Plan to map the atmospheric temperature and chemical composition of Uranus and Neptune.

Uranus and Neptune have a fairly common composition, Uranus and Varuna have more ice in their atmospheres than Jupiter and Saturn, both of which contain water ice as well as ammonia and methane gases, so astronomers call these two planets. Put it in the category of "icy gas monster". A team of researchers studying Uranus and Neptune will train on the upper atmospheres of Uranus and Neptune, the mysterious ice giants of the Solar System, with the help of the James Webb telescope.

The research team plans to map the atmospheric temperature and chemical composition of Uranus and Neptune to study their circulation patterns, chemistry and weather, as all the gases in the upper atmospheres of these two planets have unique chemical evidence, and Webb Can detect chemical in gases. Scientists believe that the weather and climate of Uranus and Neptune may be very different from those of Jupiter and Saturn, Uranus and Neptune—in the far reaches of our solar system, the farther away they are, the more mysterious they are, but Researchers hope that soon after launch in 2021, NASA's James Webb Space Telescope will uncover the secrets of the atmospheres of both planets.

The interior of Uranus and Neptune differs from that of Jupiter and Saturn, which is rich in hydrogen and helium, which is why scientists refer to Uranus and Neptune as the "gas giants". Jupiter is the largest planet in the Solar System, followed by Saturn, but being intermediate in size between the gas giants (Uranus and Neptune) and the terrestrial planets, these ice giants are much smaller than their gaseous cousins.

Uranus and Neptune represent the least explored range in the Solar System by researchers, but researchers plan to study the circulation patterns, chemistry and weather of Uranus and Neptune with the help of Webb. From this you will be able to know many secrets.

Comments

NASA/ESA Hubble Space Telescope Reveals New Details of the Orion Nebula’s Star Formation.

This NASA/ESA Hubble Space Telescope image captures the Orion Nebula (Messier 42, M42), the nearest star-forming region to Earth, located about 1,500 light-years away. A captivating new image captured by the NASA/ESA Hubble Space Telescope offers an extraordinary look into the Orion Nebula, the nearest massive star-forming region to Earth. Located just 1,500 light-years away, this nebula is visible to the naked eye below the three stars forming Orion's "belt." The region is home to hundreds of newborn stars, including two protostars featured in the image: HOPS 150 and HOPS 153. Named after the Herschel Orion Protostar Survey, conducted with ESA’s Herschel Space Observatory, the protostars HOPS 150 and HOPS 153 provide key insights into the early stages of star formation. HOPS 150, visible in the upper-right corner of the image, is a binary star system, with two young stars orbiting one another. These protostars are surrounded by small dusty disks, where material from th...

New Method Detects Small Asteroids in Main Belt, Offering Insight for Planetary Defense.

An international team of physicists, led by MIT researchers, has developed a groundbreaking method to detect small asteroids, as small as 10 meters in diameter, within the main asteroid belt. These space rocks, ranging from the size of a bus to several stadiums wide, were previously undetectable using traditional methods. The team's discovery, detailed in a paper published in Nature, could significantly improve tracking of potential asteroid impactors, aiding planetary defense efforts. The main asteroid belt, located between Mars and Jupiter, is home to millions of asteroids, but until now, scientists could only detect objects roughly a kilometer in diameter. The new detection technique, which utilizes the "shift and stack" method, is able to identify much smaller asteroids, even those far from Earth, enabling more precise orbital tracking. This breakthrough is crucial for planetary defense, allowing scientists to spot near-Earth objects that may pose a threat in the fu...

XSPECT Payload Successfully Validates Performance through Cas A Observation.

The XSPECT instrument captures a detailed spectrum of the supernova remnant Cassiopeia A (Cas A), encompassing both the Galactic Cosmic Ray (GCR) background and the Cosmic X-ray Background (CXB). The flux observed above 8 keV predominantly results from the combined contributions of CXB and GCR. The presented spectrum, depicted in the figure, is derived from a cumulative integration time of 20 ksec, collected across multiple orbits, providing valuable insights into the X-ray emissions associated with Cas A. XPoSat, India's inaugural X-ray polarimetric mission, has achieved a significant as the XSPECT instrument captures its initial observations from the Cassiopeia A (Cas A) supernova remnant. Launched on January 1, 2024, XPoSat is equipped with two co-aligned instruments, namely the POLarimeter Instrument in X-rays (POLIX) and X-ray SPECtroscopy and Timing (XSPECT). This mission is designed to unravel the mysteries of cosmic X-ray sources. While POLIX focuses on examining X-ray po...

Infinity Cosmos

Search This Blog