Currently in orbit within the inner regions of the solar system is comet 12P/Pons-Brooks, also known as Pons-Brooks, which is making its first appearance in over 70 years and is expected to be visible without the aid of telescopes soon. This massive ice chunk, roughly 30 kilometers (19 miles) in diameter, is comparable in size to Mount Everest and is considered one of the brightest known periodic comets by astrophysicists. Pons-Brooks, classified as a Halley-type comet, has an orbit around the Sun of 71.3 years and was last observed in the sky in 1954. Discovered in 1812 by Jean-Louis Pons and later confirmed in 1883 by William Robert Brooks, this is the first recorded sighting of the comet dating back to 1385.
When is Comet 12P/Pons-Brooks Visible?
Comet 12P/Pons-Brooks is currently visible and will remain so until April 21, 2024, with optimal viewing conditions expected towards the end of March. With binoculars or a small telescope, the comet is already observable in the sky, particularly when the Moon is located in the west below the Andromeda Galaxy moving through Pisces. By the end of the month, the comet will pass near the brighter stars in Aries, moving in the direction of Jupiter. As its brightness increases towards the end of the month, it may become visible to the naked eye under clear, dark skies. On March 31st, Pons-Brooks will be just 0.5 degrees away from a bright star named Hamal, which is equivalent to the diameter of the full moon, according to Strom. Those having trouble locating these constellations can benefit from downloading a stargazing app. For residents of the United States, the comet may also be visible in the sky during the total solar eclipse on April 8, 2024. Following its closest approach to the Sun on April 21, Pons-Brooks will fade and become visible only to observers in the southern hemisphere.
Why the Name “Devil’s” Comet?
The recent sighting of Pons-Brooks is not its first appearance in recent times. Referred to as the “Devil’s Comet,” due to a peculiar outburst in July 2023 that led to a temporary brightening resembling devil horns, Pons-Brooks is classified as a cryovolcanic comet that sporadically erupts, expelling dust, gas, and ice into space. These eruptions are triggered by the comet warming up as it nears the Sun, resulting in increased pressure causing the release of icy material from beneath the surface of the comet. The gas forms a bright coma, a halo of evaporated material surrounding the solid core of the comet. Comets appear brightest when closest to the Sun due to sunlight reflecting off the evaporated material, with the tails formed by interaction with charged particles from the solar wind. Pons-Brooks experienced similar but less intense outbursts on various dates in recent months, contributing to its brightness when close to the Sun.
What Does “12P” Mean?
The designation “12P” in the comet’s name indicates that it is the 12th comet discovered within a set period. Baskill explains that long-period comets, originating from the edge of the solar system, may have orbits lasting thousands or even tens of thousands of years, while short-period comets like Pons-Brooks return to the inner solar system in less than 200 years. Notable short-period comets include Comet Halley, with a period close to that of Pons-Brooks, expected to return in 2061. Current estimations suggest there are around 3,910 known comets in total, but astronomers believe there could be up to 1 trillion comets within our solar system.
Upcoming Comets
Expect to observe Comet 13P/Olbers in June and July, with observers in the Northern Hemisphere likely to spot it using binoculars. This comet, also known as a Halley’s Comet, orbits the Sun every 69 years. In late 2024, Comet C/2023 A3 is predicted to enter the inner solar system, potentially showcasing exceptional brightness in September and October, comparable to the brightest stars and potentially earning the title of “Great Comet.”
About Our Experts:
Dr. Paul Strom serves as an Assistant Professor within the Astronomy and Astrophysics Group at the University of Warwick, focusing on the PLATO space mission and various astrophysical topics, particularly far-ultraviolet observations to understand the environments where young planets form. His research paper titled “Exo-solar Comets from a Solar System Perspective” was published in the journal Publications of the Astronomical Society of the Pacific.
Dr. Darren Baskill is an outreach officer and lecturer at the University of Sussex’s School of Physics and Astronomy. Previously involved with the Royal Observatory Greenwich, he organized the annual Astronomical Photographer of the Year competition.
