of the planets. This means that the comet will be better seen in the Northern Hemisphere as it approaches the Sun and in the Southern Hemisphere as it is leaving. Since it will be closer to the Earth in the spring of 1986, Southern Hemisphere observers get a better show this time around. But the best views of the comet should come from spacecraft and orbiting observatories (see below).
The best way for the average person to observe the comet will be to use a good pair of binoculars in a location that is away from city lights and has a good view of the horizon (since the comet will be low in the sky). 7x50 or 7x35 binoculars should provide the best views.
During the second week in April the comet will be very low in the predawn sky and impossible for many of us in the U.S. to see. It will become visible later in April in the evening sky and will be getting fainter and fainter as the month goes on.
We will have much more detailed observing guides and suggestions in this newsletter as the comet comes closer.
Comets, on the other hand, spend most of their time in the "deep-freeze'' of the outer solar system. The material in the comet "iceberg'' is thus well preserved and could tell us a great deal about what things were like in that ancient time.
Astronomers can also use comets as probes of the present conditions in the solar system. By watching a comet's coma and tail develop and change, we can learn about the flow of particles and energy from the Sun, the details of the magnetic fields and particles between the planets, and the detailed characteristics of the comets themselves.
Not only will Halley be observed with all sorts of telescopes on Earth, the advent of the space age makes it possible for the first time to send space probes to make close-up measurements of the comet's properties. A small armada of spacecraft will monitor Halley, including five that will fly by the comet in March of 1986. Japan and the Soviet Union are each sending two probes to Halley, while the European Space Agency (the European equivalent of NASA) is sending one. The U.S. decided not to send a fly-by craft to Halley, but we are redirecting an older probe to fly by another comet (Giacobini-Zinner) in September 1985. In addition we will be making observations of Comet Halley with a special package of instruments called Astro 1, to be carried aloft by the Space Shuttle in early March of 1986.
Before we understood the nature and orbits of comets, people worried about the effects a comet might have on us. Today we know enough about these objects to provide a reassuring "environmental impact statement.'' Unless a comet physically collides with the Earth (which Halley will be far from doing), these small chunks of dirty ice pose no danger to us. Their effects are on the mind, stimulating our curiosity and kindling our imaginations.
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