Comet 178P Returns

Farpoint’s 1999 comet discovery returns for the third time.

The comet discovered by Graham Bell and I (C/1999 X1) at Farpoint in December 1999 and was subsequently number 178P by the Minor Planet Center has been recovered for the third time. Each orbit takes 7 years to go around the sun. This recovery image Is a stack of 20 – 30 second images taken at Sandlot Observatory the morning of 8-1-2020.

Comet C/2019 Y4 disintegration

Comet C/2019 Y4 held promise to be a spectacular comet, possibly visible to the naked eye in May 2020. Unfortunately as a lot of comets passing close to the sun, Comet C/2019 Y4 is beginning to disintegrate. This image of the comet was taken the evening of April 9th, (April 10 U.T.) with the Little Blue 22″ at Sandlot Observatory.

You can see the small star-like piece that has broken away from the main nucleus. It is located just left and above the rest of the nuclear region. Once the flurry of activity subsides the comet will not likely become any brighter an average passing comet of roughly 9th to 10th magnitude.

Image Details;

22″ f4.1 reflector imaging at prime focus with a ST10XME CCD Camera. The image was comprised of a stack of 24 – 30 second images . Each image was offset in the direction of the comet’s motion via Astrometrica. The image above was cropped out of the original 22 x 14 arc-minute field of view.

image taken 4-15-20. about 3 U.T. from Sandlot Obs.

C/2019 Y4 Image taken Apr 15 – changing fragmentation . There are now several components to the nucleus. One bright fragment in the left and a smaller fragment just below the bright one (barley discernible in the image) and a fainter condensation further toward the tail.

Interstellar Comet?

There is a comet-looking object on the NEOCP that is likely the next interstellar to enter our solar system. The object is temporarily designated as gb00234. It was discovered by L51 Margo observatory a couple of nights ago. Here is a rather
poor image taken just as dawn was breaking on 09-11-19.
The image is a composite of 3 – 1 minute images taken with an ST10 XME camera mounted on the 0.57meter Little Blue Reflector. It will be interesting to see what media does with this.

Gary Hug

M87’s black hole

Here’s M87 taken with my 22″ Reflector and an ST-8 CCD camera. The image show the jet of material traveling at some percentage of the speed of light while being squeezed out before reaching the event horizon . This does correlate with the black hole at M87 center that was recently ‘imaged’ and publicized. The ST-8 image taken at Sandlot Observatory was imaged on 04-02-19.

M87’s black hole ejection

This image by the Event Horizon Telescope project shows the event horizon of the supermassive black hole at the heart of the M87 galaxy. Credit: EHT Collaboration

Asteroid 6478 Gault sprouted a tail.

A long known asteroid suddenly sprouted a long narrow tail. This is a 22 minute (45 secs  x 30) cropped imaged taken with the Tombaugh Reflector at Farpoint 01-10-19 about 8:00 U.T.   The tail was visible faintly in each of the 45 second images.  This asteroid may have developed the tail through an impact with another rock.   [T08] ATLAS Mauna Loa images 1-5.5 U.T. showed  a comet like tail extending from the asteroid and  comments started flowing  on  mpml  and comet ml  list servers.    A couple of months ago it went through a 2 magnitude outburst and is still at that level as of last night.  

NEO Follow-up Targets

I originally thought A/2018 V3 was an asteroid (although it may end up being a comet) with a very long perihelion distance. But I was wrong; its max distance is just 4 A.U.’s but the eccentricity is .989( 99 times longer than wide orbit) and its inclination to the solar system is 165 degrees (almost perpendicular.)
Anyway some of the objects in our NEO follow-up program are as faint or even a bit dimmer than 21.5 V magnitude. Even with the arrow pointing to the object its hard to see.  Only with consistent movement in the predicted angle is it identifiable as a target.   This image is a combination of 14 – 2minute images taken on the night of 11-14-18 and severely  cropped.   At the time the MPC listed it as 21.6 V magnitude. It would also be easier to see inverted (dark stars on  white background) .

Gary

Comet 21P Giacobini-Zinner returns

This 5 minute image of the returning comet 21P (Giacobini-Zinner) was taken Sept 16, 2018 using a Cannon EOS coupled to an Apogee 80mm F6.25 refractor.    The mount was a SST EQ-25 HPFD .   At the time of this image,  the comet was in the middle of the constellation Auriga.

Peter Birtwhistle

During a recent visit to England I had an opportunity to visit with Peter Birtwhistle at his home at Great Shefford. Peter is  one of the most prolific observers for NEO follow-up in the world.    Here we are in front of his backyard observatory (MPC J95) which houses a 16″ LX200 SCT  in the small town of Great Shefford.   He has developed his own software that allows manipulating image files to produce accurate results of NEO targets.

Peter Birtwhistle and I at his backyard observatory in Great Shefford, England.

 

NGC 7331

This is an image  taken just before dawn 07-11-18 with the new (to us) STL 6303E camera mounted on the Tombaugh  .7 meter Reflector at 2 bin pixels ( 18 micron).

 

Gary

 

Sun image 6-13-17

Today’s sun

There’s a small sunspot just left of top- center of the image.
Taken with an 80mm  f/6 Apogee Refractor and a Cannon EOS.
ISO 100 – 1/500th second.

Thousand oaks Mylar solar filter in front of the lens.