Chandrayaan-2 successfully transferred first grade.

Chandrayaan-2 has successfully completed its orbital elevation in the orbit of Earth, i.e. the orbital elevation was successfully completed on Wednesday. Chandrayaan-2 was successfully launched from Satish Dhawan Space Center, Sriharikota. Rocket GSLV Mark, called 'Bahubali' after 16 minutes of launch ... The M1 had established the orbital earth in orbit.

ISRO said that two days after the yon was installed in the Earth's 170x45,475-km elliptical orbit, it would be the first 'orbital' through the 'On Board' propulsion system during 27-second 'firing' period at 2 pm 52 minutes Uplift campaign 'was executed And the new class of Chandrayaan 2 will now be 230 x 45163 kilometers.

ISRO said that the second 'orbital elevation' campaign will be carried out at around one o'clock on Friday night. After traveling around 3.84 lakh km in Chandrayaan-2, there is hope of reaching the moon on September 7.

To carry Chandrayaan 2 closer to the moon, many series of 'orbital elevation' campaigns will be carried out in the next weeks and on September 7, a 'soft landing' of the rover will be made in the South Pole region of the Moon, where no country has so far been reached.

ISRO said that the elevation campaign phases related to the Earth's orbit will be executed from Wednesday and it will conclude on August 14, 2019 with the launch of the vehicle on the launch path towards the Moon. After this Chandrayaan-2 will move forward to the moon.

Orbiter of Chandrayaan-2 will rotate in the orbit of the moon, while 'Vikram' will make 'soft landing' on the surface of the moon.After this, the Rover 'Pragyan' will come out of the lander and start his own superficial investigation.

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