Friday, 30 October 2026

NGC 7332 and NGC 7339, Galaxies in Pegasus

 

Edge on Galaxies, NGC 7332 and NGC 7339. PIRATE robotic telescope, Tenerife. BVR filters. Data Credit: Open Observatories, Open University, telescope.org. Image processing: Pip Stakkert at the JPO.

"These two galaxies are NGC 7332 and NGC 7339, a visually striking pair located approximately 67 million light-years away in the constellation Pegasus.   

NGC 7332 (Right): A bright, edge-on lenticular galaxy is noted for its distinct "peanut-shell" boxy bulge created by an internal stellar bar.   

NGC 7339 (Left): An edge-on spiral galaxy forms a gravitationally bound, interacting pair with NGC 7332". - Gary Gemini Coms Manager at the JPO. 




The Cat's Head Nebula in the Constellation Carina

 

" It is an absolute shame that the Constellation Carina, visible from the Southern Hemisphere, cannot be seen from the Jodrell Plank Observatory, located in the United Kingdom. There are just so many interesting objects to image in this constellation. Kurt is a regular reader of the NASA internet site and was much impressed by this James Webb Telescope image of the Cat's Head Nebula. The following is the NASA description copied from the site. We would recommend visiting the NASA website where there are more related images and videos" - Joel Cairo CEO of the JPO the UK's most easterly Astronomical Observatory. 

Cat’s Head Nebula (Webb MIRI Image)

Mid-infrared image of the Cat’s Head Nebula by the James Webb Space Telescope. A bluish-gray filament of dust is in the center, stretching from the bottom to almost the very top. It has a narrow, irregular shape that resembles a cat sitting with its back toward the viewer and a tail extending downward. The tail ends at the lower one-third of the image and widens to a triangular peak of dust. The cat’s head is turned toward the right, revealing a white glowing eye. The background is mostly red, with the top left and right corners revealing the black background of space. On the cat’s left is a dome-shaped grouping of faint filaments of dust. Scattered throughout the view are yellow and blue stars, some with Webb’s signature eight-point diffraction spikes.

In NASA’s James Webb Space Telescope’s mid-infrared image, emission from warm dust and carbon-based molecules excited by starlight outlines intricate structures within the nebula. Changes in local conditions and compositions cause variations in color and brightness. Fine strands and globules are especially apparent to the left of the main pillar.

To the right of the pillar, a bright yellow light source is seen against reddish mid-infrared emission, probably an infant star embedded in dust. A narrow filament appears to cross the likely star, although its physical relationship to the star is not established. Several blue stars are scattered throughout, some with Webb’s characteristic diffraction spikes.

About the Object

R.A. Position

10:45:59.76

Dec. Position

-60:06:23.76

Constellation

Carina

Distance

7,500 - 8,500 light-years

Dimensions

Image is about 5.3 arcmin across (about 12.3 light-years)

About the Data

Data Description

This image was created with Webb data from proposal: 12591 (M. Garcia Marin).

Instrument

MIRI

Exposure Dates

May 27, 2026

Filters

F770W, F1130W, F1500W

Object Name

NGC 3372; HH 903; Cat's Head Nebula; Carina Nebula

Object Description

Star forming region; Emission Nebula; HII region

Release Date

October 29, 2026

Science Release

Ghostly Cat’s Head Nebula Lurks Within Sight of NASA’s Hubble, Webb

Credit

Image: NASA, ESA, CSA, STScI; Image Processing: Joseph DePasquale (STScI)

Mid-infrared image of the Cat’s Head Nebula by the James Webb Space Telescope. A bluish-gray filament of dust is in the center, stretching from the bottom to almost the very top. It has a narrow, irregular shape that resembles a cat sitting with its back toward the viewer and a tail extending downward. The tail ends at the lower one-third of the image and widens to a triangular peak of dust. The cat’s head is turned toward the right, revealing a white glowing eye. The background is mostly red, with the top left and right corners revealing the black background of space. On the cat’s left is a dome-shaped grouping of faint filaments of dust. Scattered throughout the view are yellow and blue stars, some with Webb’s signature eight-point diffraction spikes.

Color Info

This image was acquired by the MIRI instrument on the Webb Space Telescope. Several filters were used to sample varying wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue=F770W, Green=F1130W, Red=F1500W


Thursday, 29 October 2026

Double Cluster NGC 869 and NGC 884 in the Constellation Perseus

 

Two versions of the Double Cluster
captured with the JPO Seestar S30 in EQ mode
 by Kurt Thrust


" The Double Cluster is a delight to see through the eyepiece of a widefield telescope. It is however, very difficult to photograph it's visual splendour. We have imaged this Northern Hemisphere astro-highlight a number of times using different telescope-camera set-ups. We believe this most recent image, obtained with the little Seestar S30 is our best to date". - Joel Cairo CEO of the Jodrell Plank Observatory.



Tuesday, 27 October 2026

More Clean Room Activity

 

Completed Seestar Spectrometers in dust proof cases. Each with a desicant sachet. Refurbished 500 lines/mm spectrometer for attachment at eyepiece end of the JPO's 127mm. and 66mm. Refractor telescopes.




Spectra captured on 27-10-2026 using the Seestar S30 and the 50 lines per mm Spectrometer. (Late additions).

"Jolene has done her bit and we hope, weather permitting, to use the Seestar S30 tonight to capture some stellar spectra with the 50 lines per mm. spectrometer". If all works well, we will upload images captured to this post, later tonight or tomorrow( See above and below)." - Kurt Thrust current Director of the Jodrell Plank Observatory.


Vega in Lyra - Zero and First order spectra with stars as captured.



Monday, 26 October 2026

The Seestar S30 spectrometry project.

 


"Production moves on in the JPO Clean Room under the close supervision of Jolene McSquint-Fleming our engineer. The next related activity will be the capture of data from a range of stellar spectral types. We await a clear night in Lowestoft for this work to be undertaken. Professor Chrissy H will use this data in preparation of  a dedicated processing app."- Joel Cairo CEO of the Jodrell Plank Observatory.

Asteroid Irene amongst the star clouds of Sagittarius

 

Comet Irene amongst the Star clouds of Sagittarius. Credit: Original data Rob Wadd reprocessed to show nebulosity 
 by Pip Stakkert.

" Asteroid Irene and Sagittarius is below our horizon in Lowestoft at this time of year, so we were pleased to find this data available on the Internet. " ,- Kurt Thrust current Director of the Jodrell Plank Observatory.

Thursday, 22 October 2026

Auroral Glow over Norwegian Glacier

 

The Constellation Ursa Major ,the Great  Bear over the Auroral Glow and Norwegian Glacier. Image Credit: Maisy Roberts.

" Many thanks to good friend of the Jodrell Plank Observatory, Maisy Roberts, for sending us this great photo of the aurora light from North of Bergen." -Joel Cairo CEO of the Jodrell Plank Observatory.