Skip to main content

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

ISRO: PSLV C- 46 launch

PSLV-C46 Mission on 22 May 2019, Satish Dhawan Space Center Indian Space Agency (ISRO) is preparing to launch Pslv c-46 very soon.ISRO will launch RISAT-2B using PSLV-C46.ISRO is ready to launch RISAT-2B from Satish Dhawan Space Center, Sriharikota on 21 May, 2019 at 5:27 am on ISRO PSLV-C46.                                                                                            
.                                                                                                      PSLV-C46 which is the 48th mission of PSLV, Satish Dhawan Space Center (SDSC) will launch the SHAR, Sriharikota's First Launch Pad (FLP), RISAT-2B, a Radar Imaging Earth Observation Satellite.  Subject to weather conditions, the launch on May 22, 2019 has been temporarily fixed at 0527 hrs IST.The SDSC SHAR, the 36th Launch Vehicle Mission from Sriharikota and the 36th launch from the First Launch Pad. RISAT-2B will be placed in a range of 555 km at a 37-degree inclination. ISRO has made provision to make public to view the launch from the viewer gallery, recently opened in the Shreeharikota stock of Satish Dhawan Space Center.

Comments

Popular posts from this blog

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...

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...

The a barred spiral galaxy NGC 1559 has been observed by the Webb telescope.

  This image features the barred spiral galaxy galaxy NGC 1559 as seen by the NASA/ESA/CSA James Webb Space Telescope. Captured by the NASA/ESA/CSA James Webb Space Telescope, this image showcases the barred spiral galaxy NGC 1559. Situated approximately 35 million light-years away in the seldom-explored southern constellation Reticulum (The Reticule), the galaxy exhibits a visible central region and distinctive, loosely-wound spiral arms. Utilizing two of Webb's instruments, the Mid-InfraRed Instrument (MIRI) captures the glow of interstellar dust grains, outlining the interstellar medium crucial for future star formation. Simultaneously, the Near-InfraRed Camera (NIRCam) reveals starlight, including that from young stars concealed behind extensive dust, and captures emissions from ionized nebulae surrounding these youthful celestial bodies. The PHANGS team collected the data featured in this image as part of an extensive observing program, where the James Webb Space Telescope (We...