Newly-discovered Comet ZTF is coming the closest to the Earth in 50,000 years, becoming visible to the naked eye, and making big headlines. Some are calling it a “super rare” and “bright green” comet, but will it live up to the hype? We explain.
Comet ZTF was discovered on March 2, 2022 by a robotic camera attached to a telescope known as Zwicky Transient Facility (ZTF) at the Palomar Observatory in Southern California. ZTF scans the entire northern sky every two days and captures hundreds of thousands of stars and galaxies in a single shot. Many comets have been found with this instrument. The most recent is catalogued as C/2022 E3 (ZTF), Comet ZTF for short.
Comet ZTF has travelled a distance of 2.8 trillion miles and will make its closest approach to the Earth in 50,000 years on February 1, 2023. Orbital computations suggest that Comet ZTF may never return again.
The greenish color is likely due to a molecule made from two carbon atoms bonded together, called dicarbon. This unusual chemical process is confined chiefly to the head, not the tail. If you get a look at Comet ZTF, that greenish hue is likely to be quite faint (if it is visible at all). The appearance of green comets due to dicarbon is fairly uncommon.
Recent images show the head (coma) appearing to be distinctly green and trailed by an impressively long thin blush appendage (the tail). But that is what a camera taking a long exposure sees. The tint will look much less green to the naked eye.
During the latter part of January into early February, ZTF may become bright enough to be glimpsed with the naked eye. Use a reliable star map to track the night-by-night change in position relative to the background stars and constellations. Here are dates and approximate locations.
Look towards constellation Corona Borealis before sunrise.
Look towards constellation Boötes before sunrise.
The comet will be visible in the night sky (previously only visible in the early morning hours). Look north, above and to the left of the Big Dipper.
Look near the constellation Draco (The Dragon).
Look several degrees to the east of the bowl of the Little Dipper. On the evening of the 27th, it will be about three degrees to the upper right of orange Kochab, the brightest of the two outer stars in the Little Dipper’s bowl.
Look towards Polaris.
Look near the constellation Camelopardalis.
Look towards the brilliant yellow-white star Capella (of the constellation Gemini).
Look within the triangle known as “The Kids” star pattern in Auriga, directly overhead at around 8 p.m. local time.
Look two degrees to the upper left of Mars.
Note: If you live in a big city or an outlying suburb, sighting this comet is going to be a difficult—if not an impossible task. Even for those who are blessed with dark and starry skies, finding ZTF could be a bit of a challenge.
As for the tail, comets can shed two types, composed of dust and gas. Dust tails are far brighter and more spectacular to the eye than gas tails, because dust is a very effective reflector of Sunlight. The most spectacular comets are dusty and can produce long, bright tails making them awesome and impressive celestial spectacles.
Gas tails on the other hand appear much fainter and glow with a bluish hue. The gas is activated by the ultraviolet rays of the Sun, making the tail glow in much the same way that black light causes phosphorescent paint to light up. Unfortunately, gas tails produced by most comets, appear long, stringy thin, and quite faint; impressive in photographs but underwhelming visually. And that’s what we’re currently seeing with ZTF.
Finally, when the ZTF is at its brightest in late January and early February, it’s going to have to compete with another celestial object: the Moon. During that same time frame, the Moon will be near full phase (The Full Snow Moon is on February 5th). Blazing in the night sky like a giant spotlight, the full Moon will make trying to see a relatively dim and diffuse object like Comet ZTF even more difficult.
There are nearly a dozen comets available to be viewed in tonight’s night sky. Most of these, however, are visible only with moderately large telescopes. You also would need a good star atlas as well as accurate coordinate positions in order to know where to point your instrument to actually see any of these. Most amateurs who make it a point to search them out call such comets “faint fuzzies” because that’s pretty much what they look like through the eyepiece: A faint, fuzzy blob of light. These are known as “common comets.”
Every once in a while, perhaps two or three times over a span of 15 or 20 years, a bright or “great comet” will come along. These are the types that excite those of us without binoculars or telescopes—the type where all you need do is step outside, look up and exclaim: “Oh look at that!” Such comets tend to be much larger than average. Most of these have a core or nucleus less than two or three miles across. But there are others than can be up to several times larger.
As a general rule, the closer a comet comes to the Sun, the brighter it gets. Large ones that sweep closer than Earth’s distance from the Sun (92.9 million miles) tend to get quite bright. Good examples are Comet Hale-Bopp in the spring of 1997 and Comet NEOWISE (discovered with a robotic space telescope) in the summer of 2020.
So which category does ZTF fall into? In many ways it’s pretty much a common comet, but compared to most of the other faint fuzzies, ZTF is extremely bright.
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Will you look to the sky for “green” comet ZTF?
Let us know in the comments below!
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