Monday, July 20, 2009

New Impact on Jupiter?

Starting from July 19, 2009 rumors appeared all over the astronomical internet community about a possible new impact on Jupiter.

A new dark spot was just discovered by Australian amateur astronomer Anthony Wesley on Jupiter surface. He noticed it on his images taken with his 14.5" newtonian aroud 1300UTC of 19th July. The same area was imaged by Wesley 2 days before and the dark spot wasn't there. This new dark spot shares a strikingly resemblance with the impact marks made on Jupiter by comet Shoemaker-Levy 9 when it crashed into the giant planet in 1994 (just in these days is recurring the 15th anniversary of the impacts of the comet Shoemaker-Levy 9 fragments on Jupiter, dated 16-22 July 1994).

Below the Wesley images of the new dark spot (click on the image for a bigger version)



For comparison below you can see a SL9 impact image dated back to 1994 (click on the image for a bigger version)



After the announcement on Wesley website, other amateur astronomers have been able to confirm the dark spot. Anyway the shape alone of this dark spot, was not enough for the impact nature to be confirmed. In favour of the impact hypothesis: the location of this new dark spot, near the Jupiter South Pole where usually storm activity is minor and the fact that the location was featureless in the images of 2 days earlier.

But a more resolutive proof is the Near-IR or methane-band imaging. Material from an impact should be stratospheric and hence should appear bright at these wavelengths.

A confirmation that arrived few hours ago. Leigh Fletcher, planetary scientist at Pasadena, was twittering live about this event and the work he and his colleagues were doing with IRTF.  Below are some of his tweets:

"We're now almost certain it's an impact event, extremely exciting!"

"Working with Glenn Orton, we're acquiring spectra of the impact site
with IRTF/SpeX. Very bright in refl. sunlight, high altitude
particles"

"The impact site on Jupiter is rotating into view on the IRTF, we're
imaging with Spex, have acquired spectra. VERY bright feature!!"

"New instrument for looking at Jupiter impact site: IRTF/MIRSI,
probing thermal characteristics of the impact location."

"This has all the hallmarks of SL-9 in 1994 (15 years to the day!). High altitude particulates, looks nothing like weather phenom"


While this is a note appeared on mpml mailing list by Franck Marchis (Astronomer at University of California at Berkeley):

"We observed Jupiter with the Keck telescope and its NIR camera and we confirm that the feature is unusual because of its brightness in the CH4 band. It is most likely a impact explosion in the upper atmosphere of Jupiter. We are processing the data right now and will beginning the analysis"

While waiting for an official release by professional astronomers confirming the impact event definitively, it's interesting to report this comment by astronomer Alan Fitzsimmons:
"it is no surprise that if an asteroid or inert comet had hit Jupiter recently we might not know about it. A 1-km diameter asteroid or inactive comet at that distance is roughly magnitude V=25 to 26 (100 thousand million times fainter than Jupiter itself), much too faint to pick up. SL-9 was only found because it had activated through tidal disruption - we now know that it had probably been in orbit around Jupiter since the 1930’s, but no-one picked it up because of its faintness"

Congratulations to Anthony Wesley for his finding!!!


by Ernesto Guido

Thursday, June 18, 2009

New Comet P/2009 L2 (YANG-GAO)

IAUC Circular No. 9052, issued on 2009, June 16, announces the discovery by Rui Yang and Xing Gao of a new comet on several survey images taken by Gao in the course of the Xingming Comet Survey at Mt. Nanshan using a Canon 350D camera (+ 10.7-cm f/2.8 camera lens).

We have been able to confirm this object while it was posted in the NEO-CP, both from mpc code H06 & E16. Co-adding of 10 unfiltered exposures, 60 seconds each, obtained remotely near Mayhill (NM) on 2009, June 16.4 through a 0.25-m, f/3.4 reflector + CCD showed a coma about 40 arcsec in diameter, and a tail nearly 90 arcsec long toward PA 245 deg.

Here you can see our confirming image:



An MPEC with a preliminary orbital elements and an ephemeris has been issued too:

http://www.cfa.harvard.edu/mpec/K09/K09M05.html

The first preliminary orbit for comet P/2009 L2 (Yang-Gao) indicates perihelion already on May 19, 2009, at about 1.3 AU. The period is about 6.6 years.

This is the third amateur discovery in 2009, and the second for the Xingming Survey.

Congratulations to our chinese fellow observers for this new find.

by Ernesto Guido, Giovanni Sostero, Paul Camilleri & Enrico Prosperi

Friday, May 22, 2009

Recovery of 107P/Wilson-Harrington = (4015) Wilson-Harrington

MPECs 2009-K24 & 2009-K27, issued on 2009 May 21 & 22, reports our recovery of comet 107P/Wilson-Harrington, obtained over three consecutive nights: on 2009, May 19 and 20 from Mayhill (NM) through a 0.25-m, f/3.4 reflector + CCD (details on image):



and on 2009, May 21, by means of the 0.61-m f/10 reflector + CCD of the Sierra Stars Observatory, Markleeville (CA).

This object has an interesting story, since its cometary nature (a tail without coma) has been reported only once, at the time of its discovery, so its activity appears to be rather irregular:

http://cometography.com/pcomets/107p.html
http://www.aerith.net/comet/catalog/0107P/index.html
http://en.wikipedia.org/wiki/107P/Wilson-Harrington

Also in our current stackings, the object appears perfectly stellar, with no trace of any coma or tail. Comet107P/Wilson-Harrington was last observed on 2007, March 13 by the Mt. Lemmon Survey.

Ernesto Guido, Giovanni Sostero, Paul Camilleri & Enrico Prosperi

Monday, May 18, 2009

Update about comet 19P/Borrelly

Further follow up performed by the undersigneds with the same instrumental set-up of our previous report (but with 600-sec total integration time) on 2009, May 17.21, shows that the secondary condensation (or knot) that has been reported on comet 19P/Borrelly (see our previous post) has significantly weakened, with an aspect extremely diffuse and elongated compared to our previous observation of May 15.21.

On May 17.21 the optocenter (difficult determination) of this feature had a displacement of about 4 arcsec in PA 301 with respect to the central condensation of 19P/Borrelly.

Our image is available here:

http://tinyurl.com/qnvpvw


Giovanni Sostero, Paul Camilleri, Enrico Prosperi & Ernesto Guido

Friday, May 15, 2009

Secondary condensation on 19P/Borrelly

Prompted by an alert note of Bernhard Haeusler, posted in the newsgroup [Comets-ml] on May 11, 2009 about a possible secondary "condensation" in 19P/Borrelly, we performed some follow-up about this comet.

Images obtained by the undersigneds on 2009, May 15.21 with the 0-61-m Cassegrain + CCD of the Sierra Stars Observatory (Maarkleville, CA) confirms the presence of a tailward, diffuse, secondary condensation or "knot", placed about 4.7 arcsec in PA 301 from the primary central condensation. This feature is nearly 1.5 magnitude fainter compared to the central condensation itself. Image processing techniques (azimuthal median subtraction of the inner coma) enhances the visibility of this detail.

Our image is available here:

http://tinyurl.com/qendnd


Comparing the offset data posted in the same blogspot by B. Hausler (May 7: 13 arcsec in PA 310) and F. Kugel (May 10: 8 arcsec PA 305), this feature apparently approaches the central condensation; however some foreshortening effect might be under course, also considering the fact that, on about 2009 June 5th, Earth will cross the orbital plane of this comet.

Paul Camilleri, Enrico Prosperi, Giovanni Sostero & Ernesto Guido

Wednesday, May 13, 2009

Possible Nova in Centaurus 2009

Following an alert note posted today by Grzegorz Pojmanski in the vsnet-alert newsgroup about a possible nova in Cen, on 2009 May. 13.57 we performed some follow-up of this object remotely through a 0.25-m, f/6 Ritchey-Chretien + CCD, from the RAS Observatory (Moorook, Australia).

We can confirm the presence of an optical counterpart with unfiltered CCD magnitude about 8.6 (UCAC-2 Catalogue refernce stars) at coordinates:

R.A. = 13h31m15.77s, Decl. = -63o57'38".6 (equinox 2000.0; UCAC-2 catalogue reference stars).

Comparison with an Anglo-Australian Observatory Schmidt red plate (limiting magnitude about 20), obtained on 1997, Feb. 05, show that this position is nearly coincident with a field star, whose position end figures are 15s.68, 38".6, and magnitude about 15 (however, the extreme stellar crowding due to nearby field stars, makes this measurement rather difficult).

Our image of this transient is available at the following URL:

http://tinyurl.com/qlbesc

UPDATE

This nova has been designated V1213 Cen. For more info see also this paper on NATURE.


by Ernesto Guido and Giovanni Sostero

Monday, April 20, 2009

Recovery of comet P/2002 LZ11 (LINEAR) = P/2009 H1 (LINEAR)

IAU Circular No. 9039, issued on 2009 Apr 19, announces our recovery of P/2002 LZ_11 (LINEAR), now designated P/2009 H1 (LINEAR); it was last observed in January 2004 (MPC code #372, Geisei).

After several frustating and unsuccessful tryings due to moonlight interference and stellar crowding (the searched comet was in Sgr) we initially picked-up P/2002 LZ11 on 2009, Apr. 17.45 through a remotely controlled telescope of the GRAS network (details on image):


In our stacking the comet was located about 4 arcmin to the East-Northeast of the ephemerids position: co-adding of 25 unfiltered exposures, 120 seconds each, through a 0.25-m, f/3.4 reflector + CCD, revealed the presence of an extremely compact coma, about 12-arcsec in diameter, and a short tail nearly 25-arcsec long toward West.

We tried further follow-up on April 18 from the same site and from the Skylive-Grove Creek Obs. (MPC #E16), however our efforts were hampered due to the star crowding and to the unsuitable observing conditions (a magn. 19 comet seen through amateurs instrumentation, needs a pretty good sky).

Hopefully we were more lucky using the 0.37-m, f/14 reflector + CCD of the Iowa Robotic Observatory near Sonoita, AZ ((MPC# 857) over the same night: co-adding of 20 unfiltered exposures, 120 seconds each, showed the presence of a tiny coma about 8-arcsec in diameter, with a faint extension toward West (two bright field stars were interfering with the detection of the small tail we had recorded well the day before). Our image is available here:



According to the orbital elements published so far by the Minor Planet Center website (http://tinyurl.com/cqnamw), perihelion will occur on March 2010, with the comet at 2.4 AU from the Sun. This Jupiter-family comet moves along an elliptic orbit in about 7 years, having a semi-major axis of 3.7 AU, eccentricity of 0.35 and an inclination of 11.5 deg.


Ernesto Guido, Giovanni Sostero, Paul Camilleri and Enrico Prosperi