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New Images of Comet ISON Hurtling Towards the Sun

Images of Comet ISON obtained using the Gemini Multi-Object Spectrograph at Gemini North on February 4, March 4, April 3, and May 4, 2013 (left to right, respectively; Comet ISON at center in all images). Color composite produced by Travis Rector, University of Alaska Anchorage. Credit: Gemini Observatory/AURA

Images of Comet ISON obtained using the Gemini Multi-Object Spectrograph at Gemini North on February 4, March 4, April 3, and May 4, 2013 (left to right, respectively; Comet ISON at center in all images). Color composite produced by Travis Rector, University of Alaska Anchorage. Credit: Gemini Observatory/AURA

As Comet C/2012 S1 (ISON) heads closer to Earth, we’re getting a better view of what has been billed by some as the “Comet of the Century.” Astronomers say these new photos from the Gemini North telescope on Mauna Kea, Hawai‘i provide hints of how well this comet might survive one of the closest comet encounters with the Sun ever recorded, on November 28, 2013.

With astronomy enthusiasts hopeful and optimistic about having a spectacular comet visible in our skies, it’s anyone’s guess if the comet will actually survive its extremely close pass of the Sun to become early morning eye-candy in early December 2013.
The time-sequence images, spanning early February through May 2013, show that the comet is quite active, despite how distant it is from the Sun.

When Gemini obtained these images, the comet ranged between roughly 455-360 million miles (730-580 million kilometers; or 4.9-3.9 astronomical units) from the Sun, or just inside the orbital distance of Jupiter. Each image in the series, taken with the Gemini Multi-Object Spectrograph at the Gemini North telescope on Mauna Kea, Hawai‘i, shows the comet in the far red part of the optical spectrum, which emphasizes the comet’s dusty material already escaping from the nucleus. The final image in the sequence, obtained in early May, consists of three images, including data from other parts of the optical spectrum, to produce a color composite image.

Gemini astronomers say the images show the comet sporting a well-defined parabolic hood in the sunward direction that tapers into a short and stubby tail pointing away from the Sun. These features form when dust and gas escape from the comet’s icy nucleus and surround that main body to form a relatively extensive atmosphere called a coma. Solar wind and radiation pressure push the coma’s material away from the Sun to form the comet’s tail, which we see here at a slight angle (thus its stubby appearance).

“Early analysis of our models shows that ISON’s brightness through April can be reproduced by outgassing from either carbon monoxide or carbon dioxide,” said Karen Meech, at the University of Hawaii’s Institute for Astronomy (IfA) in Honolulu. “The current decrease may be because this comet is coming close to the Sun for the first time, and a “volatile frosting” of ice may be coming off revealing a less active layer beneath. It is just now getting close enough to the Sun where water will erupt from the nucleus revealing ISON’s inner secret.”

Comet ISON will come within 800,000 miles (1.3 million km) of the Sun’s surface on November 28. Shortly before that critical passage, the comet may appear bright enough for expert observers using proper care to see it close to the Sun in daylight.

“Comets may not be completely uniform in their makeup and there may be outbursts of activity as fresh material is uncovered,” added IfA astronomer Jacqueline Keane. “Our team, as well as astronomers from around the world, will be anxiously observing the development of this comet into next year, especially if it gets torn asunder, and reveals its icy interior during its exceptionally close passage to the Sun in late November.”

NASA’s Hubble Space Telescope provides a close-up look of Comet ISON (C/2012 S1), as photographed on April 10, when the comet was slightly closer than Jupiter’s orbit at a distance of 386 million miles from the sun. Credit:NASA, ESA, J.-Y. Li (Planetary Science Institute), and the Hubble Comet ISON Imaging Science Team.

NASA’s Hubble Space Telescope provides a close-up look of Comet ISON (C/2012 S1), as photographed on April 10, when the comet was slightly closer than Jupiter’s orbit at a distance of 386 million miles from the sun. Credit:NASA, ESA, J.-Y. Li (Planetary Science Institute), and the Hubble Comet ISON Imaging Science Team.

NASA’s Swift satellite and the Hubble Space Telescope (HST) have also imaged Comet ISON recently in this region of space. Swift’s ultraviolet observations determined that the comet’s main body was spewing some 850 tons of dust per second at the beginning of the year, leading astronomers to estimate the comet’s nucleus diameter is some 3-4 miles (5-6 kilometers). HST scientists concurred with that size estimate, adding that the comet’s coma measures about 3100 miles (5000 km) across.

The comet gets brighter as the outgassing increases and pushes more dust from the surface of the comet. Scientists are using the comet’s brightness, along with information about the size of the nucleus and measurements of the production of gas and dust, to understand the composition of the ices that control the activity. Most comets brighten significantly and develop a noticeable tail at about the distance of the asteroid belt (about 3 times the Earth-Sun distance –– between the orbits of Mars and Jupiter) because this is when the warming rays of the Sun can convert the water ice inside the comet into a gas. This comet was bright and active outside the orbit of Jupiter — when it was twice as far from the Sun. This meant that some gas other than water was controlling the activity.

Meech said that Comet ISON “…could still become spectacularly bright as it gets very close to the Sun” but also added caution. “I’d be remiss, if I didn’t add that it’s still too early to predict what’s going to happen with ISON since comets are notoriously unpredictable,” she said.

Source: Gemini Observatory

About 

Nancy Atkinson is Universe Today's Senior Editor. She also works with Astronomy Cast, and is a NASA/JPL Solar System Ambassador.

Comments on this entry are closed.

  • Planemo May 30, 2013, 5:44 PM

    A comet passing 800,000 miles from our star? I will be so amazed if this icy-rock survives passage. This icy-rock is 450 X’s closer than Mercury is to our star. We should all sing: A comet roasted on an open fire……. ..lol.

    • William Sparrow May 30, 2013, 10:14 PM

      Mercury’s distance from the Sun ranges from 46 million kilometers at perihelion to 70 million kilometers at aphelion, versus this comet coming within 1.3 million kilometers of the Sun, so I’m not sure where you came up with your math. In any event, this passage may be too close for comfort!

      • Planemo May 31, 2013, 2:31 AM

        My math was simple averaging. .. Yes, Mercury is about 28 million miles at its closest and 43 million miles at its furthest(aphelion-perihelion). I was using the mediums 28+43=71 ….Half 71 is 35.5 to 36 Million miles. 36,000,000 is the “average” distance for Mercury orbiting the sun 2x’s. The comet will come 450 X’s closer than Mercury’s average distance. 800,000 X’s 450=36mil.miles. I hope my new math enlightens you…lol…lol. :-). I was just averaging the medium distance..

        • Meteodan May 31, 2013, 8:49 PM

          Check your math, 800,000*450=36000000=360 million miles, not 36 million miles. So, the correct answer is about 45X closer, not 450X.

          • Planemo May 31, 2013, 8:52 PM

            Yes you are correct. 45.0. I did not put the point/period after 45. My fault. But you got the point, ..period…..lol. 45.0 is what I did not do. 450 45.0…my fault. But I was correct for except that point/period error.

          • William Sparrow May 31, 2013, 9:29 PM

            Right……. Come on Planemo, just admit you made an error.

          • Planemo May 31, 2013, 10:39 PM

            Right? ..and ‘left’ also.45.0 or 450 I said ‘error’. Come on Dan…what else does “error” mean to you?…lol.

          • Planemo May 31, 2013, 9:09 PM

            PS: …come on man, …Dan. Where is your avatar? Everybody who’s side-kick name like yours needs an avatar. Meteodan. Good choice! My side-kick name of Planemo means a wondering planet with no sun to orbit. A loner who got kicked out or flung out of his solar system. A free’bird from the early days of Lynyrd Skynyrd. ;-)

          • William Sparrow May 31, 2013, 9:29 PM

            My point exactly, Meteodan.

          • Planemo May 31, 2013, 10:37 PM

            35.5 or 36…or 450 45.0 I admitted what I did wrong. What else do you need?

          • Planemo May 31, 2013, 10:36 PM

            Right? Left too! That’s exactly what I said. I made an error w450 45.0. I said my fault. Get ity now?

  • cschur May 30, 2013, 6:31 PM

    This is going to be an astro imagers delight. Even on the way in before it could potentially burn to a crisp, the photo opportunities will be abundant. I would like to see a more gassy comet, which sports a green head full of nice cyanogen spectral lines. Our last shots of it last month revealed so far only dust is coming off the comets nucleus or the gas has not been ionised yet. The problem now is that it is very near the sun at sunset, and will be behind the sun for a while. When it reemerges in the morning sky in a few months it will be very interesting to see how it has changed!

    Chris Schur

  • Aqua4U May 30, 2013, 11:46 PM

    Late November here in No. California is usually wet… but sometimes, there are ultra clean/clear skies between frontal systems… or so I hope!

  • Raymond Chuang May 31, 2013, 2:25 AM

    However, Comet ISON could be an astronomical “bust” because I’ve read new measurements show the comet is physically quite small. That means as the comet approaches perihelion, the brightness could be quite low. This wasn’t like Comet Hale-Bopp in 1997, which was one of the brightest comets ever seen by humans (it was almost as bright as the brightest star seen by the naked eye, Sirius).

  • M_J_Murcott May 31, 2013, 1:01 PM

    What is a coma – http://youtu.be/T3-dZHRR3eA

  • Bruno Melo May 31, 2013, 3:56 PM

    I don’t know if Jupiter’s orbit distance might be too early to start Ison’s reaction. I mean, 400 million miles? I guess my expectations are too high for it and I don’t want to get disappointed but we all do hope it survives enough to show up spectaculary by our heads early Noc/Dec.

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