Comet Corner

By Don Pearce

 

This is a periodic update on observational aspects of visible comets.

June 13, 2008

 

Comet 17/P Holmes. Discovered on Nov. 7, 1892 by Edwin Holmes from England, this short period comet will be known as one of the most astounding comets, ever. To understand why, let us go back to its discovery in 1892. At that time it was in outburst, because we know that normally, this comet ranges from about 15-19th magnitude as it makes its 7-year (average) trip around the Sun. But, then in November of 1892 it literally exploded, brightened to about 4th magnitude, and was discovered by Holmes. After about 3 weeks it, then, dimmed again, only to, suddenly brighten again in January of 1893. After that it started declining, slowly, dimming to about 12th mag. by March, and disappearing, altogether, by April 6th of that year (1893). It was seen again at the next two apparitions, but only as a dim comet. However, a close encounter with Jupiter in 1908 (around Dec. 8th at about .543 AU) increased the size of its orbital period, and although hunted down, was lost for most of the 20th century.

 

This has to be the second most fascinating quality of Holmes. For not only has it had these unpredictable outbursts, after its discovery astronomers had a very difficult time in even locating this comet, as evidenced that between 1906 and 1964 no one knew where it was. Finally, in 1963 Brian Marsden recalculated its orbit, and it was recovered at 19th magnitude in 1964. With improved instrumentation and understanding of orbital mechanics, it has been observed at every return since then.

 

The third most astounding feature of this comet is why it was so quiet for the 115 years since its initial out bursts and discovery in 1892, and then really turned on October 23rd of last year. It went from about 16.5 to about 2.5 magnitude in the span of about 2-3 days, which is about a 400,000 increase in brightness. Nothing like that has ever been observed in cometary science.

 

The next astounding aspect of this comet is its appearance. It developed a huge circular, distinctly yellow coma, and within days it expanded from about 1-2 arc minutes to 7 or 8 arc minutes in diameter. It then sprouted an outer halo surrounding the coma, and within the coma developed a bright feature, which was described as a fan-like structure, a blob, etc., which, incidentally, gave the appearance in low power that the pseudo-nucleus, which had been mostly stellar, as being off-center. But the pseudo-nucleus at that time remained centered; it was this bright feature that had been consistently southwest of the central condensation in the anti-solar direction. I, and most other observers, believed that this bright feature was the dust tail. Because of the geometrical perspective, it appeared severely foreshortened. Later, a faint tail, with “streamers,” also had been imaged in the same direction (anti-solar). It was a little uncertain whether this was a gas or dust feature. As November progressed, the size of the coma continued to increase, as it became larger and larger. At the same time the surface brightness decreased while the overall integrated magnitude remained between 3rd and 3.5 magnitude. This continued throughout December and January.

 

More amazing has been the continued increase in the size of the coma and its shape changing from near circular to parabolic, so that it became longer than its width. For a while the coma resembled an umbrella or jellyfish, but later had become even more elongated, and even from a moderately dark sky had lost its sharp edge, visually. From a very dark sky, it remains naked eye, although it has lost naked eye visibility from any area with even the slightest light pollution. I had observed it from our familiar “Area 51” site on New Year’s night, estimated its magnitude at 3.1, the size of the coma at about a full degree by about 35 arc minutes. It was very obvious naked eye. There has been much discussion as to how this comet could continue to shine at close to 3rd magnitude, while it continues to recede from the Earth. In fact, there is still no definitive resolution as to the cause of the original outburst and its subsequent behavior.

 

For myself, I am leaning towards the idea that at some time in the past, 17/P had a slightly closer perihelion distance enabling it develop a thick crust, then was shifted into an orbit further out where the ices went into “deep freeze”. It has, since 1968, been migrating again towards a closer perihelion distance. At some point after its last perihelion passage (May 4, 2007), the internal pressure built up (due to the thick crust), and with its unique combination of ices (gases) and particulates, exploded into what we have witnessed and measured.

 

What future behavior will Holmes exhibit? It now appears that it will not follow its 1892 second outburst pattern. On the night of Jan. 29th I, along with my wife Ann Nette, Kenneth Drake and his wife Joy, observed Holmes naked eye from a very dark location just a few miles south of Ft. Griffin, Texas. I was astounded that it was still visible naked eye, and I estimated its magnitude at 3.9 with a total coma size of 1.5 degrees (in binoculars). That translates into a real size of almost 6 million miles, which makes the coma of Holmes the largest body in the solar system. In binoculars the coma was very bright and discernible, and while there was a gradual brightening toward the center, there wasn’t any visual hint of a pseudo-nucleus. Holmes has gradually been fading, and I cannot find any observations later than April 26th, when Alan Hale reported he could barely see it in 8-inch aperture from a very dark location at high altitude. He estimated its magnitude at 7.5. During June it is, in effect, in conjunction with the Sun and is not observable as it resides in Gemini. Holmes may not be seen again until it returns toward perihelion in 2014.

  

C/2007 W1 (Boattini) reaches both closest approach to the Earth (.21 AU) in mid-June (11th) and perihelion (.85 AU) later this month on the 24th, and due to its proximity with the Earth, has reached about 5.2 magnitude. Unfortunately for us, it is strictly a southern hemispheric object, but many images of this comet are coming out of the south. Currently W1 is in Lepus, moving northwestward, and will end June in Eridanus, only having slightly faded.

 

Comet C/2006 Q1 (McNaught) is an evening comet, currently in Sextans and moving towards the northeast. It is about 10.9 magnitude, but because it is receding from the Earth, will not brighten, even though it doesn’t reach perihelion until July 3rd at 2.76 AU. By the end of June it will enter Crater, and then begin to slowly fade after the 3rd of July.

  

Current comet magnitudes (June 3) and observable region (June 3)

·   Comet                          Magnitude   Trend   Observable    When visible
·   Boattini (2007 W1)                  5.5    bright  20 N to 90 S  evening
·   17P/Holmes                          5.5    fade    50 N to  5 S  early evening
·   McNaught (2006 Q1)                 11.5    steady  35 N to 80 S  evening
·   19P/Borrelly                       12      bright  Poor elongation
·   LINEAR (2007 G1)                   12      bright  45 N to 80 S  best morning
·   Boattini (2008 J1)                 12      steady  50 N to 20 S  best morning
·   Chen-Gao (2008 C1)                 12      fade     5 N to 70 S  evening
·   8P/Tuttle                          12      fade     0 N to 90 S  best evening
·   McNaught (2008 J4)                 12      bright  Poor elongation
·   McNaught (2008 A1)                 12 ?    bright  25 S to 90 S  evening
·   Broughton (2006 OF2)               12.5    bright  40 N to 10 S  early morning
·   15P/Finlay                         12.5    steady  10 N to 40 S  early morning
·   Skiff (2007 B2)                    13      steady  45 N to 60 S  evening
·   P/Beshore (2008 J2)                13      fade    45 N to 75 S  all night
·   29P/Schwassmann-Wachmann           13 ?    varies  Poor elongation
·   McNaught (2005 L3)                 13.5    fade    50 N to 35 S  all night
·   Lulin (2007 N3)                    14      bright  40 N to 70 S  morning
·   Christensen (2006 W3)             [14      bright  Poor elongation