An instrument on NASA’s Parker Solar Probe was powered off by the spacecraft autonomy system on Feb. 12. It happened during the application of an approved flight software patch to the Energetic Particle Instrument (EPI-Hi). The instrument team determined the instrument was power cycled prematurely before the patch was completely loaded.
The instrument will remain off for several weeks as the geometry between the spacecraft, Sun, and Earth currently prevents a good uplink. The EPI-Hi is expected to return to normal operations after this blackout period, before the spacecraft begins its 15th close encounter with the Sun on March 12.
The overall spacecraft remains healthy and is functioning as expected and the operation of other Parker instruments has not been impacted.
On Dec. 6, NASA’s Parker Solar Probe began the 14th of 24 planned close approaches to the Sun, eventually coming within 5.3 million miles of the solar surface.
The closest approach – called perihelion – occurred on Dec. 11 at 8:16 a.m. EST, during which the spacecraft traveled at 364,639 miles per hour – fast enough to fly from New York to Tokyo in just over a minute. This is just under Parker’s record speed of 364,660 mph, set on Nov. 21, 2021.
During the spacecraft’s previous close encounter with the Sun on Sept. 5, it flew through one of the most powerful coronal mass ejections in recorded history. As the Sun’s activity continues to increase on its approach toward solar maximum – the period of greatest activity during the Sun’s 11-year cycle – scientists expect Parker to fly through and observe more exciting phenomena from its unprecedented vantage point.
“It’s a very exciting time to have a spacecraft flying so close to the Sun and observing its activity,” said Nour Raouafi, Parker Solar Probe project scientist at Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland. “The first part of the mission was during the solar cycle minimum, when we learned so much about the relatively quiet conditions in the solar atmosphere. Now Parker Solar Probe embarks on a renewed journey where the Sun is more active. Every close encounter opens up new opportunities to understand better how the Sun works and how it affects us here on Earth and beyond.”
During the encounter, which ends Dec. 16, the European Space Agency’s Solar Orbiter, NASA’s Solar Terrestrial Relations Observatory-A (STEREO-A), and radar telescopes on Earth will view the Sun from the same angle as Parker at the beginning of the encounter. They will slowly progress to an approximately 90-degree angle from Parker on the inbound side of the encounter. ESA’s BepiColombo mission will start out viewing the Sun from the same angle as Parker and progress to observing the Sun from an approximately 90-degree angle from Parker on the outbound side of the encounter. This orientation could provide an opportunity to observe a solar event from all sides.
The spacecraft entered the encounter in good health, with all systems operating normally. Parker Solar Probe is scheduled to check back in with mission operators at Johns Hopkins APL – where it was also designed and built – on Dec. 17.
Parker Solar Probe was developed as part of NASA’s Living With a Star program to explore aspects of the Sun-Earth system that directly affect life and society. The Living With a Star program is managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate in Washington. APL designed, built, manages, and operates the spacecraft.
By Ashley Hume Johns Hopkins Applied Physics Laboratory
“The Sun has changed completely since we launched Parker Solar Probe during solar minimum when it was very quiet,” said Nour Raouafi, Parker Solar Probe project scientist at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland. “When the Sun changes, it also changes the environment around it. The activity at this time is way higher than we expected.”
Raouafi expects the high level of solar activity to continue as Parker approaches this perihelion, just 5.3 million miles from the Sun. The spacecraft has yet to fly through a solar event like a solar flare or a coronal mass ejection (CME) during one of its close encounters, but that may change this coming month. The resulting data would be groundbreaking.
“Nobody has ever flown through a solar event so close to the Sun before,” Raouafi said. “The data would be totally new, and we would definitely learn a lot from it.”
Though the spacecraft has not flown through a solar event, Parker’s Wide-field Imager for Solar Probe (WISPR) instrument has imaged a small number of CMEs from a distance, including five during the spacecraft’s 10th encounter with the Sun in November 2021. These observations have already led to unexpected discoveries about the structure of CMEs.
All of Parker’s observations aid in the effort to understand the physics of the Sun, helping better predict space weather, which can affect electric grids, communications and navigation systems, astronauts and satellites in space, and more.
Although the Sun is much more active than during previous close encounters, Parker’s mission operators are not concerned about adverse effects to the spacecraft.
“Parker Solar Probe is built to withstand whatever the Sun can throw at it,” said Doug Rodgers, APL’s science operations center coordinator for the mission. “Every orbit is different, but the mission is a well-oiled machine at this point.”
While they will have very little contact with the spacecraft during its 10-day encounter, they have conducted routine operations to prepare, including readying the instruments, freeing up onboard memory space for new observations, and testing and pre-loading commands to operate the spacecraft while it’s out of contact. They have also coordinated observation times with Solar Orbiter, an ESA (European Space Agency)/NASA mission that will view the Sun from the same angle as Parker, but 58.5 million miles farther from the Sun’s surface.
Parker’s observations do not always overlap with those of other observatories, such as Solar Orbiter or Solar Terrestrial Relations Observatory-A (STEREO-A), another NASA solar probe. But when they do, it offers significant advantages.
“By combining the data from multiple space missions and even ground observatories, we can understand the bigger picture,” Raouafi said. “In this case, with both Parker and Solar Orbiter observing the Sun from different distances, we will be able to study the evolution of the solar wind, gathering data as it passes one spacecraft and then the other.”
This is not the first time Parker and Solar Orbiter have been in alignment for one of Parker’s perihelions. Scientists have used data from previous alignments of the two spacecraft to produce multiple peer-reviewed papers on solar phenomena observed by both missions.
While this perihelion promises to be exciting due to high solar activity, Raouafi is already looking ahead to future close encounters.
“While the Sun was quiet, we did three years of great science,” he said. “But our view of the solar wind and the corona will be totally different now, and we’re very curious to see what we’ll learn next.”
Parker Solar Probe is part of NASA’s Living with a Star program to explore aspects of the Sun-Earth system that directly affect life and society. The Living with a Star program is managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate in Washington. Johns Hopkins APL designed, built, and operates the spacecraft.
By Ashley Hume
Johns Hopkins University Applied Physics Lab
NASA’s Parker Solar Probe is speeding in toward the Sun after a swing past Venus on Oct. 16, successfully using the planet’s gravity to shape its path for its next closest approach to our star.
At just after 5:30 a.m. EDT, moving about 15 miles (24 kilometers) per second, the spacecraft swooped 2,370 miles (3,814 kilometers) above Venus’ surface. Such gravity assists are essential to the mission to bring Parker Solar Probe progressively closer to the Sun; the spacecraft counts on the planet to reduce its orbital energy, which in turn allows it to travel closer to the Sun and measure the properties of the solar wind near its source.
This was the fifth of seven planned Venus gravity assists. The flyby reduced Parker Solar Probe’s orbital speed by about 6,040 miles per hour (9,720 kilometers per hour), and set it up for its 10th close pass (or perihelion) by the Sun, on Nov. 21.
Parker Solar Probe will break its own distance and speed records on that closest approach, when it comes approximately 5.3 million miles (8.5 million kilometers) from the Sun’s surface — some 1.2 million miles (1.9 million kilometers) closer than the previous perihelion on Aug. 13 – while reaching 101 miles (163 kilometers) per second, or 364,621 miles per hour. Assisted by two more Venus flybys, in August 2023 and November 2024, Parker Solar Probe will eventually come within 4 million miles (6.2 million kilometers) of the solar surface in December 2024.
Parker Solar Probe, which was designed and built at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, is healthy and its systems are operating normally after the Oct. 16 Venus flyby. The flyby operation was monitored by the spacecraft and mission operations teams at APL, through NASA’s Deep Space Network.
By Mike Buckley Johns Hopkins University Applied Physics Lab