Astronomy
SKA Organization and CERN Formalize Agreement to Advance Extreme Scale Computing
The SKA Organization and CERN signed an agreement formally signaling their continued collaboration in the development of extreme scale (exascale) computing. If you are interested in exascale computing, practical applications for data management, scientific investigation, space exploration, and the origins of the universe, then this news should make your inner geek weep with joy.
CERN (Conseil Européen pour la Recherche Nucléaire)
The majority of you should have familiarity with CERN. It is the research organization operating the largest particle physics lab in the world. Most of the current experiments involve the Large Hadron collider (LHC) particle accelerator. Experiments using the LHC are responsible for proving the existence of the sub-atomic particle the Higgs boson. As a result of this proof of existence, we have proof for the existence of the Higgs field. Most physicists see this proof as the key for moving beyond the Standard Model of particle physics so that we can understand the universe in a fundamentally different way. Needless to say, CERN’s research produces massive amounts of data. Consequently, the data require enormous computing power to process and a colossal storage capacity.
The SKA Organization
However, many of you probably are not familiar with the SKA Organization (Square Kilometre Array Organization). It is an international partnership to manage the construction, maintenance, and use of the Square Kilometre Array (SKA). The SKA is still under construction, but when complete it will be the largest and most advanced radio telescope in existence. The telescope is an array composed of thousands of antennae. The deserts of South Africa and Australia are the two locations that will host the equipment. When the SKA is fully operational, it will have a total collection area of over one square kilometre.
The SKA is estimated to have a sensitivity fifty times more than any other radio instrument. The array will have the ability to survey the sky and cosmos ten thousand times faster than existing devices. As a result, the array will produce an enormous amount of data, estimated at ten times that of today’s global internet traffic. Therefore, the partnership with CERN more than makes sense.
Research Using the SKA
The central research focus is the nature of the universe. The SKA’s design allows it to detect radio signals from billions of light years away. Many of these radio signals represent the birth-sounds of the first galaxies and stars over 13 billion years old.
There is amazing potential for major research breakthroughs into dark matter, dark energy and cosmic magnetism. The project also provides the ability for more robust experimentation to test Einstein’s general theory of relativity. In addition, research will investigate the habitability of planets and include searches for extraterrestrial life.
Is That A Petabyte In Your Pocket, Or Are You Just Happy To Be Doing Scientific Research?
CERN reported that on June 29, the organization surpassed 200 petabytes (PB) of permanently stored data. Current estimates show that SKA will produce in excess of 3,000 PB per year. The first phase of the project alone will produce 300 PB per year.
This means that SKA will produce 160 terabytes of raw data per second. For perspective, this equals the data on 35,000 DVDs per second.
If you’re a bit rusty with your bits and bytes, remember that it goes byte, kilobyte, megabyte, gigabyte, terabyte, petabyte, exabyte. Each successive category is 1000 times the previous category. So, 1000 bytes equal 1 kilobyte, 1000 kilobytes equal 1 megabyte, and so on.
For perspective, the average laptop has a 500GB hard drive, the average desktop 1TB, while the average movie requires 2-5GB of space. The Playstation 4 is stock with 500GB, while the iPhone 7 has options for 32GB, 128GB, or 256GB.
As you can see, the SKA and CERN produce a tremendous amount of data at an astronomically fast rate. Such data production requires advanced computing power. This is the purpose of exascale computing.
Exascale Computing For Your Pleasure
Extreme scale computing is capable of performing a billion billion (a quintillion) calculations per second. In contrast, the current “common” fastest computers are petascale systems that perform a quadrillion calculations per second. The performance increase from petascale to exascale is incredible.
Computing performance is measured in FLOPS, floating point operations per second. An exascale system computes at the level of exaFLOPS. Returning to our earlier comparisons, your Playstation 4 is capable of 1.84 teraFLOPS and the iPhone is at 1.6 gigaFLOPs. If you want to match just one exaFLOPS, you will spend 31,688,765,000 years performing one calculation per second. Yeah, you’ll need a lot of pencils and paper.
The computing power is mind-boggling. Thus, the partnership between CERN and SKA will help continue pushing the development of computers with ridiculously fast calculation power.
SKA and CERN Partnership – A Match Made For The Heavens
Prof. Philip Diamond, the SKA Director-General, said “The signature of this collaboration agreement between two of the largest producers of science data on the planet shows that we are really entering a new era of science worldwide. Both CERN and SKA are and will be pushing the limits of what is possible technologically, and by working together and with industry, we are ensuring that we are ready to make the most of this upcoming data and computing surge.”
Prof. Eckhard Elsen, the CERN Director of Research and Computing, said “The LHC computing demands are tackled by the Worldwide LHC computing grid which employs more than half a million computing cores around the globe interconnected by a powerful network. As our demands increase with the planned intensity upgrade of the LHC we want to expand this concept by using common ideas and infrastructure, into a scientific cloud. SKA will be an ideal partner in this endeavour.”
The two statements best sum-up the collaboration. Therefore, the partnership has amazing potential to expand our knowledge of life, the universe, and, really, everything. Plus, we can hold out hope that further development of exascale computing will trickle down to us consumers and soon enough we’ll have petascale power for our entertainment purposes.
What are your thoughts on the SKA/CERN partnership and the SKA project?
Astronomy
Witness the rare celestial event of Mars and Jupiter reaching their closest proximity in the sky this week, a phenomenon that will not occur again until 2033.
Mars and Jupiter will be only 0.3 degrees apart in the sky on August 14. From our point of view, this passage is very close. If you miss it, you won’t be able to see another one until 2033.
When two objects pass each other in the sky from our point of view, this is called a conjunction. Every time two planets came together, the closer one would block out the other because they would all be moving in a perfectly flat plane. The orbits of the planets are slightly different from those of the other planets, though, so they move slightly to the north and south of each other. Every time, that gap is a different size.
When two things happen close together, the results are especially stunning. Jupiter and Saturn were close enough to each other in 2020 that they could be seen in the same field of view through a telescope. This is a treat for people who like to observe the sky.
Being 0.5 degrees wide, the full moon will fit in any view that can hold the whole moon. This pair will also look good before and after the full moon.
But even with the naked eye, a close conjunction can make the sky look even more amazing. The contrast between the red of Mars and the white of Jupiter will be especially striking. However, Mars’ brightness changes a lot. When it’s at its brightest, it’s about the same brightness as Jupiter. Right now, it’s 16 times less bright. They are so bright that, unless there are clouds, you should be able to see them from all but the dirtiest cities.
Most people in the world will miss this sight, though, because they can’t see the pair of planets in the evening from anywhere on Earth. The exact time they rise depends on where you live, but it’s usually between midnight and 3 am. To see this, you will mostly need to get up before astronomical twilight starts so that you have time to get through the thickest part of the atmosphere.
For people in Europe, Africa, west Asia, and the Americas, the closest time will be 14:53 UTC, which is during the day. The mornings before and after, though, will look almost as close.
Mars and Jupiter meet about every two and a half years, but the most recent one was almost twice as far away and could only be seen in the morning. In 2029, the gaps will be just under two degrees. The next one will be even wider, at more than a degree.
When planets are close to each other, that doesn’t always mean that their distance from each other is very small. Mars has been around the Sun for 687 days, but it is now less than 100 days past its perihelion, which means it is closer than usual. Even though Jupiter is a little closer than usual, it’s not really that close. To be as close as possible to each other, Mars has to be at its farthest point, and Jupiter has to be at its closest point. So this one is not unusual.
But if you want to see something beautiful, you will have to wait more than nine years to see it again.
Astronomy
It may not be long before we find “Earth’s Twin”
To figure out if there is life in other parts of the universe, we start with Earth, where there is life now. Finding another Earth is a good way to find aliens. We have found more than 5,000 exoplanets, but we haven’t found Earth’s twin yet. This could change soon, though. Here comes the PLATO mission from the European Space Agency (ESA).
What does PLATO stand for? It stands for PLAnetary Transits and Oscillations of stars. Its goal is very clear. It will look for nearby stars like the Sun that might have habitable worlds like Earth.
“One of the main goals is to find a way to compare Earth and the Sun.” The size of Earth is in the habitable zone of a star like the Sun. “We want to find it around a star that’s bright enough that we can really figure out how heavy it is and how big it is,” Dr. David Brown from the University of Warwick told IFLScience. “If you like, that’s our main goal.”
The telescope is not only an observatory for looking for planets, but it is also an observatory for collecting data on a huge number of stars. The mission team thinks that the fact that it can do both is a key part of why this telescope will be so important.
“You have two parts of the mission.” One is exoplanets, and the other is the stars. “From a scientific point of view, I think it’s pretty cool that these two parts are working together to make the best science we can,” Dr. Brown said.
One of the secondary goals is to make a list of all the planets that are Earth-like and all the star systems that are out there. One more goal is to find other solar systems that are like ours. Even though we don’t know for sure if our little part of the universe is truly unique, it does seem to be different from everything else.
Dr. Brown told IFLScience, “We have a bunch of other scientific goals.” “Really, how well do we know how planetary systems change and grow over time?” Planetary systems are something we’re trying to understand as a whole, not just one planet at a time.
PLATO is different in more ways than just the goals. It is not just one telescope. In fact, it’s made up of 26 different ones. Two of the cameras are fast, and the other 24 are normal cameras set up in groups of six with a small gap between them. This makes the telescope work better, has a wider field of view, and lets you quickly rule out false positives.
It can be hard to tell which of the things you find when you transit exoplanets are real and which ones are not. With the help of several telescopes, we were able to block out some of the mimics that we would have seen otherwise. “Plus, it looks pretty cool,” Dr. Brown said with excitement. “This big square with all of these telescopes pointing at you looks really cool!”
This week, Dr. Brown gave an update on PLATO at the National Astronomy Meeting at the University of Hull. The telescope is being put together and has recently passed important tests. There are no changes to the planned launch date for December 2026. An Ariane 6 rocket, the same kind that made its first launch last week, will take off from French Guiana.
Astronomy
You can watch and listen to gravitational waves coming from everywhere in the universe
Gravitational waves can be turned into sound very easily. The little chirp changes into little sounds as soon as the blocks hit each other. One of those chirps is my ringtone when my phone has sound, which doesn’t happen very often. The people at Audio Universe have now made the gravitational wave data even better.
In a 3D video, the sounds of gravitational waves hit you from the direction in the sky where it is thought they came from. The sound effects and visualization are both great. There are tiny vibrations in space-time that can hit you as you move your mouse, phone, or VR headset.
Like other sonification projects, it gives blind and visually impaired people a way to get involved in astronomy. It works well with other methods like the Tactile Universe. But that’s not the only reason why they do it.
“We want to do this for three reasons.” It helps researchers look into big, complicated datasets with lots of dimensions. It could be used to make educational materials that are immersive and interesting. Rose Shepherd from Newcastle University says, “It can also make astronomy easier for more people to understand, which is an important thing.” “Making things easier to get makes them better for everyone.”
Being able to listen to the emission lines of celestial objects is one of the most interesting things about sonification for research. As an object moves, its light spectrum peaks spread out, and sonification can make something that is barely noticeable to the eye seem very clear to the ear.
This is helpful in more than one field, though. The group has thought about how adding sound to different datasets could make them better. Warming Stripes is a cool example of this. This is a simple image that shows changes in temperature over time by using a series of stripes, from blue to red. The stripes on the right side get redder as we move from the left to the right. The left side shows decades ago. It is great to see how the climate crisis is getting worse, and now sound adds a little more to it.
“By adding sounds, it can give your data an emotional meaning.” Shepherd explained, “You can use that to show the data how you feel.” “We didn’t mean for the Warming Stripes sonification to make people feel stressed, but it was interesting to see how they reacted instead of just watching the video.”
Audio Universe is making a sonic toolkit that many people can use to make their own resources.
She gave a talk about the audio universe at the National Astronomy Meeting at the University of Hull this week.
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