I'm reading some comments saying that, as Starlink satellites are getting fainter to the naked eye, astronomers should stop complaining. Apart from the fact that they still flare, here's a short thread explaining why even faint satellites are an issue for us.
1/ Under dark conditions your pupil is, at most, 8 mm wide. Telescopes like VLT, Keck, Subaru, GTC or LSST are 8-10 m wide. The light collecting area goes as the diameter squared, so these telescopes collect 1 million times more light than your pupil in the same amount of time.
2/ Not every photon that hits a detector triggers a signal. Your eye registers only ~10% or less of the photons it receives. The efficiency of professional astronomical detectors can reach ~80%-90%.
3/ Your eye collects light for only 0.1-0.2 secs before sending it to your brain. Astronomical exposures are several seconds, minutes or even hours long. Satellites move fast, so they don't stay on the same pixel, but this is still a concern as you can have many long streaks.
4/ Satellites look faint if you're not in a truly dark spot. Even low light pollution will wipe out 1000s of faint stars, so satellites will look faint compared to the bright stars that are left. But they'll still be much brighter than most stars we see from astronomical sites.
5.a/ Then there's the issue of Radio Frequency Interference, which affects radiotelescopes regardless of whether the satellites are illuminated or not. Check this link for more info on RFI: public.nrao.edu/telescopes/rad…
5.b/ Image from the previous link (G.B. Taylor, NRAO/AUI/NSF). Left: image of a star taken with the Very Large Array. Right: same star, when a satellite was passing 25 degrees away on the sky (that's 50 full moons!). Note the dramatic increase in the background level and noise.
6/ So don't underestimate the impact of satellites on astronomical observations. We use really, really large "eyes" to observe the sky, and some of those "eyes" see radiation that our normal eyes don't. What's faint to you is ridiculously bright to us!
7/ Finally, don't buy arguments along the lines of "some more satellites in the sky are an acceptable price in exchange for <whatever>". Similar arguments have led us to more plastic in the oceans and more CO2 in the atmosphere.
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I couldn't help it and had a go at that awesome MeerKAT image of the Milky Way centre recently released by @SKA_Africa Rather than just plotting the intensity, I've used a colour palette to map the spectral index. 🌈
For those who wanted a high-resolution version and/or a colourbar mapping the spectral index, I've uploaded it to Flickr:
Just click on the download button to the lower right and pick whatever resolution you prefer, up to 7.5k by 4.7k pixels.
A note about the colourbar: don't go around with the eyedropper tool of your image viewer program of choice to get spectral indices directly from this colour composite! While this bar traces the colour map in a consistent way, you can't just use it like that.
1/ Today’s APOD is this beautiful shot by Gerardo Ferrarino (g.ferra on Instagram), featuring the Andromeda galaxy, the closest spiral galaxy. You may have read tweets saying this is how Andromeda would look like if it was brighter, but that’s not quite true. Thread!
2/ Andromeda spans 3 degrees on the sky. How much is that? Well, one finger at arm’s length is about 1 degree wide. So if you extend your arm you would be able to cover the entire galaxy with 3 fingers. That’s big, but not *that* big!
3/ “But wait, I’ve seen this image showing that Andromeda is about 6 times larger on the sky than the Moon. Is it wrong then?” Nope, that comparison is correct. It’s just that the Moon is much smaller on the sky than you think!
1/ I took this picture of @ESO’s UT4 telescope back in January. You may have read that we use lasers to correct atmospheric turbulence, but how does this work exactly? And why do we need several lasers rather than just one? Thread!
2/ Ground-based observations are affected by atmospheric turbulence, which blurs the images of astronomical sources. But we can use high speed deformable mirrors to counteract this turbulence and get very sharp images, as I explained here:
3/ This technique requires taking 1000s of images per second, so your target can’t be too faint. If it is, then you need to have a bright star next to it to do the correction. But bright stars are rare, so with this technique you can only cover about 10% of the sky.
1/ I have the feeling that all those Musk followers who want to move to Mars have extremely romanticised and unrealistic expectations of what it's like to live in another planet. Since I (kind of) live of Mars, let me tell you my own experience...
2/ The Atacama desert looks a lot like Mars, to the point that our colleagues from the European Space Agency often come here to test Mars rovers: eso.org/public/announc…
3/ Atacama looks like Mars, but unlike Mars, it's not actively trying to kill you. Yes, humidity is extremely low, UV radiation is high, the air is thin... But it's perfectly bearable if you exercise some reasonable precautions.
1/ Every once in a while clouds pay us an unwelcome visit at Paranal. This can ruin our observations, but on the other hand we can enjoy amazing Moon halos like this one I saw in November. Do you want to learn how these haloes form? Thread!
2/ These haloes are created by hexagonal ice crystals in the atmosphere. Incident light rays are refracted twice as they go through two faces of the crystals at 60º with each other. The beam then emerges at a certain deviation angle relative to the incident beam.
3/ The red curve shows the deviation angle for any incident angle. There’s a minimum deviation angle at 22º: beams can’t be refracted at smaller angles. This minimum angle is also the most probable one: if you shoot beams at random angles, they’ll most likely come out at 22º.
What I love about this chart is that back in the XIX century we actually thought that there was indeed a mysterious planet inside Mercury's orbit. We even gave it a name: Vulcan.
As you know, planets follow elliptical orbits around the Sun. But Mercury's orbit is weird, as the ellipse itself rotates. This is called "precession", and other bodies do that too. Except the precession of Mercury's orbit can't be explained with Newton's laws.
In the XIX century, the French astronomer and mathematician Urbain Le Verrier proposed that this could be due to the presence of an as of then unknown planet, located inside the orbit of Mercury. This mysterious planet was named Vulcan.