This is a picture of the hydrogen and dust cloud surrounding the star Sadr (the bright white dot near the center) also known as IC 1318. The bright parts represent hydrogen clouds and the dark parts dust clouds. Those types of clouds are the birthplace of new stars. This particular photo is in black and white because it was made by using a filter that lets only the light emitted by ionised hydrogen (the H alpha spectral line) pass through it. This increases the visibility of the hydrogen clouds. Since this light is at 656 nm, it would appear bright red if coloured. Together with H beta (496 nm) also from hydrogen and O III (around 500 nm) from oxygen both cyan in color, they represent the majority of light emitted by gas clouds. So in conclusion if you were able to see this gas cloud directly it would appear a reddish-magenta color (H alpha being the dominant emission).
Since the weather has been cloudy and rainy for about a month now (not a single night where I could take decent photos), here is a photo of the sun from last summer.
Despite the sun just looking like a bright ball of light at first glance, there are actually quite a lot of things to see on it.
This photo was taken using a specific light filter that enhances the details of the sun's surface. All of those black spots are sunspots, regions of the sun that are colder due to local magnetic fields preventing some of the heat from reaching the surface. The slightly brighter regions visible on the side of the sun are solar plage, zones that are slightly hotter, also due to the local magnetic fields.
Finally, the surface of the sun in the picture looks a bit granular/wrought, that is due to solar granulation, smaller (around 1000 km in width) convection currents (basically bubble of plasma) at the surface. (The resolution isn't great so the granulation is not super clearly visible, unfortunately).
Friendly reminder that CRT TVs were basically a particule accelerator you had in your living room. They used power supple capable of delivering tens if not hundreds of thousands of volts, to accelerate the electron that were quite literally being boiled of a glowing piece of metal.
They sometime used a lead infused glass as the front plate to limite if not eliminate the small amount of X-ray they emitted towards you.
They had to be heavy because of the thickness of the glass needed to resist the distance of pressure between the atmosphere and extremely low vacuum inside the vacuum tube. It's that difference of pressure that would result in them exploding in a shower of glass shrapnell if the tube was broken.
For those not in the US wanting to search for dark skies near you, this website is quite useful.
The black areas represent the remaining natural dark skies in the United States
Picture of the helix nebula / Caldwell 63, this one was a bit of a pain to take as this nebula stays relatively close to the horizon where I live, plus, due to the position of trees and building I only get 1h per night to take photos (had to use pictures from two different nights to get to about 2h of exposure).
This object is also a planetary nebula, like M27 I previously photographed, but it appears much bigger (about 2.5 times) in parte due to it being closer to earth (about 650 light-years compared to about 1360 light-years for the dumbbell nebula/M27).
This nebula has sometimes been referred to as ''the eye of god'' I think you can guess why.
The soon to be white dwarf star at the center of the nebula is (to me at least) a bit more visible in this picture than in the one of M27.
Ok, so I was searching for information on some of the objects visible in my photo of the horse head nebula and I found these two posts (Reddit and Astrobin) by DanielZoliro that also used a SII and Ha combination but with a slightly different processing (Notably, the RGB combination being R: SII, G: 0.6xHa + 0.4xSII, B: Ha). I loved his results and I had to try it with my own data. Did turn out great, but there was a reflection of a star on the SII data and this processing amplified it (the big reddish round/donut thing on right of the full image).
(Image taken using a CarbonStar 150/600 newtonian telescope with a 0.95 coma corrector, ZWO ASI294 monochrome camera and Baader 6.5nm SHO filter. 5x120s image for each colour filter (RGB), 22x300s for the Ha filter and 32x300s for the SII filter, total imaging time 5h, stacking and processing done in PixInsight.)
As Google has worked to overtake the internet, its search algorithm has not just gotten worse. It has been designed to prioritize advertisers and popular pages often times excluding pages and content that better matches your search terms
As a writer in need of information for my stories, I find this unacceptable. As a proponent of availability of information so the populace can actually educate itself, it is unforgivable.
Below is a concise list of useful research sites compiled by Edward Clark over on Facebook. I was familiar with some, but not all of these.
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Google is so powerful that it “hides” other search systems from us. We just don’t know the existence of most of them. Meanwhile, there are still a huge number of excellent searchers in the world who specialize in books, science, other smart information. Keep a list of sites you never heard of.
www.refseek.com - Academic Resource Search. More than a billion sources: encyclopedia, monographies, magazines.
www.worldcat.org - a search for the contents of 20 thousand worldwide libraries. Find out where lies the nearest rare book you need.
https://link.springer.com - access to more than 10 million scientific documents: books, articles, research protocols.
www.bioline.org.br is a library of scientific bioscience journals published in developing countries.
http://repec.org - volunteers from 102 countries have collected almost 4 million publications on economics and related science.
www.science.gov is an American state search engine on 2200+ scientific sites. More than 200 million articles are indexed.
www.pdfdrive.com is the largest website for free download of books in PDF format. Claiming over 225 million names.
www.base-search.net is one of the most powerful researches on academic studies texts. More than 100 million scientific documents, 70% of them are free
Finale got around to processing the photos of M33 I had taken at the end of august. M33 is a spiral galaxy about half the size of our own galaxy and located about 2.7 million light years from earth. This galaxy has a rather high rate of star formation resulting in numerous ionised hydrogen regions (the red irregular blotches inside the galaxy), some of those being notable enough to have been included in the NGC catalogue or the IC catalogue.
NGC 588 NGC 604 (Example of some of the notable nebula in M33)
On of the first recorded observation of this galaxy was possibly done by Giovanni B. Hodierna before 1654, it was independently rediscovered by Charles Messier in 1764 who added it to his catalog (hence the name Messie 33).
information on the photo - total exposure time : 1h48 min using RGB and Ha filters - camera : ASI294 mm - telescope : Newtonian 150/600 with 0.95x coma corrector - photo edited with pixinsight
For those using PixInsight for treatment/edition, I recently discovered the scrips created by Seti Astro (https://www.setiastro.com/pjsr-scripts), Blemish-Blaster was quite useful to remove the halos from my Ha filter and What's In My Image helped with the identification of nebulas. If you had not heard those scrips, you should check them out.
Photo of the Pleiades (Messier 45) I took to test my new telescope. This is an open cluster of stars situated about 440 light years from earth, the brighter stars of the cluster are visible with the naked eye (around 5 to 10 stars visible depending of the light pollution, weather and eye accommodation do darkness). Unfortunately, the nebulosity, which I composed of dust clouds reflecting the light from the bright stars, is only visible in photos or with (relatively) large telescope. The cluster is about 100 million years old which is young (for an astronomical object), the more visible stars are hot blue giants, but many other, less visible, stars are present in the cluster. This cluster due to its high visibility has taken an important place in many cultures and mythologies.
(as a fun fact the name of M45 in Japanese is Subaru, and yes the car brand dose gets its name for this star cluster (which explains the logo of the brand))
I was able to see and take pictures of the comet C2023/A3 (Tsuchinshan-ATLAS) ! This comet will be visible in the night sky probably for the next week or two, it's currently visible both with a pair of binoculars and with the naked eye. Since it's visible very early after sunset, it's a bit difficult to spot for now, but in the coming days it's will gradually be visible later in the night and thus easier to observe.
This comet is one of the brightest in the last few years so it should be quite easy to observe.
I hope you all get a chance to see it, it's magnificent
Astrophotographer & chemist, mid 20'sCurrently on the roof yelling at the clouds to get out of the wayMostly astrophotos I've taken, possibly other science related stuff
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