First pictures from Euclid satellite reveal billions of orphan stars
nottingham.ac.uk
nottingham.ac.uk
Hope all of the engineers that struggled to get this mission spacebourne can enjoy!
But if you have seen the issues that Starliner has had recently, I would echo the statement from there, that valves are hard. Very hard. Everything to do with pressurised systems in space is hard. But the propulsion team worked it through and are now seeing the fruits of the long hours.
1. What was testing/safety/static checking culture like? I have experience within a NASA software contractor that spent a lot of time and stress on balancing classic “aerospace-y” engineering practices with the more modern ones out of SV, which are paradoxically both more and less rigorous than the old ways across different situations. In other words: in a project like this where “groundbreaking” is expected, how closely did you stick to tradition?
2. I’m dumb and just realized: did they pick Euclid because it’s in the EU??
E: 3. What’s it like to be “accomplished”? Like, more so than any random app ceo or sales consultant or whatever, you have now accomplished what would be many young people’s dream: to help build a spacecraft that’s advancing science significantly. I’m assuming all stress dissolves and any sacrifices resolve into being definitely worth it? Asking for a friend, of course.
1. The testing culture is very thorough. I was involved on the propulsion side of things, and as such the safety is taken very seriously, for the safety of the test/production engineers and of course the spacecraft. Propulsion systems are typically integrated in such a way that it is very difficult (nigh impossible at times) to separate them if an issue is found at a later stage, so the testing goes through things with a very fine comb. And even still things can go wrong and can sometimes only be found at a later stage.
From the spacecraft Assembly Integration and Test (AIT) side of things, which is where I work, things are traditional but pragmatic. If a new way can be shown to be more reliable we will adopt it. But not before it is very well understood and characterised. In space, heritage is king, the best way to know if something will work in space is to already know it works in space. So it can take a lot of evidence for a new method/system to be adopted, and when we think we are moving quickly, it probably looks like a glacial pace to others.
During the build and test, we are often so far from the end goal of a spacecraft, its not possible to see the "groundbreaking" aspect of things. Perhaps the payload designers and engineers can see this better.
2. I believe it is named after Euclid, as the father of geometry, as the mission goal was to measure the geometry of the universe. And also yes, go Europe.
3. Christ, accomplished? I love the idea of being accomplished in many ways, but its also a scary concept. Wouldn't want to be having notions of grandeur either. I am very lucky to have worked on many great projects, in many countries, and in a job that I honestly think I am good at and enjoy. But I am always surrounded by so many people who have done so much more, so it mostly feels like I am trying to catch up really.
The science missions really are special to me, I have a background in Astrophysics, and sort of fell into spacecraft engineering. So it is always a real pleasure to get to work on something I understand on a deeper level. But most of the missions I have worked on have not been so special. Most spacecraft are to make money or do something for a military. Its why I have so much time for ESA. Even with their issues (cost, time, etc.), they really feel like they do the important missions for humanity. Nasa and Jaxa too, but they mix in a higher amount of the less special stuff in my experience.
The stress and sacrifice was stressful and sacrificial(?). I wouldnt say it was worth it, or not worth it. Its an odd one. Mostly I have just tried to do cool shit as often as I can, and I have been damn lucky.
Thanks for the kind words though, and I hope I wasn't rambling too much in my response.
https://www.theguardian.com/science/article/2024/may/23/eucl....
In this case, it found dozens of rogue planets in the Orion nebula, which is only 1,500 ly away.
I am presuming there are also going to be great numbers of rogue planets in deep space, not tied to any star or galaxy. But there would be no way for Euclid to spot them at that distance. Stars were hard enough.
I presume, in due time, there will be some sort of calculable estimation or projection of orphan stars and rogue planets per cubic parsec or kilosparsec.
Can we resolve these individual orphan stars? Or just see the cumulative glow from a lot of them?
• One piece cited viewing 1.5 trillion stars in the Perseus cluster of galaxies, which is 240 million ly distance: https://www.nottingham.ac.uk/news/first-pictures-from-euclid...
• The other cited spotted stars in galaxy cluster Abell 2390, which is in the Pegasus constellation, which is 2.7 billion ly away — an order of magnitude further away: https://www.esa.int/Science_Exploration/Space_Science/Euclid...
If I am reading this correctly, it seems like Euclid was able to see the light from individual stars ripped from their galaxies in Abell 2390. Which is quite the accomplishment.
Please let me know if I am reading too much into this, or reading it incorrectly.
Further we dramatically underestimated the number of expo planets for decades. Quite reasonably we don’t put a lot of weight on stuff we can’t detect.
A brown dwarf orbiting a red dwarf would beg to differ.
https://simple.wikipedia.org/wiki/Brown_dwarf
While very young they generate heat from both deuterium fusion but that only lasts millions to tens of millions of years. Energy from radioactive decay and their slow contraction lasts for much longer.
When I think of the brown dwarf I am also reminded of the hypothesized black dwarf. This would be the stage after white dwarf. It's hypothesized because it takes longer for the white dwarf bodies to cool than exists presently in the history of the universe. It's only a handful of sentences and will largely repeat the previous paragraph but there's the wiki page for black dwarf.
https://simple.wikipedia.org/wiki/Black_dwarf
Very interesting stuff all around. Space is so fucking cool, y'all.
It might even be possible to have this combination weigh less than our sun
Specifically the Perseus cluster reported on here has a mass of around 10^15 solar masses in total. Of that ~10% is in the form of stars, 20% is intergalactic gas and the remainder is dark matter.
The report here says 1.5 trillion of these stars in this cluster which is ~10^12 solar masses (assuming average star mass is similar to the sun's.)
So the newly observed stars reported here are around 0.1% of the total cluster mass, or around 1% of the total mass of stars in the cluster. All very approximate of course.
How much worse would it be if you were an intelligent life form on a planet orbiting one of those orphans, and the nearest star was a thousand, ten thousand, even a million light years away?
Large distance and time scales are rather gloomy.
Unless of course some of them manage to find ways to preserve information and keep records over those billions of years. The lost galaxies will be known from that.
As I understand, we built much of our picture of the universe on the fact that we can do precise parallax measurements of nearby stars.
Then we used that to see how far the nearby Cepheid variable stars are, and used the patterns those exhibit to measure distant galaxies. Then at some point we could determine the distance to a certain kind of supernova, and now we have a 3D model of the whole observable universe.
But it starts with parallax measurements which are limited in range.
https://www.jpl.nasa.gov/news/cosmology-standard-candle-not-...
-- Contact (1997)
So, we are almost 100% sure that there is extraterrestrial life somewhere in the universe, but if there is no possible causal relationship between us, what's the point? It is also the same reason why "the universe" is often shorthand for "the observable universe". There is probably something beyond it, but we have no way to know what it is, so it might as well not exist.
Edit: Also, "observable universe" is a frequently misunderstood concept. Just because something is now outside the observable universe (the distance between them and us is big enough so that the rate of expansion of the universe between us and them is higher than the speed of light) doesn't mean that we aren't, today, receiving light from a long time ago when the object was closer. If you go far enough back in time you can "see" the entire universe . As time passes, more and more mass moves outside of the observable universe since the size of the sphere is constant relative to the rate of expansion.
This requires more assumptions than just infinite scale.
Also, TIL we don't know whether π is normal thus the popular claim that "every string of numbers eventually occurs in π" is not known to be true
Earth won multiple jackpot lotteries in a row, and that's only the variables we are aware of:
* Right-sized star
* Right-sized planet
* Not too far and not to close to the star
* Not too little and not too much water
* Oxygen
* Iron core (magnetic field protects from radiation)
* Right-sized moon (keeps rotation stable, tides)
* Gas giants absorbing a lot of debris coming our away
* A single-star system, with nearly circular, stable planetary orbits (very rare)* ... and so on
Yes, I know there are permutations that might also work, but in general it does not look good for spontaneous life.I like a theory that states that the Universe is just the right size where one single Earth has only a single probability to spring up randomly. The Maker covered their tracks well, if you believe in higher intelligence.
If we guess that only about a quarter of any given galaxy is potentially habitable, that leaves 25 billion possibilities per galaxy. If we go with that and a middling estimate for the number of galaxies then we have maybe (25 billion * 1 trillion) stars, which is a number so big I don't even know how to say or comprehend it.
Even if we take an extremely conservative view that each galaxy only has at most 25 stars with potentially habitable planets (cutting the 1/4 galaxy estimate down by a factor of one BILLION) then we are still left with 25 trillion possibilities, which seems like a pretty good chance to me.
- that we are first
- oxygen is needed for all life forms
- the habitable zone that is ideal for us the only one that can give birth to intelligent life
- magnetic field is needed for life to exist/radiation kills off all life
If one of those stars had a planet with something capable of "gazing up at the night sky", does that mean their sky would be empty compared to our own?
Being outside a galaxy doesn't mean that you have a black night sky, it just means that you're a little bit further away from other stars and you're moving in the interstellar medium.
I assume some of the 'stars' we can see with the naked eye are actually galaxies, but I assume that's a small percentage.
Our closest galaxy, Andromeda, appears barely as a smudge to the naked eye.
I guess my question is more about how far away from their home galaxies are these orphan stars, expressed as a percentage of a hypothetical planet's sky-cover.
eg we see the milky way as a band because we're inside the galactic plane... would these orphan planets see their home galaxy as a fainter band because they've been ejected still in the galactic plane? Would they see part of the sky covered and part of the sky blank because they're outside their home galactic plane? Are they still close enough to their home galaxy that they're still surrounded by enough stars to fill the sky, or would the star density in their skies be seasonal?
I think it would be fun to speculate on different hypothetical cultural evolutions of different kinds of night sky configurations, like "winter is when our planet's night sees our home galaxy, so winter is when the gods send their nightlumination down on us" etc.
https://scitechdaily.com/euclid-mission-uncovers-1-5-trillio...
https://thedebrief.org/euclid-first-look-stunning-new-images...
...I was under the impression that there was a faint blue glow coming from everywhere, that was hypothesized to be extra galactic stars. Has there been any follow up on that?
https://en.wikipedia.org/wiki/Intergalactic_star#Observation...
https://hitchhikers.fandom.com/wiki/Total_Perspective_Vortex
Warms my little nerd heart.
Euclid Consortium
To date 14 European countries contribute to EC activities (Austria, Belgium, Denmark, Finland, France, Germany, Italy, the Netherlands, Norway, Portugal, Romania, Spain, Switzerland and United Kingdom).
Canada and USA through NASA and few US laboratories as well as few Japanese laboratories are also contributing and members of the Euclid Consortium.
In total, more than 2600 members were or are registered in the EC (status early 2023), of which more than 1000 are researchers in astrophysics, cosmology, theoretical physics, and particle physics.
More than 200 laboratories covering all fields in astrophysics, cosmology, theoretical physics, high energy, particle physics and space science that are relevant for the Euclid missions are contributing to Euclid.
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I've never heard someone use the long scale, it is only ever mentioned as a novelty. I think the scientific community, at the very least, has standardized on the short scale.
Re SI Prefixes: you _could_ make the argument that they are essential another short scale since they are named every 3 orders of magnitude.
But! When non-native speakers read news, they are not always completely fluent in English, or even aware the short scale exists. This is true even for journalists. I've seen articles written in a serious newspapers where a journalist confused "billion" and "trillion", because they incorrectly translated English "billion" to my language "bilion". Journalists! A cross-cultural mistake not unlike foots vs meters.
So that's one thing to consider if one wants to avoid miscommunication at all cost. I'm not sure if it is important enough to take into account - after all people should know better.
it’s all over papers and nobody is ever using the long scale that i’ve seen
https://en.wikipedia.org/wiki/Long_and_short_scales#/media/F...
Besides short scale and long scale, there is a sizable "short scale with milliard instead of billion" fraction, and of course some countries (China, India, Japan, Greece) have completely different systems. Most interesting is that Portugal uses the long scale, while Brazil uses the short scale. That must be confusing...
I am able to easily find plenty of Slovenian academics using short scale in their scientific writing. Remember, English is standard for scientific writing and publishing in international journals. I have yet to find a single one using the long-scale, actually.
https://link.aps.org/accepted/10.1103/PhysRevD.97.123540 https://iopscience.iop.org/article/10.3847/1538-3881/abe6a7/... https://link.springer.com/content/pdf/10.1186/s40294-016-001...
> observations by cataloging positions and redshifts of billions of galaxies in the next decade > and the configuration is stable over billions of years. > (networks having up to a billion of vertices; there is no limit—except the memory size—on the number of lines
So that's how the US government will make the mult-trillion dollar debt go away. They'll just call it Billions.
think it is more than permissible to use what is scientifically standard (trillion = 10^12)
And tell them it's only 1/35 of the US national debt, which is roughly $350,000 per US taxpayer.
[1] Defined as the distance at which 1AU subtends an angle of one arc second or 648000/pi AU https://en.wikipedia.org/wiki/Parsec