This site uses cookies to offer you a better browsing experience. Read about how we use cookies.
The most famous comet of all, Halley’s Comet, returns to the inner Solar System about every 76 years. It was last seen in 1986 and will be back in 2061. To discover this icy visitor, its bright head and its long tails, let’s build a tactile version using cheap, household items. Just like the other activities of the “Meet our Neighbours” series, the tactile Halley’s Comet will be a great resource to explore a comet for both visually impaired and sighted students.
NOTE: The "Meet our neighbours!" project is published in AstroEDU in this activity Collection. It was produced by NUCLIO and Europlanet and supported by Galileo Teaching Training Program and GalileoMobile. You can find more information at this Link
For each group bulding a tactile comet:
NOTE: These materials are only suggestions; all textures can be replaced by other local, easy to find, low-cost materials.
Image: The two files to download
To explore Comet Halley through a tactile hands-on experience for visually impaired students and their non-visually impaired peers.
Students will explore and learn the characteristics of Comet Halley (and other comets): the nucleus, the coma and the 2 tails.
General information
Comets are small objects that orbit the Sun at very large distances, hundreds to thousands of times the Sun-Earth distance. They are believed to form a huge cloud, called the “Oort cloud”, around the solar system. Some of these comets may be dislodged from their distant location by the gravitational influence of Jupiter, and their new orbits take them on a long journey across the solar system.
Most of the comets that enter the solar system never come back for a second visit, but some become periodic comets, with periods that vary from less than 200 years (short-period comets) to thousands of years (long-period comets). In the case of Halley’s comet, it’s very elongated orbit takes it as far as 5250 million kilometres and as close as 87 million kilometres from the Sun over a period of 75.3 years.
A Comet seen from close
Physically, a comet nucleus is a solid body made of dust and ice . When it gets close to the Sun, the ice that makes up most of the nucleus begins to ‘vaporize’ and forms a “coma” (from the Latin word for “hair”) . Even closer to the Sun, solar radiation pushes gas and dust particles out of the coma; these particles form a dust tail that can extend millions of kilometres into space. This tail is often curved because it takes the shape of the comet’s orbit. The gas can also be ionized by solar radiation, and the charged molecules and atoms then develop an “ion tail” that is straighter than the dust tail and always directed in the direction opposite to the Sun.
Image: the different parts of a comet. Credits: ESA
Why are comets important?
Comets are leftovers from the formation of the Solar System, about 4.6 billion years ago. They have spent most of their lives far from the Sun, so their ices and dust have changed very little. Studying them is like opening a time capsule: they tell us what the Solar System was made of when the planets were born. Comets may also have helped bring water and organic molecules to the young Earth, although scientists are still debating how much. Finally, comets leave trails of dust along their orbits. When Earth crosses these trails, we see meteor showers. Halley’s Comet is the parent of two of them: the Eta Aquariids in May and the Orionids in October.
Halley's Comet story
Halley is the most famous comet: its passages have been recorded by astronomers since at least 240 BC, but they were not recognized as periodic visits by the same object. It was only in 1705 that the British astronomer Edmond Halley determined that the orbit of a comet that appeared in 1682 was the same as the orbit of two earlier comets that were observed in 1531 and 1607. He was the first to realize that these three comets were, in fact, three successive passages of the same comet, with a periodicity of about 76 years. He then predicted the return of the comet in 1758, a prediction that proved correct when the comet passed near the Sun in March 1759. In recognition of his work, the comet was given his name. Halley’s Comet last passed close to the Sun in February 1986. Its next return is expected in July 2061. In December 2023 it reached the farthest point of its orbit, beyond Neptune, and it is now on its way back towards us.
Image: Comet 1P/Halley as taken March 8, 1986 by W. Liller, Easter Island, part of the International Halley Watch (IHW) Large Scale Phenomena Network.
Step 1Cut the section on Tactile_Comet_Mold and with a pen outline the cut section on in the thick fabric;
Step 2Cut the thick fabric accordingly to the area outlined;
Step 3Place abundant glue on the area that correspond to the inner side of the comet’s surface on the Tactile_comet file and place the fabric on top of the glue;
Step 4Place the thick fabric on top of the glue;
WAIT FOR THE IMAGE TO DRY.
Step 5Place glue in the curved areas around the thick fabric and place sand on top of the glue;
Step 6Place glue in the thick wavy areas correspondent of the upper tail and place sand on top of the glue;
Step 7Place glue in the thin wavy area corresponding to the lower tail and place sand on top of the glue;
WAIT FOR THE IMAGE TO DRY. IT MIGHT TAKE A WHILE BEFORE YOU CAN EXPLORE THE IMAGE.
There are several ways in which you can explore the scientific content of the tactile schematic images. If you’re presenting the final tactile image to the students, first let them explore and feel the different textures. Questions will arise as the students explore; encourage them to write their questions down and share them with the other groups. Read “Background Information” to understand the different features present in the Comet schematic tactile image, and share with the students as they ask about them, or (if you have more time), prompt each group to choose a feature to learn more about and then have them present to the other groups in the class.
In the image above, you can identify the following features:
(1) Halley’s comet nucleus materialized by the round patch of fabric on the tactile image(2) the coma: when the comet gets close to the Sun, the ice that makes up most of the nucleus begins to ‘vaporize’ and forms it. It is materialized by glued-on sand on the tactile image(3) the dust tail materialized by glued-on sand extending from the coma. It forms even closer to the Sun, when solar radiation pushes gas and dust particles out of the coma. This tail is often curved because it takes the shape of the comet’s orbit. (4) The gas can also be ionized by solar radiation, and the charged molecules and atoms then develop an “ion tail” materialized by the straw on the tactile image that is straighter than the dust tail and always directed in the direction opposite to the Sun.
Call out a feature of the comet (the nucleus, the tails or the coma). For each feature give a brief description. e.g. - This forms when this object gets near the Sun (Answer: the Great Red spot).
Ask the class to suggest how Comets are important for Humankind and why.
Find the original project "Meet Our Neighbours" at https://ark.nuclio.org/astroneighbours/
Europlanet Outreach, Núcleo Interactivo de Astronomia