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Category: space – Page 677

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Although planets, stars, and galaxies all spin along an axis of rotation, new research suggests that the universe itself might also revolve around an axis, or several, but on a cosmic scale challenging one of the fundamental assumptions of astrophysics, the cosmological principle, which holds that the same physical laws are homogeneous and uniform, isotropic, everywhere in the universe. This exotic new theory paints a picture of a spinning universe that creates structural anisotropies and asymmetries on cosmic scales of hundreds of millions of light years.

Enter one Lior Shamir, a computational astronomer at Kansas State University, who presented evidence that has yet to be peer reviewed at the recent virtual Zoom meeting of the American Astronomical Society that the early universe rotated like an enormous, complex galaxy, and continued this momentum through the galaxies we see today, hinting that the early universe had a more uniform structure that it has been steadily losing through time, resulting in an increasingly chaotic cosmos.

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This is the inaugural episode of my new podcast “Cosmic Controversy” which is available at the moment on Podbean. Many thanks to my first guest astrobiologist Lara Maldanis who talks about her and colleagues’ recent work in identifying ancient earth microfossils and how we can hope to identify microfossils on Mars.

Cosmic Controversy delves into current aerospace, astronomy, and astrobiology as well as long-standing issues in aerospace and aviation history…

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Researchers from the Moscow Institute of Physics and Technology, joined by a colleague from Argonne National Laboratory, U.S., have implemented an advanced quantum algorithm for measuring physical quantities using simple optical tools. Published in Scientific Reports, their study takes us a step closer to affordable linear optics-based sensors with high performance characteristics. Such tools are sought after in diverse research fields, from astronomy to biology.

Maximizing the sensitivity of measurement tools is crucial for any field of science and technology. Astronomers seek to detect remote cosmic phenomena, biologists need to discern exceedingly tiny organic structures, and engineers have to measure the positions and velocities of objects, to name a few examples.

Until recently, no measurement could ensure precision above the so-called shot noise limit, which has to do with the statistical features inherent in classical observations. Quantum technology has provided a way around this, boosting precision to the fundamental Heisenberg limit, stemming from the basic principles of quantum mechanics. The LIGO experiment, which detected for the first time in 2016, shows it is possible to achieve Heisenberg-limited sensitivity by combining complex optical interference schemes and quantum techniques.

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While scanning the skies, humanity has identified thousands of exoplanets orbiting distant stars. However, very few of them are at all similar to Earth. Now, the Max Planck Institute for Solar System Research in Göttingen reports a newly discovered exoplanet could be a “mirror image” of our own.

We currently lack the technology to directly image exoplanets, so we can only infer their presence via two methods. Astronomers either look for small wobbles in a star’s rotation caused by the gravity of planets or drops in brightness from our perspective on Earth, which indicates a planet has transited the star. Kepler used the latter method to identify more than 2,600 exoplanets, and that number will probably continue to rise. Teams like the one from the Max Planck Institute are still combing through the luminance data gathered by Kepler to uncover new exoplanets. That’s how they found the very Earth-like candidate exoplanet KOI-456.04.

If it exists, KOI-456.04 orbits a sun-like star called Kepler-160 about 3,000 light-years away from Earth. Previous analysis of Kepler-160 revealed two large exoplanets — these gas giants are much easier to spot in the background noise, so many of the worlds we’ve discovered are very unlike Earth. One of those planets, Kepler-160c, showed small perturbations in its orbit that could indicate another planet, so the Max Planck Institute set out to find it.

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