Category Archives: Optical

Image

The Lagoon Nebula from Sydney

Updated version of my test image of the Lagoon Nebula (M8) with the first light of the ZWO ASI1600MM Pro camera and broad-band filters.

This image combines:

  • 39 x 120s H-alpha (Baader 3.5nm ultra-narrow filter), in red. Darks and flats included.
  • 40 x 15s OPTOLONG L-Pro filter, in green. No flat or darks.
  • 28 x 300s [O III] 3 nm ultra-narrow Antlia filter, in green. Includes darks and flat (this image is the new addition).
  • 56 x 6s ZWO B filter, in blue, no flat or dark.

H-alpha data taken on 21st Aug 2020, L-Pro and B data taken on 23rd Aug 2020, from my backyard at home, 15 km North from Sydney’s city center.

Telescope: Skywatcher Black Diamond 80, f=600mm (f/7.5)

Equipment: I used the ZWO ASIAir to control the camera, the mount (Skywatcher AZ-EQ6) and the guiding system (ASI120MM + Orion 50mm finderscope). ZWO filter drawer for changing filter.

The [O III] data taken on 18 August 2021, including the Orion 0.75x focal reducer and the ZWO 7×2″ filter wheel.

Processing: Data processed with Siril software. FITS converted on TIFF using NASA’s Fits Liberator considering a logarithmic function. Color / saturation / levels / contrast / smart sharpen with Photoshop.

Full resolution image in my Flickr.

Credit: Ángel R. López-Sánchez (AAO-MQ).

Carina Nebula in natural colours

Image of the Carina Nebula using broad-band filters B (blue), G (green) and R (red), trying to achieve natural colours (i.e. the colours we would see with our eyes).

For avoiding saturating the brightest part of the nebula, only 10s exposures were taken, with a small “manual” (*) dithering pattern. 42 single frames were combined in each filter (7 minutes per filter).

The data were taken at around 3am, Saturday 13 March 2021, from Siding Spring Observatory (near Coonabarabran, NSW, Australia).

I used a ZWO ASI1600MM-Pro with the ZWO 2″ BGR filters, my new 7×2″ ZWO filter wheel, a Skywatcher Black Diamond 80mm with an Orion x0.8 focal reducer (effective focal length 480 mm, f/6). I used the ZWO ASIAir to control the camera, filter wheel, the mount (Skywatcher AZ-EQ6) and the guiding system (ASI120MM + Orion 50mm finderscope *).

The data have been processed with SIRIL, and then Photoshop for getting the colours. Darks were used but not flats were taken.

Credit: Ángel R. López-Sánchez (AAO-MQ).

Full resolution available in My Flickr.

(*) Well, actually I didn’t use guiding: the ZWO ASIAir didn’t want to talk to the mount, and I had to reset the mount a couple of times because, after doing the 3-stars alignment, the solution was completely wrong, once it pointed me to the ground to go to Canopus! After 3 hours fighting, very tired and cold, I decided to do something quick at least for saving the night. This was it. I had to do the dithering manually moving slightly the telescope with the keypad every 3-4 exposures. Dithering is VERY important for removing extra noise / artefacts of the camera.

PS: The astrometry of the image can be found in this link. Well, actually I uploaded the previous version I quickly created, that had too much magenta. But I wanted to check a curious object in the image, V* FU Car, a carbon star with magnitudes V = 11.2 and G= 12.4 en G, meaning V-G = -1.2 mag!

Image

Helix Nebula in H-alpha from Sydney

Deep H-alpha image of the Helix Nebula obtained from my backyard, 15 km from Sydney’s city centre.

This image combines the best 40 frames of the 82 frames I got the nights of 24-30 August, 7, 12 and 15 September 2020 using the ZWO ASI1600MM Pro and the H-alpha Baader 3.5nm ultra-narrow filter.

All frames had an exposition time of 900s (15 minutes), hence this image combines a total of 10 hours of telescope time!

Telescope: Skywatcher Black Diamond 80, f=600mm (f/7.5)

Equipment: I used the ZWO ASIAir to control the camera, the mount (Skywatcher AZ-EQ6) and the guiding system (ASI120MM + Orion 50mm finderscope). The H-alpha filter was in the ZWO filter drawer.

Processing: Data processed with Siril software. FITS converted on TIFF using NASA’s Fits Liberator considering a logarithmic function. Color / saturation / levels / contrast / smart sharpen with Photoshop.

I hope to get soon some data in broad-band filters to get the colours!

Full resolution image in my Flickr.

Credit: Ángel R. López-Sánchez (AAO-MQ).

Image

M42 from Sydney

Image of M 42 (The Orion Nebula) from my backyard, 15 km North from Sydney’s city center, on 10th Mar 2020.

Equipment: Skywatcher Black Diamond 80 (F=600mm, f/7.5), Skywatcher AZ-EQ6 (mount), ZWO ASI178MC (main camera), ZWO ASI120MM + Orion 50mm guidescope (guiding), 2″ UHD Optolong filter, and ASIair controlling everythin (using my son’s iPad).

This image combines 60 x 20s light frames, and 21 x 20s dark frames. Aligned and stacked with SiriL, stretching, colour contrast, saturation, levels, and luminosity with Photoshop.

Full resolution image in my Flickr.

Credit: Ángel R. López-Sánchez (AAO-MQ).

The Betelgeuse hype

Although we are “enjoying” the Christmas break, today I’ve been contacted (thanks to Rami Mandow @CosmicRami) by Kelsie Iorio, an ABC News Digital journalist who was preparing an article about the situation of the red supergiant Betelgeuse.

The article published in ABC News, entitled “Is Betelgeuse, the red giant star in the constellation Orion, going to explode?“, can be found in this link. It includes comments from Rami Mandow, Associate Professor Michael Brown from Monash University’s School of Physics and Astronomy and myself, with some other tweets from several astrophysicists who are talking about the “mysterious dimming of Betelgeuse“.

The red supergiant star Betelgeuse in Orion was the very first star after the Sun we got a direct image of its surface. That is because it is a huge star: if it were where the Sun is its outer layers will reach the orbit of Jupiter! This image was taken with the Hubble Space Telescope in 1995. More info in the APOD (Astronomy Picture of the Day) on April 19th, 1998. Credit: A. Dupree (CfA), R. Gilliland (STScI), FOC, HST, NASA.

But I want to share with you my full interview here, and keep it for my records, so here it goes.

The Betelgeuse hype

Interviewer: Kelsie Iorio  (ABC News Digital )

Interviewee: Ángel R. López-Sánchez (AAO-MQ)

Q: For those who don’t know, what is Betelgeuse and what is it doing at the moment that’s out of the ordinary?

Betelgeuse is a bright star in the famous constellation of Orion the Hunter. It is a red supergiant star, meaning that it is star that is much more massive than our Sun (10 – 15 times) and that is already in the latest stages of its live. The star will eventually explode as a (type II) supernova. We astrophysicists know this will happen “soon”, but “soon” in Astronomy means 100 thousands years or perhaps even more.

During the last month observers worldwide have measured a dimming in the brightness of Betelgeuse.

This is actually completely ordinary, as it is well known and documented that Betelgeuse is a variable star (that means that it’s periodically changing its brightness).

Social media has again played a role here with the “hype” of the brightness of Betelgeuse: it is a normal situation that is happening at the moment and we can explain the dimming of Betelgeuse in many ways (a small shrinking of its huge size, solar spots, magnetic activity, a combination of factors) without the need of thinking that is going to explode now.

But people have been talking about that and many of them would love to see Betelgeuse explode! (I do not).

 

Q: Why is the astronomy world so excited about what’s happening?

If Betelgeuse really explodes as a supernova this would be a great opportunity for use to study how massive stars explode and get a better understanding of stellar evolution and stellar interiors. It will create a point-like object as bright as the Moon that would be visible even during the day, that will be fading during months till disappear.

However I must insist: the dimming of the brightness is the typical behaviour of the star. It is periodically changing its brightness and it has had this “low” brightness in the past. Even Aboriginal Australian knew this star changed brightness!

 

Q: Can we see Betelgeuse from Australia? For people who haven’t seen it or don’t know how to look for it, what does it look like from earth?

Of course! This is a star located very close to the celestial equator, meaning it can be seen essentially from everywhere (just not from the very same South Pole and around). Right now it is clearly visible to the North-East at the beginning of the night. The constellation of Orion is one of the most famous constellations of the sky and can be very easily recognised even by non-experts. Just use a stellar map (there are plenty free in internet, I recommend http://skymaps.com, and also plenty of apps) and you’ll see it. Despite it has noticeable dimmed in the last month, Betelgeuse still is one of the brightests stars in the night sky.

As any other star Betelgeuse is just a point of light, even when using a powerful telescope: stars are very, very, very far away from us to see them like a little disk. Betelgeuse is at a distance of around 700 light years.

 

Q: What do you think will happen to Betelgeuse next? Is it likely to explode?

No, it is very unlikely we see it exploding. The latest astrophysical research conducted about Betelgeuse clearly shows that it should still have a life of around 100 thousand years. Again, that is almost NOTHING in the cosmic scale, but a lot for us.

As it has done plenty of times in the past, Betelgeuse will eventually gain brightness again and all will be back to usual, continuing being sometimes a bit brighter sometimes a bit dimmer during the rest of all our own lifetimes.

 

Q: Is what’s happening with Betelgeuse a rare event?

No, it is not a rare event.

There are PLENTY of variable stars in the sky. A nice example is the star Mira in the constellation of Cetus (the Whale). This star sometimes can be easily seen with the naked eye and sometimes it is imposible to see, needing binoculars or telescopes to detect it. And it is not going to explode as supernova!

 

Q: Do you believe it’s important for the wider public to have a basic knowledge of astronomy and understand what’s happening in situations like this? Why?

I think it is important because everyone loves Astronomy but nowadays it is very easy to be confused because of the mixed bag of content found in social media and the internet.

I could tell the story about why supermoon are NOT a thing, but that is for another time (or read it here: https://angelrls.wordpress.com/2016/11/11/supermoons/)

 

Article in ABC News: “Is Betelgeuse, the red giant star in the constellation Orion, going to explode?“, Kelsie Iorio, 28th December 2020.