Friday, April 10, 2015

New Comet: C/2015 G2 (MASTER)

CBET nr. 4092, issued on 2015, April 10, announces the discovery of a comet (magnitude ~11) on R-band images taken by P. Balanutsa et al. with the MASTER (Mobile Astronomical System of the Telescope-Robots) 0.4-m f/2.5 reflector at the South African Astronomical Observatory.  The new comet has been designated C/2015 G2 (MASTER).

We performed follow-up measurements of this object, while it was still on the neocp. Stacking of 10 unfiltered exposures, 30-sec each, obtained remotely on 2015, April 08.8 from Q62 (iTelescope network - Siding Spring) through a 0.50-m f/6.8 astrograph + CCD + focal reducer, shows that this object is a comet with a very bright coma nearly 3 arcmin in diameter and a tail about 15 arcminutes long in PA 253.

Our confirmation image (click on it for a bigger version)




M.P.E.C. 2015-G28 (including pre-discovery MASTER observations from Mar. 30.1 UT, showing the comet at mag 11.5-11.6) assigns the following preliminary parabolic orbital elements to comet C/2015 G2: T 2015 May 23.80; e= 1.0; Peri. = 257.48; q = 0.78;  Incl.= 147.56

Below you can see a graph generated using the software Orbitas and showing the C/2015 G2 predicted magnitude (in red) versus its elongation from the Sun. Click on the image for a bigger version.


by Ernesto Guido & Nick Howes

Tuesday, March 31, 2015

New Comet: C/2015 F4 (JACQUES)

CBET nr. 4085, issued on 2015, March 31, announces the discovery of a comet (magnitude ~16) by C. Jacques on CCD images taken on 2015, March 27.2  by C. Jacques, E. Pimentel and J. Barros with a 0.28-m f/2.2 astrograph at the SONEAR Observatory (Oliveira, Brazil).  The new comet has been designated C/2015 F4 (JACQUES).

We performed follow-up measurements of this object, while it was still on the neocp. Stacking of 14 unfiltered exposures, 60-sec each, obtained remotely on 2015, March 27.7 from Q62 (iTelescope network - Siding Spring) through a 0.43-m f/6.8 astrograph + CCD, shows that this object is a comet with a sharp central condensation surrounded by a coma about 8" in diameter and a tail about 15" long in PA 237.

Our confirmation image (click on it for a bigger version)


M.P.E.C. 2015-F159 assigns the following preliminary parabolic orbital elements to comet C/2015 F4: T 2015 Aug. 8.20; e= 1.0; Peri. = 31.64; q = 1.73;  Incl.= 47.82


Below you can see the discovery images  (click on it for a bigger version)

Credit: SONEAR Observatory

by Ernesto Guido & Nick Howes

Thursday, March 26, 2015

New Comet: C/2015 F2 (POLONIA)

CBET nr. 4083, issued on 2015, March 26, announces the discovery of a comet (magnitude ~17) by R. Reszelewski, M. Kusiak, M. Gedek and M. Zolnowski on CCD images taken on 2015, March 23 with a remote-controlled 0.1-m f/5 astrograph of the Polonia Observatory at San Pedro de Atacama, Chile, in the course of their comet-search program. The new comet has been designated C/2015 F2 (POLONIA).
 
We performed follow-up measurements of this object, while it was still on the neocp. Stacking of 14 unfiltered exposures, 30 seconds each, obtained remotely on 2015, March 23.8 from Q62 (iTelescope network - Siding Spring) through a 0.43-m f/6.8 astrograph + CCD, shows that this object is a comet with ill-defined central condensation surrounded by diffuse irregular coma 15" in diameter.

Our confirmation image (click on it for a bigger version)


M.P.E.C. 2015-F120 assigns the following preliminary parabolic orbital elements to comet C/2015 F2: T 2015 Apr. 28.77; e= 1.0; Peri. = 351.97; q = 1.21;  Incl.= 28.87

by Ernesto Guido & Nick Howes

Monday, March 16, 2015

Bright Nova in Sgr - (PNV J18365700-2855420)

Following the posting on the Central Bureau's Transient Object Confirmation Page about a possible bright Nova in Sgr (TOCP Designation: PNV J18365700-2855420) we performed some follow-up of this object remotely through a 0.61-m f/6.5 astrograph + CCD) of  iTelescope network (MPC Code  U69 - Auberry, California - USA).

On our images taken on March 16.5, 2015 we can confirm the presence of an optical counterpart with R-CCD magnitude 5.9 at coordinates:

R.A. = 18 36 56.85, Decl.= -28 55 40.0 (equinox 2000.0; UCAC-4 catalogue reference stars).

Our wide-Field colour image of Nova Sagittarii 2015 No. 2. Details on the caption. Click on the image for a bigger version.


Click here or on the thumbnail below to see the full wide-field frame with the nova at the center.


Our annotated confirmation image. Click on it for a bigger version.


An animation showing a comparison between our confirmation image and the archive POSS2/UKSTU plate (R Filter - 1996). Our image was obtained when the object was only about +15 degree on the horizon. Click here or on the thumbnail below for a bigger version:

Possible Nova in Sgr - 16 March 2015 photo 
PNV_SGR_16_March_Guido_U69_T24_animation_zpse5moqno2.gif

According to the Atel #7230 "an optical spectrum of PNV J18365700-2855420 (see CBAT TOCP) was obtained using the FRODOspec spectrograph on the Liverpool Telescope at 2015 March 16.27 UT. The spectrum shows strong Balmer series emission exhibiting P Cygni profiles with velocities of ~2800 km/s. Numerous Fe II emission lines (also with P Cygni profiles) are also seen, along with O I, Si II and Mg II features. This confirms that PNV J18365700-2855420 is a bright classical nova of the Fe II spectral type"

by Ernesto Guido & Nick Howes

Friday, February 13, 2015

Possible Nova in Sco - (PNV J17032620-3504140)

Following the posting on the Central Bureau's Transient Object Confirmation Page about a possible Nova in Sco (TOCP Designation: PNV J17032620-3504140) we performed some follow-up of this object remotely through a 0.50-m f/6.8 astrograph + CCD + f/4.5 focal reducer) of iTelescope network (MPC Code  Q62 - Siding Spring).

On our images taken on February 13.7, 2015 we can confirm the presence of an optical counterpart with R-CCD magnitude 8.6 at coordinates:

R.A. = 17 03 26.19, Decl.= -35 04 18.1

(equinox 2000.0; UCAC3 catalogue reference stars).

Our annotated confirmation image. Click on it for a bigger version:


An animation showing a comparison between our confirmation image and the archive POSS2/UKSTU plate (R Filter - 1991). Click here or on the thumbnail below for a bigger version:

Possible Nova in Sco - (TOCP Designation: PNV J17032620-3504140) - 2015, February 13.7 photo ezgif.com-crop_zpsorqoizoh.gif

by Ernesto Guido & Nick Howes

Friday, January 23, 2015

Close Approach of Asteroid (357439) 2004 BL86

The asteroid (357439) 2004 BL86 was discovered  (at ~ magnitude +18.6) on 2004, January 30 by Linear Survey (MPC code 704) with a 1.0-m f/2.15 reflector + CCD.

Asteroid (357439) 2004 BL86 has an estimated size of 420 m - 940 m (based on the object's absolute magnitude H=19.0) and it will have a close approach with Earth at about 3.1 LD (Lunar Distances = ~384,000 kilometers) or 0.0080 AU (1 AU = ~150 million kilometers) on 2015, January 26 at 16:20UT. This asteroid will reach the peak magnitude about +9.0 between Jan 26 & 27. Astronomers at Goldstone will try to observe it "as the radar signal-to-noise ratios will be very strong and will provide an extraordinary opportunity to study this object". 

This flyby of 2004 BL86 will be the closest by any known space rock this large until asteroid (137108) 1999 AN10 (absolute magnitude H=17.9) flies past Earth in 2027 within one lunar distance. On April 2017, another asteroid "2014 JO25" (absolute magnitude H=18.1) will pass at about 4.8 LD from Earth.

We performed some follow-up measurements of this object on 2015, January 23.4, remotely from the Q62 iTelescope network (Siding Spring, Australia) through a 0.43-m f/6.8 astrograph + CCD). Below you can see our image taken with the asteroid at about magnitude +15 and moving at ~ 10.51 "/min. The asteroid is trailed in the image due to its fast speed. At the moment of its close approach on Jan 26, around 16:20UT, (357439) 2004 BL86 will move at ~ 162 "/min (or about  2.7 deg/hour). Click on the image below to see a bigger version. (North is up, East is to the left).


Click here or on the thumbnail below to see a short animation showing the movement of (357439) 2004 BL86 (two consecutive 120-second exposure). (North is up, East is to the left)

Animation of Asteroid (357439) 2004 BL86 on January 23, 2015 photo ezgif.com-crop_zpsxljxpdkv-1-1.gif

The graphic below depicts the passage of asteroid (357439) 2004 BL86 past Earth on January 26, 2015.  The view is nearly edge-on to the Earth's orbit; the Moon's nearly circular orbit is highly foreshortened from this viewpoint. The asteroid moves from the south to the north, from below the Earth's orbit to above. Times indicated on the graphic are Universal Time. Click on the image for a bigger version.

Credit: NASA/JPL-Caltech

When 2004 BL86 will reach the peak magnitude +9 on the evening between January 26-27, it should be visible for several hours in small telescopes if you know where to look. The image below shows its path in the sky in those days. When brightest, it will be in the constellation Cancer. A more detailed map is available here.

Credit: Sky & Telescope

UPDATE - January 26, 2015

Scientists working with NASA's 70-meter Deep Space Network antenna at Goldstone, California, have released the first radar images of asteroid (357439) 2004 BL86. The images show that this asteroid has its own small moon. The signature of the satellite was seen in lightcurve data reported earlier by J. Pollock (Appalachian State University, North Carolina) and  P. Pravec (Ondrejov Observatory, Czech Republic) and then confirmed by radar.

"The primary body is approximately 325 meters across and has a small moon approximately 70 meters across. In the near-Earth population, about 16 percent of asteroids that are about 200 meters or larger are a binary (the primary asteroid with a smaller asteroid moon orbiting it) or even triple systems (two moons). The resolution on the radar images is 4 meters per pixel."

Below you can see the animation made by using 20 radar images obtained at Goldstone and showing asteroid (357439) 2004 BL86 and its moon. Click on the animation to see a bigger version.

Credit: NASA/JPL-Caltech

by Ernesto Guido, Nick Howes & Martino Nicolini

Monday, January 19, 2015

Comet C/2014 Q2 (Lovejoy) puts on a show

Comet C/2014 Q2 (Lovejoy) was discovered (at magnitude +14.8) by T. Lovejoy (Birkdale, Qld., Australia) on 17 August 2014 on CCD images obtained with a 20-cm f/2.1 Schmidt-Cassegrain telescope. It is the fifth comet discovered by Terry Lovejoy.

On 7 January 2015, comet C/2014 Q2 passed 0.469 AU (1 AU = ~150 million kilometers) from Earth and it will reach the perihelion (closest approach to the Sun) on 30 January 2015 at a distance of 1.29 AU from the Sun. Comet Lovejoy reached few days ago its peak brightness at about magnitude +3.8, as bright as it should get, making it a naked-eye object. It is currently still at about magnitude +4.3. See below an updated light-curve.

Credit: S. Yoshida

Comet C/2014 Q2 (Lovejoy) puts on a great show on January’s evening sky, with its very long, structured and rapidly changing ion tail. Below an image of comet C/2014 Q2 taken on 14 January 2015. More info on the caption. Click on it or here for a bigger version

Credit: E. Guido
Credit: E. Guido

Below an image of comet C/2014 Q2 taken on 16 January 2015. Click on it for a bigger version.

Credit: Nick Howes/Tzec Muan Observatory

Below a finder chart to help you locate this comet during January 2015. The dates are in Universal Time; the ticks are at 0:00 UT. Click on it for a bigger version.

Credit: Sky & Telescope

by Ernesto Guido, Martino Nicolini & Nick Howes