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Abstract Comets—big lumps of rock, ice, and frozen gases that orbit the Sun—are among the most amazing heavenly objects seen in the night sky. The glowing tail behind the comet's nucleus inspires wonder. But did you know that a comet's tail is evidence that it's melting? As a comet passes by the Sun on its orbital path, it starts to melt. But do bigger comets melt faster than smaller comets? In this astronomy science project, you will investigate how the size of the comet affects the rate at which it melts and by how much.Objective To model comets using ice forms and determine how weight affects the rate of melting. Introduction A comet streaking across the sky, its tail stretching behind, is an amazing sight. Because comets are not visible all the time, they are usually special and even spectacular for people on Earth. In olden times, comets were considered as both good and bad omens. But what is a comet? Where do comets come from? And what is a comet made of? A comet is basically a "dirty snowball" of dust and sometimes rock, frozen water, and frozen gases like ammonia, methane, carbon monoxide, and carbon dioxide. Comets travel in an orbit; a short orbital-period comet is one that takes 200 years or less to go around the Sun, and a long orbital-period comet takes more than 200 years—often thousands or even millions of years. Halley's Comet is a short orbital-period comet that can be seen from Earth every 75 to 76 years. Comet Hale-Bopp, which was visible to the naked eye for 18 months spanning 1996 and 1997, is a long orbital-period comet that won't be visible from Earth again for several thousand years. Short orbital-period comets are thought to originate from the Kuiper Belt, while long orbital-period comets are believed to be from the Oort Cloud. The Kuiper Belt lies beyond the planet Neptune (between 30 astronomical units [AU] and 55 AU from the Sun), and the Oort Cloud, which is thought to be a spherical cloud surrounding the solar system, lies about 50,000 AU from the Sun. Objects in the Oort Cloud are made up of frozen water, frozen ammonia, and frozen methane. Comets are made up of a nucleus, a coma, and a tail, as shown in Figure 1 below. A comet's nucleus can range from hundreds of meters to tens of kilometers across.
Occasionally, the gravitational influence of one of the outer planets or, in the case of the Oort Cloud, the gravitational influence of nearby stars, causes a comet to enter an elliptical orbit that carries it closer to the sun. The nucleus is volatile because it is made up of unstable matter that evaporates easily. As the comet orbits closer to the Sun, solar radiation—the energy that the sun gives out—begins to melt the nucleus and causes the volatile material and dust to come out. (We also feel solar radiation, in the form of sunlight, on our skin.) The dust surrounds the nucleus to form the coma. Solar winds push the melted material away from the nucleus, causing the tail to form. Some comas can be nearly a million kilometers wide while tails can be more than 100 million kilometers long. Later, when the comet moves away from the Sun to the outer solar system and beyond, the coma and tail disappear and the nucleus remains frozen. Figure 2 below shows a comet as seen through a telescope. Sometimes, we can see comets from Earth without telescopes when they pass close to the Sun because their tails and comae reflect sunlight.
As a comet travels towards the Sun, how does it melt? Do bigger comets melt faster than smaller comets? In this astronomy science project, you will model comets of different sizes and then use a hair dryer as a heat source (to mimic the Sun and other "warm" planetary objects) to determine how the size of a comet affects melting. Terms, Concepts, and Questions to Start Background Research
Questions
Bibliography
Materials and Equipment
You will also need to purchase, or borrow from your science teacher, these pieces of laboratory equipment. Or, with a little bit of problem-solving, you may find a way to rig up your own way of hanging the comets rather than using the support stand and ring clamp.
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| Comet | Trial | Amount of Water Melted into Pot (in Milliliters) |
| Large
(350 ml) |
1 | |
| 2 | ||
| 3 | ||
| Small
(250 ml) |
1 | |
| 2 | ||
| 3 |
| Table 1. Milliliters of melted water for large and small comets |
Comet |
Average Amount of Water Melted into Pot (ml) |
Percentage Comet Melted (%) |
| Large (350 ml) |
||
| Small (250 ml) |
| Table 2. Average amount of water melted in large and small comets and its percentage in terms of the total amount of water |
| Average = | X1 + X2 + X3 3 |
| Percentage Comet Melted (%) = | Average Amount of Water Melted Amount of Water in Comet |
× 100 |
Variations
Credits
Michelle Maranowski, PhD, Science Buddies
This project is based on one of the Science Buddies – Lick Observatory Astronomy Contest winning projects: Boulos, Bassam N. (2011). "Comets"
Last edit date: 2011-11-21 12:00:00
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