Skip to main content

Parker Solar Probe headed toward the Sun, performing a Venus flyby.

 



NASA’s Parker Solar Probe zoomed past Venus on Aug. 21, using the planet’s gravity to aim toward a record-setting series of flights around the Sun that start next month. The spacecraft was moving at a speed of 15 miles per second, and passed 2,487 miles above the Venusian surface as it curved around the planet. The mission operations team at the Johns Hopkins Applied Physics Laboratory in Maryland kept in contact with the spacecraft during the flyby through NASA’s Deep Space Network and determined that it was on course and functioning properly.


 Except for an 8 minute period when Venus blocked communication between the spacecraft and Earth, the mission operations team were able to successfully monitor and track the probe’s progress. The flyby marks a significant step towards Parker Solar Probe's goal of exploring the Sun's atmosphere, and hopefully uncovering answers to some of its biggest mysteries.


Nick Pinkine, Parker Solar Probe mission operations manager from APL, recently announced that Parker Solar Probe remains on track to make its closest flybys yet of the Sun. He expressed his pride in the mission team, especially the mission operators who have worked hard over the past five years to ensure smooth operations of this incredible spacecraft with a history-making mission. Venus gravity assists are a crucial part of Parker Solar Probe's journey, as the planet reduces its orbital energy to allow it to travel closer to the Sun. Since 2018, it has been exploring the origins and unlocking the secrets of the solar wind and other properties of the near-Sun environment at their source.


The Parker mission’s sixth of seven planned Venus gravity assists served as an orbit maneuver to reduce the spacecraft’s speed by 5,932 miles per hour (9,547 kilometers per hour). This maneuver changed the spacecraft’s orbit and set Parker Solar Probe up for its next five close passes by the Sun, with the first occurring on Sept. 27. During each close approach, Parker Solar Probe will break its own records for speed and distance when it comes to within 4.5 million miles (7.3 million kilometers) from the solar surface at 394,800 miles per hour. Developed as part of NASA’s Living With a Star program, Parker Solar Probe was designed, built, and operated by the Johns Hopkins Applied Physics Laboratory for NASA’s Science Mission Directorate.

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...

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...