PHOTOS OF THE SOLAR SYSTEM AND THE UNIVERSE FROM MY BACKYARD
Comets
Comets are icy/rocky bodies (usually a few kilometers in size) that originate from the regions beyond Neptune; remnant material from the formation of our solar system. Their characteristic wispy tails are formed as some of their icy crust and dust boils off as they heat-up as they fall inward through our solar systems toward the Sun. Some comets have established stable orbits around the Sun and return periodically (ie Halley’s Comet every 86 years) while others make a one-time passage through our solar system as they whip around the Sun and are then flung outward with sufficient velocity never to return. What we see as meteors is the earth traveling through the dust and debris trail left behind by comets, the dust particles burning up as they impact the earth’s atmosphere.
Many people seem to confuse comets with meteors in the sense that they think that cometary appearances are very fleeting events. While this is certainly true of meteors where they literally come and go in the blink of an eye, Comets are much more lasting events, which can be viewed for weeks if not months with the aid of binoculars or small telescopes. There are usually a half-dozen or more comets every year that are viewable to the enterprising observer, and every few years there is a comet that brightens to the naked-eye visibility and garners much publicity.
Comets are usually identified by the year they are first observed and the name of the Observatory, Facility or person that made the discovery. So for the case of Comet 2023 A3 Tsuchinshan-ATLAS, it was co-discovered in 2023 by the Tsuchinshan Observatory in China and the ATLAS (Asteroid Terresestrial-impact Last Alert System) early-warning system.
The “A3” designates the month the comet was discovered. Each month is split in half with “A” being the first-half of January and “B” the second-half while “C” is the first-half of February and “D” is the second-half, and so on (with “I” not being used). The number designates the order in which the Comet was discovered in that particular half-month period. Thus “A3” means that this comet was the third comet to be discovered in the first-half of January 2023.
If the comet has a “P” designation it means that it is a “Periodic Comet” – one that has previously been observed with a well defined orbit. Halley’s Comet “1/P Halley“ which appears every 72-80 years is the best known example of a periodic comet.
In regards to the published magnitude values for Comets, and for that matter all extended objects such as Nebulae and Galaxies, the magnitude values are integrated values. That means the brightness is calculated on the total light emitted (or reflected) over its entire surface area. For stars the light is emitted from a single concentrated point while for extended objects, like comets, it includes not only the bright nucleus but also the extended tail – if any. Thus a comet or galaxy may appear dimmer than the published magnitude value might suggest as the total emitted light is spread over a larger area.
Below are photos of some of the comets I have observed over the years and many of the photos show what can be achieved using nothing more than a simple camera or cellphone.
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For the better part of a year the approach of comet C/2023 A3 Tsuchinshan-ATLAS has been eagerly anticipated as it was projected to reach “Naked Eye” visibility. As shown in the photos below it didn’t disappoint and is the best “Naked Eye” comet since Comet NEOWISE in 2020 and is being called the most photographed comet in history.
At the time of this photo the Comet was faintly visible to the naked eye under less than ideal conditions – a waxing moon and clouds – but showed up easily in binoculars and photos. This photo was taken from Daniels Park, CO at 7:50 pm MDT looking West. 40-150mm lens – f5 – ISO 3200 – 10 sec.
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A close-up view. * * *
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The comet a day later under much clearer skies but having to compete against a full Moon. * * *
A close-up photo of the comet shining at magnitude +3.7 and also shows the faint “Anti-Tail” projecting downward from the head. Photo is from a stack of 11 frames – 82mm – f5.6 – ISO 3200 – 8 second exposures. * * *
This composite photo shows the position of the comet at 8:00 pm MDT on Oct 15 & Oct 17 from my viewing location at Daniels Park Colorado. The reduced size/visibility of the comet on the 17th was to some extent due to the increasing brightness of the Moon between these dates. * * *
By this date the comet was high enough to appear above the trees blocking my view of the western horizon so that I could get some long exposure photos from my observatory. This photo was taken through my 80mm ED refractor and is from a stack of five frames – ISO 3200 – 20 second exposure. At this point the magnitude of the comet was +5.4, near the limit of naked eye visibility from a dark site. * * *
By this date the comet finally reach an altitude during the early evening where it cleared the trees surrounding my permanent pier allowing me to get some longer exposure photos. This photo was taken with my C80 ED scope: 5 frames – ISO 3200 – 20s * * *
Taken through my C9 @ f6.3 – 6 frames x ISO 3200 x 30 seconds * * *
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Here is an early view of Comet 2023 A3 Tsuchinshan-ATLAS on its Sun-ward journey. At a distance of 1.77 AU from the Earth it is shining at magnitude 9.6 and already displaying a significant tail. At its closest approach to the SUN in October of 2024 it is predicted that it will brighten to Magnitude 1.0 which would make it easily visible to the naked eye. * * *
Another photo of Tsuchinshan-Atlas a month later than the photo above. * * *
Comet 12/P was discovered in 1812 by Jean-Louis Pons and William Robert Brooks. It has an orbital period around the Sun of 71 years. * * *
The periodic comet 62P/Tsuchishan was first discovered in 1965. Its orbit ranges from 1.265 AU (just beyond that of earth) to 5.5 AU (just beyond Jupiter at 5.2 AU) with an orbital period of 6.2 years. The photo above was taken in the early morning (5 am local time) and remained visible in the Northern Hemisphere through mid-February 2024. * * *
Comet 2022 E3 is projected to reach a maximum brightness of mag 5 around February 5th which would make it a naked eye object under dark skies. The photo above was taken through my C9 telescope with the comet shining at ~ mag 7.5. Its closest approach to earth in 2024 occurred on January 29 at a distance 0.28 AU.
This photo shows the comet near its maximum brightness of magnitude 5.5 and was taken with my Olympus E-M10 Mark II digital camera and a 45mm lens. Comet C/2022 E3 reached Perihelion (its closest approach to the Sun) on January 12, 2023 and in this photo the comet is moving toward its closet approach to earth which occurred on February 1. If you look closely you can see a faint “Anti-Tail” streaming downward from the head of the comet.
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Discovered in March 2020 by the NEOWISE space telescope, the comet F3 NEOWISE was somewhat of a surprise, brightening to naked-eye visibility in early July 2020.
Another view of the comet 6 days later. The sky is a bit grey due to a thin cloud layer reflecting the city lights from Denver.
A closer view of Comet NEOWISE taken with a 300mm lens
Photo is 10 frames x 3sec @ ISO 1600. 90mm lens @ f2, cropped. I did a plate solve and measured the length of the tail as extending 5 degrees – a very conservative measurement I’m sure.
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First discovered in 1889, 64P Swift-Gehrels is a faint periodic comet with a period of 9.23 years. For its 2018 appearance it reached a peak magnitude of 9.0 and passed within 0.45 AU of Earth on October 18.
Comet Giacobini-Zinner – This relatively faint comet (magnitude 8.0) was photographed through my C9.25 telescope. A time-lapse video of the motion of this comet can be found in the “Video” section of this website.
Comet Wirtanen, (diameter = 0.75 miles) orbits between Earth and Jupiter with a period of 5.44 years. This photo was taken just 12 days before its closest approach to Earth (7.3 million miles on Dec 16) using a digital camera and 100mm zoom lens. The field-of-view of the photo is approximately 4 degrees square.
Comet Wirtanen four days later – the comet is noticeably brighter from the earlier photo as it approaches the Sun.
Close-up view taken through my Celestron C9.25 scope. The green color is from ultraviolet light emitted by the Sun reacting with the molecular carbon compounds (C2) found in the comets icy core. Comets move relatively quickly as they approach the Sun and usually when viewed through a telescope their movement can be noted over the course of several minutes or hours. The above photo is an example of multiple exposures being combined and centered on the image of the comet. The individual dots are the stars in the field-of-view for each exposure and show just how quickly the comet moves relative to the background stars over the course of several minutes. * * *
A composite photo of comet Wirtanen taken the day before the comet reached the point of its closest approach to earth (7.3 million miles). At this date the comet had already made its closest approach to the Sun three days earlier and is now heading back out toward the outer reaches of its orbit – beyond the orbit of Jupiter. The photo shows the comets’ movement over a two hour period near the Pleiades Star Cluster.
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Comet PanSTARRS at sunset viewed from an overlook at Castle Pines. Faintly visible to the naked eye this photo was taken using a digital camera on a tripod. Exposure time: 6 seconds.
Comet Hale-Bopp (1997) taken with my Pentax SP500 35mm SLR camera and a 50mm f2.0. Note the twin tail – the light blue tail is an ion tail of charged particles while the white tail is formed from ice & dust. You can see the star trails due to the time exposure.
Comet Hale-Bopp (1997) taken with a SLR film camera & 50mm lens. This view is looking North towards Denver.
Comet Hale-Bopp (1997) taken with my SLR film camera – this time looking West. * * *
Comet Hyakutake – officially comet C/1996 B2 (Hyakutake) – was discovered on January 31, 1996 shining at magnitude 11.0 and quickly brightened to naked eye visibility by early March. Hyakutake was fast moving and reached its closest approach to Earth (0.1AU) on March 25. The photo above was taken two days later using my Pentax SP500 35mm SLR camera and a 50mm f2.0 lens from my backyard looking over the roof of my house. I don’t recall the exposure time but since the stars do not exhibit any “trailing” the exposure had to be less than 10 seconds according to the “500 Rule” (500/focal length). According to the ephemerides for this comet its magnitude on this date was 0.5.
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Comet Hyakutake was also noted for an extremely log tail – said to stretch up to 35 degrees on March 25 and later up to 100 degrees as seen from earth. The photo above was plate solved and the surrounding stars identified. From this relatively short exposure photograph, the length of the tail appears to extend upwards of 41 degrees.
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This photo was taken with a Sony DSC-H5 (7MP) 12x zoom digital camera (ISO 800) which perhaps explains the somewhat poor image quality. Nevertheless it did manage to capture this rather diffuse comet which is about 20 arc-min in diameter in the above photo.
Comet West (1976) was the first comet that I was able to capture on film. This photo was taken taken in the early morning hours in Aurora Colorado using my Pentax SP500 35mm SLR camera and a 50mm f2.0 lens.