A Cometary Breakup

While Comet 168P Hergenrother may be a bit of a mouthful, it is the proper designation for an interesting comet. Discovered in 1998, the comet is one of dozens that orbit in the inner solar system. Normally inconspicuous objects, these comets orbit quietly, objects that only astronomers love, or even know about. You would normally have needed a substantial telescope to see 168P, shining very dimly at magnitude 15.5 at it’s brightest. A community of amateur astronomers keeps tabs on these comets, occasionally photographing them, updating the orbits.

As the comet approached perihelion during the beginning of October, it became apparent that something had happened. Several observers were reporting that the comet had brightened. Suddenly the comet was far brighter, eventually reaching near 8th magnitude, over 500 times brighter than expected. We have seen this sort of thing before, a cometary breakup. Observations from several large telescopes, including Gemini North here on Mauna Kea, showed that the comet has split into at least four pieces.

When a breakup occurs it exposes a great deal of fresh material and debris, dramatically adding to the supply of dust and gas in the coma and creating a far brighter object. It is not the comet itself we see, that is fairly small. It is the coma and tail, the cloud of dust and gas that reflects the sunlight and gives a comet the synonymous appearance.

Comet 168P Hergenrother currently sports a small fan shaped tail, easily visible in the telescope. We enjoyed this classic comet shape in the telescopes last new moon at the Mauna Kea VIS. Setting up a telescope and CCD camera last night allowed me to photograph the comet, appearing much the same as it did a few weeks ago.

Comet 168P Hergenrother
Comet 168P Hergenrother taken with a 28cm SCT and a CoolSNAP ES2 CCD camera at f/10, sum of 12x30s exposures binned 4×4

Comet C/2012 S1 ISON

A new comet discovered earlier this week has caught the attention of the astronomy community. Comet C/2012 S1 (ISON) was discovered Tuesday by a telescope affiliated with ISON, the International Scientific Optical Observation Network. This is a network of mid-sized telescopes dedicated to surveillance of the near earth region of our solar system.

The reason this comet is intriguing is a combination of a large estimated size and an orbit that appears to provide both a close approach to the Sun and favorable viewing from the Earth.

The comet will approach the sun as close as 0.012 AU on November 28th, 2013, quite close indeed. The comet will also approach Earth as close as 0.4 AU (60 million kilometers or 37 million miles) on December 26th, 2013. As a result this comet could achieve a magnitude well into the negative numbers, brighter than most objects in the sky except the Sun or Moon.

This comet is in addition to comet C/2011 L4 (PanSTARRS), expected to be an unaided eye comet during the spring of 2013. If we get lucky 2013 will be a great year for comets.

As I have cautioned in the past, comet predictions are to be taken with a good amount of skepticism. This could be a spectacular comet, or this could be a mediocre comet, we will just have to wait and see. In the meantime pay attention to the light curve as it nears the Sun. As my friend David Levy observed… “Comets are like cats; they have tails, and they do precisely what they want.”

Postcard from the Universe – C/2009 P1 Garradd

Currently passing through Usra Major, comet C/2009 P1 Garradd, is bright enough to appreciate in small telescopes. It is well placed for observation, well up in the sky through much of the night. At about magnitude 6.8 it is also bright enough to make an attractive photographic target.

I am not totally happy with the photo, I could have really used more time on target. Another issue, the exposures I used were a bit too long for this fast moving target, the coma is elongated in the frames. I will probably re-shoot the comet if I get a chance soon.

C/2009 P1 Garradd
Comet C/2009 P1 Garradd taken on 28Mar2012, average of 14 x 8min frames with a Canon 20Da and the AT6RC

Driveway Astrophotography and Comet Garradd

Finally, a night where… A) The sky is clear. B) The wind is not howling through the palm trees. C) I am not exhausted by working the summit. D) I do not have to get up early the next morning.

A + B + C + D = Astrophotography from the driveway!

Comet C/2009 P1 Garradd
Comet C/2009 P1 Garradd on 29 March 2012 showing both tails, sum of 50 x 1 min exposures CoolSNAP ES and 180mm f/2.8 lens
Thus, under a very pretty sky, I rolled the photo rig out of the garage and spent some time getting everything back together. I was not in a hurry, time to let a bright crescent Moon set a little and my primary target rise a little. The target at the top of the list? Comet C/2009 P1 Garradd.

The comet is nicely placed in Ursa Major, transiting late in the evening, available for several hours of exposures. And expose I did, with the auto-guider locked on the a dim star beside the comet, the shutter open for well over two hours. I was shooting my Canon 20Da and the AT6RC, a combination that framed the comet nicely.

It will take a while to get the resulting images processed. In the meantime I did a quick process on a set of images taken with the wide field/finder CCD camera. The results of which can be seen at the right. I also shot a few quick images of the M95 area with the CCD to capture SN2012aw.

Comet Lovejoy in the Daylight

I did attempt to see comet C/2011 W3 Lovejoy in the daylight. I actually tried several times. Once on the morning of the 15th and a couple more times on the morning of the 16th after I heard that the comet had survived perihelion passage. Neither time did I see the comet with an unaided eye.

On the 15th I was not surprised I could not see it. I was in Waimea where there was a lot of low altitude haze and a lot of glare around the Sun. On the 16th I had a much better chance using the clean high altitude air of the summit of Mauna Kea. But still, no comet seen even though it should be just over four degrees from the Sun. This is about the same separation that had allowed me to see comet McNaught in early 2007.

Just to be certain I set the camera on a tripod, placed it just inside the shadow of the Keck 1 dome, and blazed away. Examining the photos on the camera display likewise revealed no trace of the comet, but there were some interesting spots of light.

It was not until I sat down and really analyzed the raw frames that I found something. Using some astronomy software, I calculated the position of the comet when the shots were taken and the field of view of the camera. And lo! There it was, a small spot with a trace of tail. It showed up best in the green channel, and not at all in the blue thanks to Rayleigh scattering in our atmosphere. Stacking nine of ten frames and processing the heck out of the frames does allow you to clearly see the comet…

Comet C/2011 W3 Lovejoy
Comet C/2011 W3 Lovejoy photographed 4° from the Sun on at 19:47UT on the morning of 16Dec2011. Canon 60D and an 85mm lens, stack of nine frames, green channel only.

Daytime Comet Reminder

Will Comet C/2011 W3 Lovejoy be visible in the daytime? This is the morning to find out. Look about 2° below the rising Sun once it is well up in the clear sky for a small white object. Two degrees is four times the Sun’s width in the sky.

C2006/P1 McNaught
C2006/P1 McNaught photographed five degrees from the Sun, stack of three images
If the comet is not visible to the eye, it should be spectacularly visible in the imagery sent back by one of our solar monitoring satellites. Check out the SOHO page for the latest imagery. The comet should have entered the field of view of the LASCO C3 instrument early on Dec 14th (late on the 13th HST) and well in by the time this posts. If the comet does not survive perihelion passage, this is one of the best views of the event.

I have seen one other daytime comet in my life, C2006/P1 McNaught back in January of 2007. That time the comet was about 5° from the Sun, over twice as far away from the glare. The photo at the right should give an idea of what to look for today. Remember to shield your eyes from the Sun’s glare by positioning yourself to put the Sun behind some object like a wall or streetlight. There is no guarantee that Lovejoy will be at all visible, but it is worth taking a look this morning.

A Daytime Comet?

The rumor is running around the various astronomy sites and listservers that Comet C/2011 W3 Lovejoy might be daytime visible. Will it be? That is a very qualified maybe.

C2006/P1 McNaught
C2006/P1 McNaught photographed five degrees from the Sun, stack of three images
This sun-grazer comet was discovered just a few days ago, on November 27th, by Australian amateur astronomer Terry Lovejoy. The comet is a member of the Kreutz comet family, and like other members of the family it will approach the Sun quite closely, about 548,000 miles (882,000 km) from the Sun. Of course those distances are solar centric distances. Taking the radius of the Sun into account means that the comet will be a mere 115,000 miles (186,000 km) above the photosphere, hot indeed!

It becomes a valid question to ask if comet Lovejoy will even survive perihelion transit.

Passing that close to the Sun will mean that the volatile elements of the comet will be streaming off the comet at a fantastic rate, enough to dramatically brighten the comet. Below you will find the ephemeris for perihelion on Dec 16th (Dec 15th HST) from the Minor Planet Center. As you can note, the predicted magnitude is -8! This is bright enough to be seen in broad daylight. Thus the possibility of a daytime comet.

The catch is that the comet will be quite close to the Sun. Within 2° as the Sun and comet rise on the morning of the 15th here in Hawai’i. For observers in the islands the best chance to look is on the morning of the 15th, as perihelion will occur in the afternoon as the comet passed behind the Sun from our point of view.

Will it be visible? Maybe. It depends on the accuracy of the magnitude estimates, which are uncertain to say the least. It could be substantially dimmer, or even substantially brighter than forecast under such conditions. The proximity to the Sun also complicates the issue. It is worth a look, seeing a daytime comet is highly unusual.

If you do look please take a few simple precautions… Do NOT use any sort of optical aid this close to the Sun, the risk of permanent eye damage is too great. If it is bright enough the comet should be a naked eye object. It will greatly help to position yourself to put the Sun just behind some obstruction. A building, a streetlight, anything to block the Sun’s glare and aid in picking out the comet. On the morning of the 15th the comet will rise 2° behind the Sun, thus 2° lower in the sky.

Give it a try!

Comet iPhone App

One drawback to the many iPhone astronomy apps is the lack of large databases. To an advanced amateur such as myself, the lack of detailed databases is a distinct negative in these programs. I venture way beyond the Messier catalog, or even the NGC on a regular basis. I understand the price to be paid in speed and memory required to support larger databases, but I would like to have the option.

C/2007 N3 Lulin
Comet C/2007 N3 Lulin on the evening of 26 Feb 2009, a stack of 10 x 4 min exposures, Canon 20Da and TeleVue 76mm APO
The programs I have seen also lack the ability to display comets or asteroids. This last issue has become a problem lately, as we have several nice comets available in the sky for observing. A quick way to look up the current position for the object is essential for comets and asteroids if you wish to observe them. Last night’s coordinates will have you looking at an empty starfield tonight.

There is one decent answer for comets… I found a very nice app for comet ephemerides published by Keith Yohn. Called simply Comet, this free program downloads the latest ephemeris data from the Minor Planet Center and displays the current and future coordinates for each comet. Just what I needed!

There are no charts, the data is simply displayed in table form. Every observable comet is displayed and can be search for using a simple set of filters.

When attempting to observe comet C/2009 P1 Gerradd a few times recently. I have found the coordinates to be quite accurate. The comet was in the sky, right where the app showed it would be. Nothing like a real world test.

Postcard from the Universe – 103P/Hartley 2

I am waiting for the Moon to leave the evening sky before shooting the comet again. In the meantime I am processing more of the material obtained earlier in the month. In this case a photo of Comet 103P/Hartley 2 taken October 6th with Keck 2 and DEIMOS. The image marks the first time I have attempted to take and process an image with a 10m telescope. Just a wee bit larger than the 76mm refractor I usually use to take astrophotos!

The image is notable for its complete lack of any interesting structure. There are no jets, shells or other inner coma detail visible. The tail is simply a general brightening to the southwest (lower right in this image).

The comet is moving very quickly across the sky, even more so with the high magnification lent by a large telescope. Even short exposures turn the stars into long streaks. In this case multicolor streaks as the camera cycles through the filters needed for a color image.

103P/Hartley 2
Comet 103P Hartley 2 with Keck2 and DEIMOS 6Oct2010 @ 7:27UT, 3x60s, 3x60s and 3x120s with standard BVR astrometric filters, credit: Cooper/Wirth/W.M. Keck Observatory