Parker Solar Probe makes second close pass by Sun

An artist’s impression of the Parker Solar Probe, oriented heat-shield forward, during a close pass by the Sun. Image: NASA/Johns Hopkins APL/Steve Gribben

NASA’s Parker Solar Probe is making its second close flyby of the Sun this week on a trajectory that will carry it within about 15 million miles of the star’s visible surface on 4 April. Peak velocity at perihelion was expected to be about 343,00 kph (213,000 mph), fast enough to fly between New York and London 39 times in one hour.

During the encounter, Parker’s four sets of science instruments, operating in the shade provided by the spacecraft’s sun shield, will be recording data about the high-temperature corona. The goal of the mission is to help researchers understand what causes the temperature between the Sun’s visible surface and its outer atmosphere to jump to more than a million degrees.

The Parker Solar Probe’s position and trajectory as of 28 March, one week before the spacecraft’s second close approach to the Sun. Image: NASA/Johns Hopkins APL

Keeping its thermal protection system facing the sun, Parker will be out of contact during the encounter, beginning 30 March and ending 10 April. Recorded data will be beamed back to Earth over several weeks later this spring. A third close flyby at a similar distance is planned for 1 September followed by the second of seven Venus gravity-assist flybys on 26 December. That will put the spacecraft on course for a fourth, even closer flyby on 29 January 2020 at an even higher velocity.

While blindingly fast by human standards, even the Parker Solar Probe, moving at a constant velocity, would need more than 13,000 years to cross the gulf between the Sun and Proxima Centauri, the nearest star beyond Earth’s solar system.