I have been posting a lot of photos from others lately. Not something I do a lot of, I prefer to use my own shots. But when I get shots like this…
Tag: C/2011 W3
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…
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.
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.
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!
12 Date TT R. A. (2000) Decl. Delta r Elong. Phase m1 m22011 12 05 15 16 55.0 -49 16 23 0.7020 0.5385 31.9 104.4 10.5 16.7<br>2011 12 06 15 35 50.9 -47 54 07 0.7082 0.5050 29.3 107.4 10.3 16.8<br>2011 12 07 15 53 36.9 -46 18 58 0.7170 0.4704 26.6 110.4 10.0 16.8<br>2011 12 08 16 10 07.0 -44 32 30 0.7285 0.4344 23.9 113.4 9.7 16.9<br>2011 12 09 16 25 18.7 -42 36 14 0.7429 0.3970 21.2 116.2 9.3 16.9<br>2011 12 10 16 39 12.4 -40 31 31 0.7604 0.3576 18.5 119.0 8.9 16.9<br>2011 12 11 16 51 50.3 -38 19 18 0.7813 0.3161 15.9 121.7 8.5 16.9<br>2011 12 12 17 03 15.7 -35 59 57 0.8060 0.2716 13.2 124.2 7.9 16.9<br>2011 12 13 17 13 31.2 -33 32 42 0.8352 0.2233 10.5 126.5 7.1 16.7<br>2011 12 14 17 22 37.5 -30 54 29 0.8705 0.1691 7.7 128.3 6.0 16.4<br>2011 12 15 17 30 26.9 -27 55 51 0.9153 0.1048 4.8 128.7 4.0 15.5<br>2011 12 16 17 31 43.4 -23 03 22 0.9885 0.0057 0.2 42.0 -8.5 5.4<br>2011 12 17 17 17 12.6 -25 07 18 0.9135 0.1046 4.7 130.1 4.0 15.6<br>2011 12 18 17 11 57.9 -27 12 24 0.8656 0.1692 7.5 130.6 6.0 16.6<br>2011 12 19 17 08 21.5 -29 13 16 0.8260 0.2234 10.1 129.7 7.1 17.0<br>2011 12 20 17 05 34.5 -31 14 08 0.7912 0.2717 12.5 128.6 7.8 17.2<br>2011 12 21 17 03 19.7 -33 17 03 0.7597 0.3162 14.8 127.2 8.4 17.3