Saturday, 16 December 2017

3200 Pheathon

Click on image to enlarge
Object: 3200 Pheathon
Type: Asteroid 
Distance: 0.0797 AU (11.9 million km) 
Constellation: Perseus/Andromeda
Date: 14 December 2017
Equipment: SXV-H9, Vixen 114mm f5.3 ED refractor
Subframes: 322 x 3s, 17s between frames

The above image shows the track of NEO (Near Earth Object) 3200 Pheathon (pronounced Fay-Ath-On - I think!) as it crossed the Perseus/Andromeda border during the early evening of 14th. December. The field is about a degree wide (52' to be precise).

Images were acquired in Astroart, with selected frames stacked and time-annotated in PaintShopPro. Magnitude of the asteriod appeared to be around 10.7 when compared with similarly bright stars in the image.

The three brightest stars in the image have been labelled by way of positional reference.


Above is a GIF animation using all 322 frames, showing the progression of the asteroid.  A stray meteor crosses the field about a second into the video. I don't think it's a satellite (couldn't find evidence of one in the region at the time from various web searches) or a Geminid (wrong radiant).

3200 Phaethon (1983 TB) was discovered on Oct. 11 1983 by NASA's Infrared Astronomical Satellite (IRAS). Phaethon is the third largest near-Earth asteroid classified as "Potentially Hazardous" after 53319 1999 JM8 (~7 km) and 4183 Cuno (~5.6 km). At over 3 miles wide and moving at 20 km/s, one can only imagine the devastation that this potential "dinosaur killer" might cause were it to strike the UK.

Probably not as much as Brexit of course, although unlike Brexit, there is no risk of such an impact coming to pass in the foreseeable future.

Phaethon is categorized as an Apollo asteroid, as its orbital semi-major axis is greater than that of the Earth's at 1.27 AU (190 million km). It is also suspected to be a member of the Pallas family of asteroids.

Phaethon has an unusually high eccentricity of 0.890 and a perihelion (closest approach to the Sun) of 0.140 AU, the smallest known in the near-earth asteroid population. Its surface temperature at perihelion reaches around 750 C.

Due to the close perihelion, Phaethon is named for the Greek mythological son of Helios (the Sun god). In Greek mythology, Phaethon drove his father's chariot for one day, lost control of its horses, and nearly set the Earth on fire.

On December 16, at its closest approach, the asteroid was only 6.4 million miles (10.3 million kilometers) away, the nearest it will be until 2093. The radar images below were taken by the Arecibo Observatory Planetary Radar during its close fly-by, and have allowed astronomers to distinguish details of its surface.





These images, captured at a resolution of 250 feet (75 meters) per pixel, show the asteroid to be spheroidal in shape, with a diameter of roughly 3.6 miles (6 kilometers). The researchers also used Arecibo’s radar to spot a depression near 3200 Phaethon’s equator that stretches a few hundred meters at minimum, as well as a dark, spherical spot close to one of the asteroid’s poles.

Phaethon’s highly eccentric orbit more closely resembles that of a comet than an asteroid; it has been referred to as a "rock comet".

Phaethon is widely thought to be the parent body for the Geminid meteor stream due to similarities between its orbit and that of the meteors. Most meteor streams are associated with comets, suggesting that Phaethon may be an inactive comet nucleus, although in recent studies performed by NASA's STEREO spacecraft, dust tails have been observed and in 2010, Phaethon was detected ejecting dust.

Saturday, 9 December 2017

M33 - The Triangulum Galaxy

Click on image to enlarge

Object: Messier 33 (NGC 598/604)
Type: Spiral galaxy 
Distance: 3,000,000 light years 
Constellation: Triangulum
Date: 25 November & 07 December 2017
Equipment: SXV-H9, Vixen 114mm f5.3 ED refractor, guiding with Lodestar X2/PHD
Subframes: 50 x 300s luminance (via an Astronomix CLS filter), 20 x 80s 2x2 binned each for Ha, RGB

Images acquired, pre-processed and stacked in Astroart.  Digital development and high/low pass filters applied, colour composited all in Astroart.  Final cosmetic processing (cropping, mild edge preserving smooth for noise) in PaintShop Pro.

The bright red patch at upper right centre is NGC 604, the brightest of the numerous H-alpha emission regions in this galaxy.  This image could have probably done with longer luminance subs as the outer arms are not as well defined as I would have liked.  I had previously imaged M33 in "white light" and actually got better luminance data with shorter exposures, suggesting that the CLS filter wasn't actually helping

More information about this object can be found here.

A 40mm eyepiece on the ED114 shows M33 up as a definite central glow fading to a less obvious oval, featureless glow about half the size of the full moon. This seems to equate to the brighter inner arms as shown in the image above. Visually, I can't see any hint of spiral structure.

Sunday, 12 November 2017

The Bubble Nebula NGC 7635


Object: NGC 7635 (Caldwell 11)
Type: Emission Nebula
Distance: 7100 light years 
Constellation: Cassiopeia
Date: 5&6 November 2017
Equipment: SXV-H9, Vixen 114mm f5.3 ED refractor, guiding with Lodestar X2/PHD
Subframes: 42 x 300s H-alpha as luminance, 12 x 75s 2x2 binned each for RGB

Images acquired, pre-processed and stacked in Astroart.  Digital development and high/low pass filters applied, colour composited all in Astroart.  Final cosmetic processing (cropping, mild edge preserving smooth for noise) in PaintShop Pro.

More information about this object can be found here...

A faint trace of nebulosity around the bright star inside the Bubble can just be seen with the ED114 and a 25mm eyepiece. Larger aperture scopes don't really reveal any more details, at least not to me.

Wednesday, 1 November 2017

Open Cluster M52...

Open Cluster in Cassiopeia: Messier 52
Object: Messier 52 (NGC 7654)
Type: Open Cluster 
Distance: 5100 light years 
Constellation: Cassiopeia
Date: 27 October 2017
Equipment: SXV-H9, Vixen 114mm f5.3 ED refractor
Subframes: 12 x 150 second luminance, 6 x 40 second 2x2 binned each for RGB

Images were acquired, stacked and colour-composited in AstroArt.  Final cosmetic processing was in PaintShop Pro.

This was really just a test of PHD guiding, which I had never used before and which worked just fine, first time.

Visually, this cluster is a real treat through the ED114 and a 15mm eyepiece, looking pretty much as it does in the image given a dark sky.

Friday, 19 May 2017

Jupiter and Io...

This image represented "first light" from my observatory...


Date: 19 May 2017 @ 21.00hrs BST
Equipment: Phillips TouCam Pro II, Celestron C9.25, Vixen x2 Barlow
Subframes: 1 minute @ 20fps, AVI output stacked and sharpened in Registax 2.1.14.

This was really just a test to make sure that the observatory electrics were working and all of the software and hardware were talking to each other.  As it worked out, EQASCOM and SkyMap Pro 9 worked well enough to get Jupiter showing in the finder scope first time, with but a few small tweaks to get the image onto the tiny web cam chip.

Jupiter was only 34 degrees above the southern horizon at the time, and the seeing was pretty unsteady.
Nevertheless, the magic of the Registax processing software recognised enough decent subframes and put them together to give a reasonably decent view.  There are much more recent versions of this magical bit of freeware available, but I like the simplicity of the 15 year old version I have, and for the little bit of planetary imaging I do, it works just fine.

Jupiter's closest moon, Io, was hardly visible on the original image so I took it back into PaintShop Pro to stretch and sharpen it up to make it match the view through the eyepiece.