Have you ever looked up in the sky and seen a little ball creeping by? If so, did you wonder what it was? That little ball is called a comet. Comets are small, fragile, and irregularly shaped. Most are composed of frozen gas. However, some are composed of frozen gas and non-volatile grains. They usually follow very strict paths around the sun. Comets become most visible when they cross the sun. This also applies to people who view comets with telescopes. When a comet gets near the sun it becomes very visible because the sun’s radiation starts to sublime its volatile gases, which, in turn, blow away small bits of the little solid material the comet has.
Another feature of a comet is a long tail. This is caused by materials breaking off and expanding. They expand into an enormous escaping atmosphere called the coma. This becomes at least the size of our planet. With the comet going so fast, these materials are forced behind the comet, forming a long tail of dust and gas.
Comets are cold bodies. We see them only because the gases they are composed of glow in the sunlight. All comets are regular family members of the solar system family. They are bound by gravity to a strict path around the solar system. Scientists believe that all comets were formed of material, originally in the outer part of the solar system, which did not become incorporated into planets. This material is from when the planets just started forming. This makes comets an extremely interesting topic to scientists who are studying the history of the solar system.
In comparison to planets, comets are very small. They can be anywhere from 750 meters (or less) to 20 kilometers in diameter. However, lately, scientists have been finding proof that there are comets 300 kilometers in diameter or greater.
Comets are still compared to the planets, though. Planets usually follow the shape of a sphere. Most planets are fat at the equator. Comets come in all different shapes and sizes. Most evidence that science has revealed says that comets are extremely fragile. A comet is so poorly structured that it is like a loose snowball–it can be pulled apart with one s own bare hands.
Comets have very awkward rotation periods. They are very oblong. When comets reach their aphelion they are usually near Jupiter or even sometimes Neptune. Other comets, however, come from even farther out in the solar system. No matter what, if a comet passes Jupiter, it is strongly attracted to it. Sometimes Jupiter s massive gravitational pull makes comets slam into planets .
Comets’ nuclei look like dirty snowballs. They are solid, persisting of ice and gas. Most nuclei contain rock, actually, small grains of rock somewhat like rock here on Earth. A nucleus appears to be black in color because it is made up of carbon compounds and sometimes free carbon. Since comet nuclei are so small they are difficult to study from Earth.
An interesting feature of a comet that few people know is that even though a comet appears to have a single tail, it actually has two. One tail is a dust tail and the other is an ion tail.
Although comets are very old, the oldest comet recorded is Comet Halley. They are Chinese records of this comet dating as far back as 240 BC Sir Edmund Halley predicted in 1705 that a comet which had appeared in 1531, 1607, and also 1682 would return in 1758. (unfortunately, the comet appeared on the day he was born and the day he died, he never got to see the comet) It was named Comet Halley in honor of him. A sighting of the comet was confirmed on Christmas day 1758.
Halley predicted the date on which the comet would return using Kepler s Third Law which states:
1. All orbits are ellipses with the sun at one focus.
2. A line between a planet and the Sun sweeps out an equal area during any fixed interval of time (i.e. planets move quickly when they are close to the sun)
3. (OrbitalPeriod(years))squared = (OrbitalRadius(AU))cubed
Alan Hale is a native New Mexican. Hale is a professional astronomer, he specializes in studying sunlike stars and searching for other planetary systems. He has been studying comets since 1970. Here is how he discovered the comet:
During my normal study of comets, it is my practice to observe comets once a week, on the average, and measure their brightnesses. On the night of July 22–the first clear night here in a week and a half–I planned to observe two comets. I finished with the first one–Periodic Comet Clark–shortly before midnight, and had about an hour and a half to wait before the second one–Periodic Comet D Arrest–rose high enough in the east to get a good look at. I decided to pass the time by observing some deep-sky objects in Sagittarius, and when I turned my telescope (a Meade DS-16) to M70, I immediately noticed a fuzzy object in the field that hadn t been there when I had looked at M70 two seeks earlier. After verifying that I was indeed looking at M70, and not one of the many other globular clusters in that part of the sky, I checked the various deep-sky catalogues, then ran the comment-identification program at the IAU Central Bureau s computer in Cambridge, Massachusetts. I sent an e-mail to Brian Marsden and Dan Green at the Central Bureau at that time informing them of a possible comet; later, when I had verified that the object had moved against the background stars, I sent them an additional e-mail. I continued to follow the comet for a total of about 3 hours, until it set behind trees in the southwest, and then was able to e-mail a detailed report, complete with two positions.
After he discovered the comet he said I love this irony — I ve spent over 400 hours of my life looking for comets, and I haven t found anything, and now, suddenly, when I m not looking for one, I get one dumped right in my lap. I had obtained an observation of P/Clark earlier, and I needed to wait an hour or so before P/d Arrest got high enough to look at, and I was just passing time til then and I decided to look at some deep-sky objects in Sagittarius. When I turned to M70, I saw a fuzzy object in the same field, and almost immediately expected a comet, since I had been looking at M70 last month, and *knew* there wasn t any objects there.
It all started for Bopp on July 22nd, 1995 on the exact night that Alan Hale saw the comet. In fact, they both saw the comet within 5 minutes of each other. Alan Hale was the first person to see it however. Here is the story of Thomas Bopp.
On the night of July 22, some friends and I headed out into the desert for a dark moon observation session. The site, which is west of Stanfield, Arizona, and a few miles of interstate 8 is about 90 miles southwest of my home.
My friend Jim Stevens had brought his 17-1/2 Dobsonian. We started the evening observing some of the messier objects such as the Veil and the North American Nebulae in Cygnus, when Jim said Lets look at some of the globularsin Sagittarius. We started our tour with M22 and M28, observing at 50X and then 180X. Around 11:00 local time, we had M70 in the field when Jim went to the charts to determine the next object of investigation. I continued watching M70 slowly drift across the field, when it reached a point 3/4 of the way across an alight glow appeared on the eastern edge. I repositioned the scope to the center on the new object but was unable to resolve it. I called to Jim and asked him if he knew what it might be, after visual inspection he stated he was not familiar with it but would check the charts. After determining the general position of the object he was unable to find it on Sky Atlas 2000.0 or Uranometria.
The moment Jim said we might have something excitement began to grow among our group and I breathed a silent prayer thanking God for his wondrous creation. My friend, Kevin Gill then took a position from his digital setting circlesand estimated a magnitude.
At 11:15 I said that we needed to check the object for motion and should watch it for an hour. The group observed it change position against the star field over that period and at 12:25 I decided to drive home and report our finding.
Arriving at home, initial attempts to send a telegram were unsuccessful due to an incomplete address I had. After searching my library I was able to locate the correct address and confirmation was requested.
At 8:25 A.M. July 23rd, 1995, Daniel Green of the Harvard Smithsonian Astrophysical Observatory telephoned and said, Congratulations Tom, I believe you discovered a new comet. And that was one of the happiest moments of my life.
Thomas Bopp lives in Glendale, Arizona. (Small suburb just barely outside Phoenix) He is the supervisor for a construction material company in Phoenix. Bopp is an enthusiastic observer of deep sky objects. The exact name of the site Bopp saw the comet at is Vekol Ranch.
Since they discovered the comet within minutes of each other the comet was named the Hale-Bopp Comet.
Nobody knows the exact orbital period of the comet but it is believed to be a little over 3000 years. It has passed through our solar system before (that is, it is not a new comet from the Oort Cloud)
On April 1, 1997, the comet is expected to reach its closed point to the sun. At this time it will also be most visible because the sun reflects off the tail of the comet.
Although the comet will be closest to the sun on April 1, it will be closest to the earth on March 23, 1997. Some people have been saying that the comet will hit earth and cause human extinction, just like the dinosaurs. The fact is, however, THE COMET WILL NOT HIT EARTH. The closest it will come is 120 million miles away from the earth.
Some people are saying that the comet is going to Be huge, and others say it will be small. We will never know though because we can not see the nucleus of a comet. The part of the comet we see is the tail. The tail of a comet can be over 10,000 kilometers long.
In all, comets, the history of comets, and comets waiting to be discovered is very interesting. I think that one day we will get to see the nucleus of a comet, and be able to watch comets form in the Oort Cloud.