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NASA’s Juno will come within 645 miles (1,038km) of Jupiter’s largest moon Ganymede and gather significant observations. On Monday, June 7, at 1:35pm EDT (11:05pm IST), the flyby will be the closest a spacecraft has come to the solar system’s largest natural satellite since NASA’s Galileo in May 2000. NASA said that besides the striking imagery, the spacecraft will also gather insights into Ganymede’s composition, ionosphere, magnetosphere, and ice shell. The Galileo spacecraft had passed as low as 162 miles (261 km) over the surfaces of the Galilean moons, producing detailed images.

The space agency said that Juno will start collecting data at least three hours before approaching the closest point it’s expected to get to the largest satellite in the solar system. Among instruments, NASA said that besides the Ultraviolet Spectrograph (UVS) and Jovian Infrared Auroral Mapper (JIRAM), Juno’s Microwave Radiometer’s (MWR) will look into Ganymede’s water-ice crust and collect data on its composition and temperature.

A report in NASA Jet Propulsion Laboratory (JPL) quoted Scott Bolton, Principal Investigator, Juno, as saying that the spacecraft carries a suite of sensitive instruments capable of seeing Ganymede in ways never before possible. “By flying so close, we will bring the exploration of Ganymede into the 21st century, both complementing future missions with our unique sensors and helping prepare for the next generation of missions to the Jovian system – NASA’s Europa Clipper and ESA’s (European Space Agency’s) JUpiter ICy moons Explorer (JUICE) mission,” he said.

Bolton added that Jupiter’s largest moon has some light and dark regions that indicate some areas may be pure ice, while others may contain dirty ice too. He said that the MWR instrument will give the first in-depth investigation of how the composition and structure of the ice vary with depth helping us better understand how the ice shell forms and the ongoing processes that resurface the ice over time.

The JPL report states that Ganymede is bigger than Mercury and is the only moon in the solar system with its own magnetosphere — a bubble-shaped region of charged particles surrounding the celestial body.

According to Space.com, several spacecraft, in the past, including Pioneer 10 in 1973, Pioneer 11 in 1974, Voyager 1 and Voyager 2, have flown by the Ganymede and returned striking photos during their flybys. The Galileo spacecraft passed as low as 162 miles (261km) over the surfaces of the Galilean moons and produced detailed images.

According to information on NASA’s Juno Overview page, the principal goal of Juno is to understand the origin and evolution of Jupiter.

The space agency says that under its dense cloud cover, Jupiter safeguards secrets to the fundamental processes and conditions that governed the solar system during its formation. The planet can also provide critical knowledge for understanding the planetary systems being discovered around other stars.


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MIT Just Proved Einstein Wrong in the Famous Double-Slit Quantum Experiment

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MIT Just Proved Einstein Wrong in the Famous Double-Slit Quantum Experiment

Physicists at MIT conducted a precise version of the renowned double slit quantum experiment, which challenges Einstein’s objections to quantum mechanics. With the help of ultracold atoms and single photons, they have shown the reaction of the long-standing wave-particle duality discussion without traditional spring setups. The researchers ignored the classical apparatus components and allowed nature’s inherent uncertainty to unleash Bohr’s complementarity, as both wave and particle-like behaviour cannot be observed simultaneously. The finding matches the quantum theory and disagrees with Einstein’s local realistic expectations.

MIT’s Quantum Experiment Challenges Einstein’s Classical View

As per Sci Tech Daily, Einstein argued for the deterministic reality, and claimed that the particles must be definite properties irrespective of the observation and that nothing could travel faster than light. With the Copenhagen interpretation, Bohr held the views which posit that only measurement defines the physical reality, along with complementary properties such as wave and particle behaviour, which are exclusive. The result of MIT supports this interpretation by Bohr.

With the removal of spring elements and the intrinsic quantum uncertain reliability of the ultracold atoms, MIT has sidestepped classical interference artefacts. Through this design, the experiment cleanly isolates the quantum effects and makes the result more robust and vague. Their behaviour demonstrates the dual nature when the individual photons pass through this experiment.

Bohr’s Complementarity Confirmed: Nature Obeys Quantum Rules

The findings through this experiment not only give the mechanical predictions and however, but also reinforce the significance of the theorem by Bell. Experiments done by Delft and Aspect have questioned the inequabilities under restricted conditions, strongly discrediting the hidden variable arguments of Einstein.

In a nutshell, MIT’s ultra double-slit experiment provides compelling evidence against the local realism of Einstein but in favour of the indeterminacy of quantum. Through the demonstration of the complementarity of the minimal classical interference, it is clear that the experiment underscores that nature follows the rules of quantum mechanics.

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PSR J0922+0638 Pulsar Keeps Glitching Every 550 Days, Scientists Are Intrigued

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PSR J0922+0638 Pulsar Keeps Glitching Every 550 Days, Scientists Are Intrigued

PSR J0922+0638 is one of the pulsars, which are typically ultradense remains of a massive star that exploded as a supernova. These are quite compact and lie a few miles away; however, they carry more weight than several other suns. Their density infers that the internal matter is packed tightly, and the borders diverge toward the black hole. However, the collapse of these stars is prevented due to the pressure from the quantum forces. Neutrons and protons smash together at the time of extreme densities, and then they create a single gigantic atomic nucleus. However, the core of the neutron stars is still a mystery.

Unraveling the Structure and Rotation of PSR J0922+0638

As per space report, these dense stars act as giant atomic nuclei together with the neutrons and protons pulled together under the gravity. One of the behaviours of pulsars is their rotation, which is stable. For example, PSR J0922+0638 rotates after every 0.43063, and this continues for thousands of years.

Astronomers studied the data from over 22 years to further understand the stability. The data was collected from South Africa’s MeerKAT array and China’s Nanshan Radio Telescope array. Although the changes were minuscule, even less than a billionth, the stars show an energy shift because of the intense physical forces. The scientists found a dozen glitches that we call a little change in the rate of rotation. The glitches followed a cycle in which rotation repeats after every 550 days.

Glitches, Magnetic Cycles, and the Mystery Within Pulsars

Furthermore, due to sudden glitches, a slow and cyclic speeding up and slowing down of the spin of the pulsar was seen during a 500-600-day period. This behaviour made the scientists question the glitches and the time variations of the pulsar, with the unawareness of the exact cause.

The theories put forward by the scientists comprise the magnetic cycle, which is similar to the movement of the superfluid in the star or the sun. Even after these theories, the internal mechanics of a pulsar are speculative. Further, long-term observations are important to know these secrets.

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Starlink’s Unintended Signals Threaten Astronomical Research, Study Finds

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Starlink’s Unintended Signals Threaten Astronomical Research, Study Finds

Astronomers have concerns over SpaceX’s Starlink connection, as the world is interlinked by the Starlink internet service, but there are big concerns about it. The satellite is interfering with the universe’s observation, and these fears have been confirmed by Curtin University. As per the analysis of 76 million images from the prototype station, it was found that the Starlink satellite emissions affect up to 30 percent images in some datasets. This kind of interference could change the outcome of the research that depends on that data.

Starlink’s Unintended Emissions Threaten Astronomical Research

As per NASA, it was found that from 1,806 Starlink satellites, there occurred 112,000 radio emissions. Further, it was observed that much of the interference is not deliberate. Some satellites detected emitting data in bands in which no signals are present at all. This includes 703 satellites that were identified at 150.8 MHz. This is meant to be protected for radio astronomy, as said by study lead Dylan Grigg.

Grigg observed that these unintended emissions might have come from onboard electronics. Astronomers can’t easily predict or filter these out as they are not part of the intentional signal. The International Telecommunication Union regulate the satellite emissions for protecting astronomical observations, current rules, and focuses on the intentional transmissions and does not address these unintended emissions, as said by Steven Tingay. Executive director of the Curtin Institute of Radio Astronomy.

Calls Grow for Policy Updates to Safeguard Radio Astronomy

The problem is not just the Starlink Satellite; the team found that it currently has the most expansive constellation, including around 7,000 satellites, which can be deployed during the survey. However, the satellite network can release non-deliberate transmissions too.

Tingay said that it is crucial to note that Starlink is not disturbing the current regulations, so there is nothing wrong with it. He further added that we hope this study adds support for the international efforts and updates the policies which control the impact of this technology on the radio astronomy that is currently going on.

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