Saturn from the VATT

On my last night at the VATT, the clouds rolled in right before dawn. Rather than close up early I tried a little Saturn observing. Thanks to the use of a narrow-band Vilnius S filter (central bandpass ~0.655 nm), a shutter that can take short exposures and the clouds, I was able to get a few good shots of the ringed planet.

Usually when astronomers image the planets they use video rate cameras and take 1000s of images. Specialized software is then used to pick out the best of the images which are then co-added together to bring out subtle details. The VATT4K is not optimized for such rapid imaging so I was limited to taking only a few images. Still the image shows lots of good detail. It sure helped that the mountain was experiencing sub-arc second seeing.

The image below was one of the best.

Saturn_2013Jan21_Hergenrother

Comets from the VATT

Last week I spent three nights observing asteroids and comet with the Vatican Observatory’s 1.8-m VATT telescope on Mount Graham in southeastern Arizona. The observing run was part of my program to characterize asteroids that could be good spacecraft targets as well as objects that are analogous to the OSIRIS-REx target asteroid. When possible I never pass up the opportunity to observe a few comets.

Though clouds affected two of the nights, the conditions were rather good. In fact, the seeing was exceptional and was as good as 0.7″ at times.

As luck would have it, the brightest comets in the sky were not visible from the VATT either because they were too far south or too close to the Sun for observation (or in the case of C/2012 K5, I just couldn’t fit it into my observing schedule).

The following is an update on a few long-period comets with some images I took from the VATT.

C/2011 L4 (PANSTARRS)

C2011L4_orbitThe big comet of the spring is supposed to be comet C/2011 L4 (Panstarrs). When discovered back in June of 2011 the brightness of the comet at a distance of ~8 AU (halfway between the distances of Jupiter and Saturn) suggested this comet could be a brilliant negative magnitude at perihelion in March of this year.

There was some questions whether this comet was on its first passage through the inner Solar System or if it had been through the neighborhood before. This is an important distinction because comets fresh from the Oort cloud have a tendency of being very active while far from the Sun. Then as the most volatile ices are sublimed off, the comet settles down into a less active state and never gets quite as bright as predicted. We have seen this many times in the past with comets being lauded as “great” or “future” comets, only to disappoint when they finally reach perihelion. Comet Cunningham in 1941, Kohoutek in 1973/74 and Austin in 1990 are prime examples

Comet PANSTARRS has an orbit that is almost indistinguishable from parabolic meaning the comet is likely to be a fresh comet from the Oort cloud. This fact had many people doubting whether it would really reach magnitude -1 as predicted by its early behavior. Now that the comet is once again observable (though only from the Southern Hemisphere) it does appear the comet’s brightening has slowed down and the comet will only reach a magnitude of +2 to +3 if that.

Recent visual observations place the comet between magnitude 7.0 and 7.5. It will continue to be a southern-only comet till mid-March when it will become visible in the early evening sky for northern observers. Sky and Telescope has some nice finder charts for the comet here. Even with a peak brightness of “only” 2nd or 3rd magnitude, the comet will be quite a sight in binoculars and small telescopes.

C/2012 F6 (Lemmon)

C2012F6_orbitIf Comet PANSTARRS is an example of the “over-hyped” comet that is “under-performing”, Comet Lemmon is the exact opposite. When discovered by the Mount Lemmon Survey last March, the comet was nothing special. Even with a perihelion distance of only 0.73 AU, the comet looked too faint to amount to much. I even placed it on my watch list for small comets that were likely to disintegrate and not survive perihelion. Instead this comet has been brightening at a much faster rate than predicted and is now the brightest comet in the sky.

Back on January 9 I spotted it in my 30×125 binoculars at magnitude 7.9. It was an easy object even though it only got ~10° above the horizon as it was speeding to the south. Its southward motion now means the comet is only visible for Southern Hemisphere observers.

The most recent visual observations place is around magnitude 6.5. If it continues like this it could rival or even surpass Comet PANSTARRS in brightness at magnitude +2 to +3 when it reaches perihelion at the end of March. For those of us up north the comet will again become visible in late April/ early May. At the time the comet will be fading but should still be around 5th magnitude.

273P/Pons-Gambart

273P_orbitThe surprise return of Pons-Gambart has been discussed in earlier posts (here, here, and here). After spending a month too close to the Sun for Earth-based observations, the comet is once again visible between magnitude 8.5 and 9.0. The comet may remain brighter than magnitude 10 and within range of small telescope users for another month or so.

Pons-Gambart has a period of ~188 years. It was seen once before in 1827 during its last perihelion passage. Its period will actually shorten by a few years results in the next return in 2191.

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C/2012 K1 (LINEAR)

C2012K1_orbitDiscovered on May 19, 2012 by the LINEAR survey at a faint 19-20th magnitude, the comet was then located at a distant 8.8 AU from the Sun. It is now ~6.8 AU out and has brightened to magnitude ~17.2. Though the comet does not look like much, it will get much brighter as it approaches its August 27, 2014 perihelion at a distance of 1.05 AU from the Sun.

Right now the comet looks on track to reach 6th magnitude at perihelion, but… similar to Comet PANSTARRS, C/2012 K1 is also an Oort cloud comet making its first visit to the inner Solar System. It is likely that it will also experience a slow down in brightening and will not get as bright as predicted. Time will tell …

In the here and now, the VATT showed K1 to be a nice small condensed comet at 17th magnitude.

C2012K1_TranSky

C/2012 S1 (ISON)

Comet ISON is the big one. Many media outlets are already calling this one the “Comet of the Century” which will shine brighter than the Full Moon. Possibly…

C2012S1_orbitAs the lesson of Comet PANSTARRS has taught us, the past behavior of a comet does not guarantee its future performance.The aforementioned Comets Cunningham and Kohoutek were also called “Comets of the Century” in their time. Neither lived up to the moniker.

ISON does have a few things going for it. The best news is its orbit which is very similar to the Great Comet of 1680. It is doubtful that ISON and the 1680 comet are one and the same. It is possible that the two comets are pieces of an older comet that split in the past. Simply being related to the 1680 comet does not mean ISON will be as spectacular as that comet but it does mean ISON has been around before and is not a new Oort cloud comet. This bodes well for ISON to brighten at a good rate and also survive perihelion.

A year ago, Comet C/2011 W3 (Lovejoy) passed even closer to the Sun than ISON will. Though Lovejoy disintegrated a few days past perihelion that was still enough time for it to produce a long bright tail that was observable for weeks (only for southern observers though, Lovejoy was invisible for Northern Hemisphere observers after perihelion). If ISON can survive it close brush with the Sun by even a few days it will produce a long bright tail that should be easily visible by northern observers (sorry southerners, ISON is our turn to enjoy a brilliant sun-grazing/skirting comet) throughout the month of December 2013.

When it reaches perihelion this November 28 (Thanksgiving Day!) it will be located only 0.012 AU from the center of the Sun or ~1.1 million km (660,000 miles) from the Sun’s surface which just under 3 times the distance from the Earth to the Moon. (Editors Note: Thanks to Joe Stieber for pointing out the error in my perihelion Sun distance!) Right now ISON is currently located at ~5 AU (the distance of Jupiter) from the Sun and still has almost 10 months to go before perihelion.

The VATT found ISON to be a nice compact 15th magnitude comet wandering among the stars of Gemini.

C2012S1_TranSky

C/2012 T5 (Bressi)

C2012T5_orbitFrom a potential great comet to an absolute runt of a comet. Comet Bressi was first spotted by Spacewatch observer Terry Bressi from Kitt Peak on October 14, 2012. If any of the comets in this blog post are likely to not survive perihelion, this is the one.

The comet is currently just within 1 AU of the Sun and little over 1 AU from Earth. Even after a recent outburst a week or two ago the comet is still rather faint. My observations place it at V magnitude 13.0 but this is most likely an underestimate as the observations were hampered by a very right Moon nearby and the comet’s low elevation. Visual observers place it closer to magnitude 11-12.

Note that unlike most comets in this blog post, Bressi is much brighter in the V versus the R. Most of the more distant comets are actually brighter in the R. The reason is that Bressi is a much more gaseous comet due to its closer distance to the Sun and perhaps even internal composition.

Comet Bressi will reach perihelion on February 24 at a distance of 0.32 AU from the Sun. It will be interesting to see if it survives. If it does it may brighten enough to be seen in small telescopes though observations will be limited to southern observers until March.

C2012T5_TranSky

C/2012 V2 (LINEAR)

C2012V2_orbitThis LINEAR comet was discovered on November 5. At perihelion on August 16, 2013 at a distance of 1.45 AU from the Sun the comet should be no brighter than 12-13th magnitude. It should remain out of reach of most visual observers.

Last week the VATT caught 2012 V2 out at a distance of ~3.1 AU from the Sun. The comet was magnitude 16 and sported a short tail extending to the northeast.

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C2012V2_TranSky

C/2012 X1 (LINEAR)

C2012X1_orbitYet another inbound Comet Linear, C/2012 X1 was first spotted last month on December 8th. It is currently at a distance of ~4.8 AU from the Sun which is just inside the distance of Jupiter’s orbit. When it reaches perihelion next year on February 21st, it will be 1.60 AU from the Sun. That’s not too close so it should only brighten to about 11th magnitude by then.

Last week the comet was seen at 18th magnitude with a broad fan tail.

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C2012X1_TranSky

C/2013 A1 (Siding Spring)

C2013A1_orbitThe first comet to be discovered in 2013 is the most recent comet to be discovered that may become bright enough for backyard observers. Rob McNaught found C/2013 A1 on January 3rd from Siding Spring, Australia. Right now the comet is further from the Sun than Jupiter is at a distance of ~7 AU. The VATT found the comet to be around V magnitude 18.7 with a nice tail to the northeast

The comet is almost 2 years from perihelion which won’t occur until October 23, 2014 at a distance of 1.39 AU from the Sun. It could become as bright as 7th magnitude at that time though a lot can happen over the next 2 years and the comet may end up significantly fainter.

C2013A1_TranSky

C/2009 P1 (Garradd)

C2009P1_orbitThe next two comets are examples of objects that were bright enough for small telescope users in the past but are now fading as they leave the inner Solar System.

Comet Garradd was a splendid sight for many months between the 2nd half of 2011 and the 1st half of 2012. During that stretch the comet was an easy binocular object of 6th-7th magnitude. Now over a year past its December 2011 perihelion (at a distance of 1.55 AU from the Sun) and 3.5 years since its discovey, the comet has retreated to a distance of 4.8 AU from the Sun which is nearly the distance of Jupiter.

My VATT images from January 20 find the comet at V magnitude 13.5. The comet displays a small condensed coma of ~1′ within a much larger diffuse coma of 3′. The bright inner coma is dust recently released by the comet while the diffuse faint outer coma is dust released when the comet was more active in the past. The fact that we are observing dust released over many months or years does make it difficult to properly measure the current activity level of the comet.

A faint broad tail can also be seen extending towards the north. Too bad the Moon was bright that night and affected the images or the tail and outer coma would have been better defined. This will be a fun comet to watch as it continues its journey back into the depths of the outer Solar System. Based on the latest orbit by Syuichi Nakano, Comet Garradd won’t be back for ~500,000 years.

C2009P1_TranSky

C/2011 UF305 (LINEAR)

C2011UF305_orbitAnother comet on the way out, C/2011 UF305 reached perihelion last July at a rather distant  2.13 AU from the Sun. Though it had a large perihelion distance it did brighten to 10th magnitude for a few months during the summer and fall of 2012.

The comet is now ~230 days past perihelion at a distance of 3 AU from the Sun. My VATT observations yield a V magnitude of ~13.8 which is still bright enough for visual observers with very large backyard telescopes to observe it. For small telescope users, the comet is well out of reach.

Drifting against the stars of Cancer, the comet was near opposition. Similar to C/2009 P1, a large diffuse dust tail can be seen extending towards the north. Most likely this is dust that was released many months ago when the comet was more active. This will also be a fun comet to see how long it can be followed as it recedes into the depth of the outer Solar System. Based on the latest orbit by Syuichi Nakano, Comet Garradd won’t be back for ~90,000 years.

C2011UF305_TranSky

Meteor Activity Outlook for January 26 – February 1, 2013

The following is a slightly edited version of Bob Lunsford’s excellent weekly summary of meteor activity. The original version can be found at the American Meteor Society’s site.

During this period the moon reaches its full phase on Sunday January 27th. At this time the moon will be located opposite the sun and will be in the sky all night long.  As the week progresses the moon will rise a little later each evening but there is little meteor activity to be seen during the dark evening hours. The estimated total hourly meteor rates for evening observers this week is near two for observers located at mid-northern latitudes and one for observers in mid-southern latitudes. For morning observers the estimated total hourly rates should be near eight from the mid-northern hemisphere and four from the mid-southern hemisphere. The actual rates will also depend on factors such as personal light and motion perception, local weather conditions, alertness and experience in watching meteor activity. Rates are reduced during this entire period due to intense moonlight.

The radiant (the area of the sky where meteors appear to shoot from) positions and rates listed below are exact for Saturday night/Sunday morning January 26/27. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The table below presents a condensed version of the expected activity this week. Rates and positions are exact for Saturday night/Sunday morning . Details of each shower will again be provided next week when the situation with interfering moonlight improves.

Antihelions (ANT) – 09:20 (140) +15   Velocity – 30km/sec.
Northern Hemisphere – 2 per hr.   Southern Hemisphere – 1 per hr

IMO #22- 113:04 (196) +12   Velocity – 65km/sec.
Northern Hemisphere – <1 per hr.   Southern Hemisphere – <1 per hr

Alpha Centaurids (ACE)  – 13:12 (198) -56   Velocity – 56km/sec.
Northern Hemisphere – <1 per hr.   Southern Hemisphere – <1 per hr

Alpha Coronae Borealids A (ACB)  – 15:28 (232) +29   Velocity – 60km/sec.
Northern Hemisphere – 1 per hr. Southern Hemisphere – <1 per hr

Alpha Coronae Borealids B (ACB)  – 16:04 (241) +42   Velocity – 51km/sec.
Northern Hemisphere – <1 per hr. Southern Hemisphere – <1 per hr

Clear Skies!
Robert Lunsford
American Meteor Society

Meteor Activity Outlook for January 12-18, 2013

The following is a slightly edited version of Bob Lunsford’s excellent weekly summary of meteor activity. The original version can be found at the American Meteor Society’s site.

During this period the moon reaches its new phase on Friday January 11th. At this time the moon is located near the sun and will remain invisible at night. Next week the waxing crescent moon will enter the evening sky but will set long before the more active morning hours arrive. The estimated total hourly meteor rates for evening observers this week is near three no matter your location. For morning observers the estimated total hourly rates should be near fifteen from the mid-northern hemisphere and eleven from the mid-southern hemisphere. The actual rates will also depend on factors such as personal light and motion perception, local weather conditions, alertness and experience in watching meteor activity.

The radiant (the area of the sky where meteors appear to shoot from) positions and rates listed below are exact for Saturday night/Sunday morning January 12/13. These positions do not change greatly day to day so the listed coordinates may be used during this entire period

The following showers are expected to be active this week:

The large Antihelion (ANT) radiant is currently centered at 08:20 (125) +18. This position lies in central Cancer, four degrees west of the fourth magnitude star Asellus Australis (Delta Cancri). These meteors may be seen all night long but the radiant is best placed near 0100 local standard time (LST) when it lies on the meridian and is highest in the sky. Rates at this time should be near two per hour as seen from the northern hemisphere and one per hour from south of the equator. With an entry velocity of 30 km/sec., the average Antihelion meteor would be of slow velocity.

The December Leonis Minorids (DLM) are currently the most active shower in the sky. The radiant is located at 12:16 (184) +19. This position lies in southwestern Coma Berenices, seven degrees northeast of the second magnitude star Denebola (Beta Leonis). These meteors are best seen near 0400 LST when the radiant lies highest above the horizon. This shower peaked on December 17th so current rates would be near two per hour as seen from the northern hemisphere and one per hour as seen from south of the equator. At 64 km/sec. the December Leonis Minorids produce mostly swift meteors.

IMO Shower #14 is an unnamed shower active in mid-January. Peak activity occurs on January 18th from a radiant located at 13:16 (199) -20. This position is located in southwestern Virgo, nine degrees south of the first magnitude star Spica (Alpha Virginis). This radiant does not rise until after midnight so activity is strictly limited to the morning hours. Rates would mostly likely be less than one shower member per hour, no matter your location. These meteors are best seen during the last dark hour before dawn, when the radiant lies highest above the horizon in a dark sky. At 70 km/sec. IMO Shower #14 would produce mostly swift meteors.

The Canum Venaticids (CVN) are a new shower discovered by Peter Brown and his associates at the University of Western Ontario, using meteor orbits obtained by radar. This activity was verified by the IMO video network which has 271 possible candidates in its database. This shower is best seen from January 11-17, with maximum activity occurring on the 11th. Rates never exceed one shower member per hour yet it is the 3rd strongest radiant in the sky on the mornings of January 13 and 14. The radiant is located near 14:08 (212) +36, which places it in southeastern Canes Venatici. This position also lies 5 degrees southwest of the famous third magnitude double star known as Cor Caroli (Alpha Canum Venaticorum). Do not be too strict with this position as the radiant is not well defined at this point. Any meteors from this area this time of year should be suspected as possible Canum Venaticids. I would suggest using radiant distance and velocity to further determine possible shower association. These meteors encounter the atmosphere at 59 km/sec., which would produce mostly swift meteors. These meteors are best seen during the last few hours before dawn, when the radiant lies highest in a dark sky. This activity would be difficult to view from the southern hemisphere as the radiant lies low in the north at dawn.

The Theta Coronae Borealids (TCB) are another new shower discovered by Peter Brown and his associates at the University of Western Ontario, using meteor orbits obtained by radar. This activity was also verified by the IMO video network which has 189 possible candidates in its database. This shower is only active on six nights centered on January 16th. Rates again never exceed one shower member per hour yet it is the 3rd strongest radiant in the sky on January 16th. On that morning the radiant is located at 15:40 (235) +51, which places it twenty degrees north of Theta Coronae Borealis. Earlier visual observations must have placed the radiant much too far south. Either that or this shower is completely different from the early TCB radiant. The closest bright star to the radiant is third magnitude Edasich (Iota Draconis), which lies eight degrees to the north. These meteors are best seen during the last dark hour before dawn, when the radiant lies highest above the horizon in a dark sky. At 39 km/sec. the Theta Coronae Borealids would produce meteors of medium velocity.

As seen from the mid-northern hemisphere (45N) one would expect to see approximately ten sporadic meteors per hour during the last hour before dawn as seen from rural observing sites. Evening rates would be near two per hour. As seen from the mid-southern hemisphere (45S), morning rates would be near eight per hour as seen from rural observing sites and two per hour during the evening hours. Locations between these two extremes would see activity between the listed figures.

The list below presents a condensed version of the expected activity this week.
Rates and positions are exact for Saturday night/Sunday morning .

Antihelions (ANT) – 08:20 (125) +18   Velocity – 30km/sec.
Northern Hemisphere – 2 per hr.   Southern Hemisphere – 1 per hr

December Leonis Minorids (DLM) – 12:16 (184) +19   Velocity – 64km/sec.
Northern Hemisphere – 2 per hr.   Southern Hemisphere – 1 per hr

IMO #14 – 13:16 (199) -20   Velocity – 70km/sec.
Northern Hemisphere – <1 per hr.   Southern Hemisphere – <1 per hr

Caneum Venaticids(CVN) – 14:08 (212) +36   Velocity – 59km/sec.
Northern Hemisphere – <1 per hr.   Southern Hemisphere – <1 per hr

Theta Coronae Borealids (TCB)  – 15:40 (235) +51   Velocity – 39km/sec.
Northern Hemisphere – <1 per hr. Southern Hemisphere – <1 per hr

Clear Skies!
Robert Lunsford
American Meteor Society

Last Night’s Quadrantids

The Quadrantid meteor shower was predicted to peak last night. Even though the nearly Last Quarter Moon was high in the sky and resulted in a somewhat washed out sky, a number of Quadrantids could still be seen.

I spent an hour watching the Quads between 11:22 and 12:22 UT (4:22 and 5:22 am MST). In that time, I observed 29 Quadrantids and 5 sporadics (or more accurately non-Quadrantids since I wasn’t keeping track of any other active showers). Six of the Quadrantids were brighter than 0th magnitude and two were as bright as -3. During one ten second period, three Quadrantids were seen in rapid succession all moving in the same direction across the bowl of the Big Dipper and head of Ursa Major.

The Moon had an effect on the number of meteors that were seen. Usually my early morning limiting magnitude from my backyard is +6.1. With the Moon it is was +5.6. Plugging my numbers into the ZHR formula yields a range of ZHRs of 64, 96 and 90 for the 3 20-minute periods I was observing. Averaging the meteors over the hour yielded a ZHR of ~89. This is about normal for an average peak Quadrantid rate so the peak must have been withing a few hours of my observing time.

The year may start off with a meteor ‘bang’ but for the next few months there is little to watch meteor-wise as no major showers occur till the Summer. The next major shower to look forward to is the Perseids of mid-August.

In the Transient Sky – January 2013

January 2013 Highlights
* Quadrantid meteor shower peaks on the morning of January 3
* Jupiter is bright in the eastern evening sky
* Jupiter and the Moon pair up on the evening of January 21
* Four comets may be brighter than 10th magnitude
* Comet C/2011 L4 (Panstarrs) approaches naked eye brightness (though it will only be visible from the southern hemisphere and will be located near the Sun)

Note: If anyone has pictures or observations of these objects/events and want to share them with my readers, send them to the Transient Sky at <transientsky1@yahoo.com>.

Planets

Evening Planets

Mars - One needs a very clear southeast horizon to catch Mars in the early evening. Glowing at magnitude +1.2 Mars is currently not as bright as other planets. But it is traveling through a patch of sky with few bright stars so it is rather apparent as the brightest, reddest, “star” in that part of the sky. It spends most of the month against the stars of Capricornus. The Moon passes near Mars on the evening of the 12th.

Jupiter – Jupiter is now a month past opposition. It spends the month slowly retrograding just north of the stars of the Hyades cluster in Taurus as it fades from magnitude -2.7 to -2.5. It is already well up in the northeast at sundown. On the evening of January 21, the Moon and Jupiter make a beautiful pair.

Morning Planets

Saturn – Saturn is an early morning object rising around 3:00 am at the start of the month. By the end of the month, Saturn rises 2 hours earlier.  All month Saturn glows at magnitude +0.6 between Virgo and Libra. The Moon passes close to Saturn on the mornings of the 6th and 7th.

Venus – Venus is approaching its next superior conjunction (when it passes by the far side of the Sun from Earth) which takes place on March 28 and enters the evening sky. This month Venus is still a morning object though it can only be seen within an hour of sunrise. On the morning of January 10th, a very thin crescent Moon is located near Venus. This will be the last month to easily see Venus until the Summer when it will reappear in the western Evening sky.

Mercury – Mercury is too close to the Sun for easy observation this month. It will be observable next month in the evening sky.

Meteors

The year is usually split in 2 with January through June having low rates with few major showers while July through December have high rates with many major showers. Meteor activity is still near an annual maximum this month.

Sporadic Meteors

Sporadic meteors are not part of any known meteor shower. They represent the background flux of meteors. Except for the few days per year when a major shower is active, most meteors that are observed are Sporadics. This is especially true for meteors observed during the evening. During early January mornings, 10 or so Sporadic meteors can be observed per hour from a dark moonless sky. The rate drops as the month progresses.

Major Meteor Showers

Quadrantids (QUA) [Max Date = January 3, Max ZHR = ~60+ per hour]

This year’s Quadrantids will peak during the morning of January 3rd. Unfortunately, a very bright Moon will be located high in the southern sky during the prime morning meteor watching hours.

The Quadrantids are the best shower that you’ve probably never heard of. It’s bad enough that this shower peaks in the middle of winter in the northern hemisphere, but it is also named after a long defunct constellation. When first identified in the early 1800s, the meteors were observed to radiate from the small faint constellation of Quadrans Muralis (the Mural Quadrant). Unfortunately, the constellation didn’t make the cut when the official list of 80 constellations was set in 1930. Today, Quadrans Muralis and the radiant of the Quadrantids can be found on the northern reaches of the constellation Bootes.

Another strike against observing the Quadrantids is their short duration. Most showers, like the Perseids and Orionids, produce high rates of meteors for a few days near their maximum. The Quadrantids are only highly active for 12-24 hours. As a result, the shower can be missed if the peak does not coincide with your early morning observing.

The peak time for this shower is always uncertain on the order of half a day or so and the IMO prediction calls for a peak at 13:30 UT on Jan 3 though this time could be off be 12 hours or more. Observers in Europe and the Americas will be well placed for seeing this year’s peak. Unfortunately observers south of the Equator will not see much from the Quadrantids.

Back in 2009 this shower put on a great show with the peak well observed from the US. Peak rates that year reached a ZHR of ~150-160. But in 2008, 2011 and 2012, rates “only” reached into the 80s. The waning gibbous Moon will be a problem as it rises around 10:45 pm and is up for the rest of the night. With the radiant only getting high enough for easy observing after 3 am the Moon will be a hindrance. Meteor watchers should try to look at a part of the sky that does not include the Moon in your field-of-view.

Minor Meteor Showers

Minor showers produce so few meteors that they are hard to notice above the background of regular meteors. Info on many minor showers are provided on a weekly basis by Robert Lunsford’s Meteor Activity Outlook.

Additional information on these showers and other minor showers not included here can be found at the International Meteor Organization’s 2012 Meteor Shower Calendar.

Comets

Naked Eye Comets (V < 6.0)

C/2011 L4 (PANSTARRS)

This comet is forecast to reach a brilliant magnitude ~-1 near its March 10th perihelion. At the time the comet only be 0.30 AU from the Sun. As bright as this is, the comet will be poorly situated close to the horizon. Still it will be a very nice binocular or small telescope sight. The comet was first seen by the Hawaiian based PanSTARRS asteroid survey on June 6, 2011 at a large distance of 7.9 AU from the Sun.

This month, the comet starts at a distance of 1.6 from the Sun though that distance will drop to 1.0 AU at the end of the month. A few recent observations place it at magnitude ~8.3. If it continues to brighten as expected it may even break 6th magnitude by the end of the month. The comet will only be observable from the Southern Hemisphere this month as it slowly moves away from the Sun against the stars of Scorpius and Corona Australis. Northern observers will have to wait till late March when the comet should be a naked eye object.

Finder charts can be found at Chasing Comets.

Ephemeris for C/2011 L4 (Panstarrs)
Date            RA        DEC    Delta   r   Elong    V
2012 Jan 01   17h 17m  -39d 17'  2.427 1.589   24    8.3
2012 Jan 11   17h 46m  -41d 23'  2.185 1.412   29    7.6
2012 Jan 21   18h 23m  -43d 31'  1.932 1.226   32    6.7
2012 Jan 31   19h 14m  -45d 15'  1.674 1.030   34    5.6

RA = Right Ascension, DEC = Declination, Delta = distance from Earth in AU
r = distance from the Sun in AU, Elong = elongation from Sun in degrees
V = Visual magnitude

Binocular Comets (V = 6.0 – 8.0)

C/2012 F6 (Lemmon)

Everyone was expecting C/2011 L4 (PANSTARRS) and C/2012 S1 (ISON) to be the two naked eye comets of 2013. No one was expecting C/2012 F6 (Lemmon) to be vying for the status of naked eye comet when it was discovered by Alex Gibbs of the Mount Lemmon survey back on March 23, 2012. At that time the comet was a faint 20th-21st magnitude and 5.0 AU from the Sun. It also appeared to be an intrinsically faint comet. So faint in fact that I though it had a good chance of disintegrating near perihelion. Instead the comet has brightened at a rapid rate. If this brightening trend continues the comet may be a faint naked eye object this February through May. Perihelion will occur on March 24, 2013 at a distance of 0.73 AU from the Sun.

Over the past few days visual observers have estimated the comet at magnitude ~8.5. I was able to observe the comet on Christmas morning at magnitude 9.6. Since there was cirrus around my estimate is probably an underestimate. The comet was rather big (6′ across) and diffuse with no sign of a tail in my 30×125 binoculars.

The comet is already too far south for most northern observers and the comet will continue to travel deeper into the southern sky this month. As a result, this comet will only be visible to southern observers till May.

The comet starts the month around magnitude 8.5 and will continue to rapidly brighten all month. By the end of the month the comet may be as bright as magnitude 6.0. It will be traveling south from Hydra through Centaurus, Crux, and Musca.

Finder charts can be found at Chasing Comets.

C2012F6_2012Dec20

Ephemeris for C/2012 F6 (Lemmon)
Date            RA        DEC    Delta   r   Elong    V
2012 Jan 01   12h 08m  -36d 30'  1.453 1.660   83    8.6
2012 Jan 11   12h 18m  -47d 42'  1.243 1.518   85    7.8
2012 Jan 21   12h 33m  -62d 08'  1.084 1.376   83    7.0
2012 Jan 31   13h 19m  -79d 22'  0.997 1.235   77    6.2

RA = Right Ascension, DEC = Declination, Delta = distance from Earth in AU
r = distance from the Sun in AU, Elong = elongation from Sun in degrees
V = Visual magnitude

Small Telescope Comets (V = 8.0 – 10.0)

C/2012 K5 (LINEAR)

This is a long-period comet discovered by the LINEAR near-Earth asteroid survey program on May 25, 2012. At the time the comet was around magnitude 17-18. Though it passed through perihelion on Nov. 28 at a distance of 1.14 AU, the comet reached its brightest last month as it rapidly approached Earth. Close approach occurred at the very end of December at a distance of 0.29 AU (27 million miles or 44 million km).

Recent visual observations place the comet around magnitude ~8.6 at the end of December. Since the comet is now moving away from the Earth and Sun this month, it should rapidly fade to magnitude ~11.4 by the end of the month. The comet is now an evening object as it moves from Auriga through Taurus into Eridanus.

I imaged the comet back on Oct. 21 with the University of Arizona’s Kuiper 1.5-m telescope. Though still over a month from perihelion and located low in the sky, the comet displayed an impressive tail and even some near-nucleus jet activity.

Finder charts can be found at Chasing Comets.

C2012K5_2012Nov21

Ephemeris for C/2012 K5 (LINEAR)
Date            RA        DEC    Delta   r   Elong    V
2012 Jan 01   06h 25m  +45d 45'  0.294 1.259  157    8.5
2012 Jan 11   04h 40m  +10d 17'  0.428 1.333  138    9.4
2012 Jan 21   04h 13m  -04d 25'  0.673 1.418  116   10.6
2012 Jan 31   04h 04m  -10d 35'  0.942 1.512  103   11.4

RA = Right Ascension, DEC = Declination, Delta = distance from Earth in AU
r = distance from the Sun in AU, Elong = elongation from Sun in degrees
V = Visual magnitude

273P (Pons-Gambart)

On June 21, 1827, French astronomers Jean Louis Pons and Jean-Félix Adolphe Gambart discovered a comet among the stars of Cassiopeia. Both men were prolific comet finders. Pons was the most prolific discoverer of comets up until the modern era and still holds the record for most visual discoveries. A record that is unlikely to ever be broken. Between 1801 and 1827, Pons found 26 comets. Comet Pons-Gambart was his second to last comet find. Though not as prolific as Pons, Gambart is credited with 5 comet discoveries between 1822 and 1834. Comet Pons-Gambart was his 3rd find.

As the comet was already a few weeks past perihelion at discovery, it was only observed for ~1 month before it faded. Over the years, orbit computers have noticed that Pons-Gambart was on an obvious elliptical orbit and determined periods between ~45 and 65 years. The only problem was with periods that short the comet should have returned at least 2 to 4 times since 1827. Perhaps the comet was fainter now or even broke up in the intervening years to explain why it was constantly being missed.

Fast forward to this year… Robert Matson of Newport Coast, CA found evidence of an unknown comet on images taken with the SOHO spacecraft. SOHO’s SWAN imager is used to map the Lyman-α emission of the solar wind. SWAN is also very good at detecting hydrogen was dissociated water molecules released by comets. As a result, SWAN has been used to discover comets. Matson noted the presence of a comet on SWAN images from Nov. 7, 10, 11, 13 and 19. He then informed a number of observers about the new find and on Nov. 29 Terry Lovejoy of Australia found the comet.

Before the comet was even formally announed, Maik Meyer of Limburg, Germany noticed the similarities between the new SWAN/Matson comet and long-lost Comet Pons-Gambart. There is little doubt that the two are related and are probably the same object. Only problem is the 2012 observations don’t exactly match the 1827 observations assuming orbital periods of 45-65 years. A recent MPEC released by Gareth Williams of the Minor Planet Center found that the 2012 observations are consistent with a much longer period than previously assumed. It is likely that Pons-Gambart wasn’t really missed before because with a 188 year orbit this is actually its first return since 1827.

At first there was still come question as to whether the newly seen comet was Pons-Gambart and for awhile the comet was only known by its designation C/2012 V4. The Minor Planet Center has now officially announced it as 273P/Pons-Gambart.

The comet has been too close to the Sun to be seen since early December. By the end of the January, the comet will be far enough from the Sun to once again be seen by visual observers as it moved through the stars of Serpens Cauda. How bright it will be at the time is still uncertain though the comet could still be brighter than magnitude 9.

Finder charts can be found at Chasing Comets.

Ephemeris for 273P/Pons-Gambart
Date            RA        DEC    Delta   r   Elong    V
2012 Jan 01   18h 51m  -09d 54'  1.770 0.843   13    8.2
2012 Jan 11   18h 45m  -05d 14'  1.773 0.911   19    8.4
2012 Jan 21   18h 38m  -00d 30'  1.728 1.007   30    8.7
2012 Jan 31   18h 31m  +04d 37'  1.646 1.120   41    9.0

RA = Right Ascension, DEC = Declination, Delta = distance from Earth in AU
r = distance from the Sun in AU, Elong = elongation from Sun in degrees
V = Visual magnitude

Quadrantids Peak Tonight

This year’s Quadrantids will peak during the morning of January 3rd. Unfortunately, a very bright Moon will be located high in the southern sky during the prime morning meteor watching hours. The American Meteor Society has a nice summary and map of the sky for this year’s Quadrantids.

The Quadrantids are the best shower that you’ve probably never heard of. It’s bad enough that this shower peaks in the middle of winter in the northern hemisphere, but it is also named after a long defunct constellation. When first identified in the early 1800s, the meteors were observed to radiate from the small faint constellation of Quadrans Muralis (the Mural Quadrant). Unfortunately, the constellation didn’t make the cut when the official list of 80 constellations was set in 1930. Today, Quadrans Muralis and the radiant of the Quadrantids can be found on the northern reaches of the constellation Bootes.

Another strike against observing the Quadrantids is their short duration. Most showers, like the Perseids and Orionids, produce high rates of meteors for a few days near their maximum. The Quadrantids are only highly active for 12-24 hours. As a result, the shower can be missed if the peak does not coincide with your early morning observing.

The peak time for this shower is always uncertain on the order of half a day or so and the IMO prediction calls for a peak at 13:30 UT (8:30 am EST, 7:30 am CST, 6:30 am MST, 5:30 am PST) on Jan 3 though this time could be off be 12 hours or more. Observers in Europe and the Americas will be well placed for seeing this year’s peak. Unfortunately observers south of the Equator will not see much from the Quadrantids.

Back in 2009 this shower put on a great show with the peak well observed from the US. Peak rates that year reached a ZHR of ~150-160. But in 2008, 2011 and 2012, rates “only” reached into the 80s. The waning gibbous Moon will be a problem as it rises around 10:45 pm and is up for the rest of the night. With the radiant only getting high enough for easy observing after 3 am the Moon will be a hindrance. Meteor watchers should try to look at a part of the sky that does not include the Moon in your field-of-view.

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