A comet is a small, icy celestial body that orbits the Sun. s are typically composed of frozen gases, such as carbon dioxide, methane, and water, and rock. When a comet approaches the Sun, the heat from the Sun causes the gases to sublimate and form a tail. The tail always points away from the Sun, and it can be several million kilometers long.

Structure of a

s are divided into two main parts: the nucleus and the coma. The nucleus is the solid, central part of the comet, and it is typically only a few kilometers in diameter. The coma is the fuzzy cloud of gas and dust that surrounds the nucleus. The coma can be several hundred thousand kilometers in diameter.

Orbit of a

s orbit the Sun in a highly elliptical path. This means that they spend most of their time far from the Sun, and they only come close to the Sun every few hundred or thousand years. The orbital period of a comet is the amount of time it takes for the comet to complete one orbit around the Sun. Orbital periods can range from a few years to several thousand years.

Types of s

There are two main types of comets: short-period comets and long-period comets. Short-period comets have orbital periods of less than 200 years, while long-period comets have orbital periods of more than 200 years. Short-period comets are thought to originate in the Kuiper Belt, which is a region of icy bodies that lies beyond the orbit of Neptune. Long-period comets are thought to originate in the Oort Cloud, which is a vast cloud of icy bodies that surrounds the solar system.

Notable s

Some of the most famous comets in history include:

Halley’s is a short-period comet that has been observed by humans for thousands of years. It has an orbital period of 76 years, and it last appeared in 1986.
Hyakutake was a long-period comet that was discovered in 1996. It had a very bright tail, and it was visible to the naked eye for several months.
Shoemaker-Levy 9 was a comet that collided with Jupiter in 1994. It was the first time that a comet had been observed colliding with a planet.

s and Life on Earth

s have been hypothesized to have played a role in the origin of life on Earth. s are thought to have delivered water, organic molecules, and other essential ingredients to the early Earth. These ingredients may have helped to create the conditions necessary for life to begin.

Frequently Asked Questions (FAQ)

What is a comet made of?

s are composed of frozen gases, such as carbon dioxide, methane, and water, and rock.

How big is a comet?

The nucleus of a comet is typically only a few kilometers in diameter, but the coma can be several hundred thousand kilometers in diameter.

How often do comets visit the Sun?

Short-period comets visit the Sun every few hundred or thousand years, while long-period comets visit the Sun every few thousand or million years.

What is the most famous comet?

Halley’s is the most famous comet in history. It has been observed by humans for thousands of years, and it last appeared in 1986.

Have comets ever collided with Earth?

There is no definitive evidence that a comet has ever collided with Earth, but some scientists believe that comets may have been responsible for some of the mass extinctions in Earth’s history.

References

Names

s are named using a system established by the International Astronomical Union (IAU). The naming convention consists of two parts:

Prefix: This indicates the discovery type of the comet. Common prefixes include:
- C/: Non-periodic comets
- P/: Periodic comets
- X/: s whose orbits are not well-determined
- D/: s that have broken up or become inactive
Number: The year of the comet’s discovery is followed by a lowercase Roman numeral assigning it a unique designation within that year. For example, "C/2023 E3" refers to the third non-periodic comet discovered in 2023.

If a comet is named after its discoverer, a letter or letters representing that person’s name may be added after the number. For example, "C/1995 O1 (Hale-Bopp)" is named after its discoverers, Alan Hale and Thomas Bopp.

s may also receive additional names or designations, such as:

Orbital period: The time it takes for the comet to complete one orbit around the Sun.
Orbital eccentricity: A measure of how elliptical a comet’s orbit is.
Perihelion: The point in the comet’s orbit closest to the Sun.

Neowise

Neowise (C/2020 F3) is a comet that was discovered in March 2020 by NASA’s Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) space telescope. It is the brightest comet observed from Earth since Hale-Bopp in 1997.

Neowise passed its closest point to the Sun (perihelion) on July 3, 2020, and made its closest approach to Earth on July 22, 2020. It was visible to the naked eye in the northern hemisphere during July and August 2020. Observers noted its bright tail, which extended across the sky for several degrees.

Neowise is a member of the Kreutz sungrazing family of comets, which are believed to have originated from a single parent comet that broke up thousands of years ago. The comet is estimated to have a nucleus of about 5 kilometers (3 miles) in diameter and a mass of about 10 billion tons.

Hale-Bopp

Hale-Bopp was a spectacular comet discovered in 1995 that became one of the brightest and most visible comets in recorded history. It was named after its discoverers, Alan Hale and Thomas Bopp.

Hale-Bopp was a large, long-period comet, estimated to be 40 kilometers (25 miles) in diameter. It originated from the Oort Cloud, a distant region of the solar system, and had an orbital period of 2,300 years.

The comet’s approach to the sun, and its subsequent appearance in the night sky, captured the attention of the public worldwide. It was visible to the naked eye for 18 months and put on a spectacular display with its bright nucleus and a distinctive dust tail that stretched across multiple constellations.

Hale-Bopp provided valuable scientific data and insights into the nature of comets and the early formation of the solar system. Its prolonged visibility and vivid appearance left a lasting impact on the human fascination with celestial objects.

Hyakutake

Hyakutake (C/1996 B2) was a spectacular comet that graced the skies in early 1996. Discovered by Japanese amateur astronomer Yuji Hyakutake, the comet rapidly brightened and developed a prominent tail visible to the naked eye.

Hyakutake made its closest approach to the Sun on March 25, 1996, at a distance of about 0.1 AU. During this time, it displayed a magnificent tail that stretched millions of kilometers into space. The tail featured a distinctive blue ion tail and a yellowish dust tail.

The comet’s close proximity to Earth allowed astronomers to study it in great detail. Observations revealed that Hyakutake was a complex body composed of a rocky core surrounded by an icy mantle. The comet’s nucleus was estimated to be about 4 kilometers in diameter, while its coma reached a width of over 100,000 kilometers.

Hyakutake’s appearance was a breathtaking sight for observers worldwide. It became one of the most visible comets in recorded history, inspiring awe and wonder in people around the globe. The comet’s passage also provided valuable scientific insights, contributing to our understanding of these celestial objects.

Shoemaker-Levy 9

Shoemaker-Levy 9 was a comet that collided with Jupiter in July 1994. The comet was originally discovered in 1993 and was found to be a series of fragments. It is thought that the comet had been broken up by the gravitational pull of Jupiter during a previous close encounter with the planet.

The impact of Shoemaker-Levy 9 on Jupiter was a major event. The comet fragments created a series of large dark spots on the planet’s surface, and the impact also caused a large amount of dust and gas to be ejected into the atmosphere. The impact was observed by telescopes around the world, and it provided scientists with valuable information about the composition and structure of Jupiter.

Tempel 1

Tempel 1 is a Jupiter-family comet with a nucleus approximately 7.6 kilometers in diameter. It was discovered by Wilhelm Tempel on April 3, 1867, and has been observed closely by several space missions, including Deep Impact in 2005 and Stardust-NExT in 2011. Deep Impact’s impactor spacecraft released a copper projectile into the comet’s nucleus, creating a crater and ejecting material that was collected by the spacecraft’s flyby probe. Stardust-NExT flew by the comet and collected samples of its coma, providing valuable insights into its composition and history. Tempel 1 is a notable object of scientific study, offering clues to the early formation and evolution of the solar system.

Halley

Halley is a periodic comet that orbits the Sun every 76 years. It has been observed and recorded throughout history, with the earliest known sighting dating back to 240 BC. Halley is named after the English astronomer Edmond Halley, who predicted its return in 1705.

The comet is known for its bright, white tail, which can be seen from Earth with the naked eye. It is composed of frozen gases, such as carbon monoxide, methane, and water vapor, which sublime as the comet approaches the Sun. The tail can extend for millions of miles and is always pointed away from the Sun.

Halley’s last perihelion (closest approach to the Sun) was in 1986, and its next perihelion will be in 2061. The comet’s orbit is highly elliptical, and its distance from the Sun varies between 0.9 AU and 35 AU.

McNaught

McNaught, also known as the Great of 2007, was a long-period comet that was visible to the naked eye in early 2007. Discovered in August 2006 by Australian astronomer Robert McNaught, the comet reached its peak brightness in January 2007 and was visible in both the Northern and Southern Hemispheres. The comet’s distinctive blue-green tail, which spanned over 100 million kilometers, made it one of the most spectacular celestial events in recent years.

ISON

ISON (C/2012 S1) was a sungrazing comet that was discovered in 2012 and attracted wide attention due to predictions that it could become extremely bright when it passed close to the Sun in 2013.

The comet originated from the Oort cloud and was estimated to be about 500 meters wide. As it approached the Sun, it developed a massive tail and was expected to produce a bright coma, potentially becoming visible in broad daylight.

Hartley 2

Hartley 2 is a periodic comet with an orbital period of about 6.5 years. It was discovered in 1986 by Malcolm Hartley. The comet has a nucleus of about 1 kilometer in diameter and a coma of about 10,000 kilometers in diameter. It is made up of dust and ice. The comet was visited by the Deep Impact spacecraft in 2010. The spacecraft took images of the comet’s nucleus and released a probe that impacted the comet. The probe sent back data about the comet’s composition.

Siding Spring

Siding Spring, also known as C/2013 A1, is a non-periodic comet that made a close approach to the Sun and Mars in October 2014. Discovered in January 2013, it is estimated to be around 2.5 miles (4 kilometers) in diameter.

On October 19, 2014, Siding Spring passed within 87,000 miles (140,000 kilometers) of Mars, the closest cometary approach to a planet ever recorded. The comet’s tail and dust trail interacted with Mars’ atmosphere, creating a bright aurora and offering scientists unique insights into the planet’s magnetic field and upper atmosphere.

Siding Spring is not believed to be a threat to Earth, as its orbit does not intersect with our planet’s. However, it remains an object of scientific interest due to its unusual characteristics and its role in providing valuable data about the interplanetary environment and the history of the solar system.

Borisov

Borisov (C/2019 Q4 Borisov) is the first known interstellar comet discovered in our Solar System. Discovered by Gennady Borisov in August 2019, it is the first interstellar object known to originate from outside our Solar System and the second to be observed within it, after ‘Oumuamua in 2017.

Borisov entered the inner Solar System in December 2019 and was closest to Earth in December 21, 2019. It passed its closest point to the Sun in early December 2020 and is now moving away from the Sun and out of the Solar System.

Borisov is composed of a mixture of water ice, carbon dioxide, and other organic compounds. It was estimated to be about half the size of ‘Oumuamua, with a diameter of about 2 kilometers. The comet’s surface was dark and dusty, and it showed no signs of activity such as jets of gas or dust.