The ESA/JAXA BepiColombo mission is gearing up for its second close flyby of Mercury on 23 June. ESAโs spacecraft operation team is guiding BepiColombo through six gravity assists of the planet before entering orbit around it in 2025.
Like its first encounter last year, this weekโs flyby will also bring the spacecraft to within about 200 km altitude above the planetโs surface. Closest approach is anticipated at 09:44 UT (11:44 CEST).
The primary purpose of the flyby is to use the planetโs gravity to fine-tune BepiColomboโs trajectory. Having been launched into space on an Ariane 5 from Europeโs Spaceport in Kourou in October 2018, BepiColombo is making use of nine planetary flybys: one at Earth, two at Venus, and six at Mercury, together with the spacecraftโs solar electric propulsion system, to help steer into Mercury orbit against the enormous gravitational pull of our Sun.
Even though BepiColombo is in โstackedโ cruise configuration for these brief flybys, meaning many instruments cannot yet be fully operated, it can still grab an incredible taste of Mercury science to boost our understanding and knowledge of the Solar Systemโs innermost planet. A sequence of snapshots will be taken by BepiColomboโs three monitoring cameras showing the planetโs surface, while a number of the magnetic, plasma and particle monitoring instruments will sample the environment from both near and far from the planet in the hours around close approach.
โEven during fleeting flybys these science โgrabsโ are extremely valuable,โ says Johannes Benkhoff, ESAโs BepiColombo project scientist. โWe get to fly our world-class science laboratory through diverse and unexplored parts of Mercuryโs environment that we wonโt have access to once in orbit, while also getting a head start on preparations to make sure we will transition into the main science mission as quickly and smoothly as possible.โ
A unique aspect of the BepiColombo mission is its dual spacecraft nature. The ESA-led Mercury Planetary Orbiter and the JAXA-led Mercury Magnetospheric Orbiter, Mio, will be delivered into complementary orbits around the planet by a third module, ESAโs Mercury Transfer Module, in 2025. Working together, they will study all aspects of this mysterious inner planet from its core to surface processes, magnetic field and exosphere, to better understand the origin and evolution of a planet close to its parent star. Dual observations are key to understanding solar wind-driven magnetospheric processes, and BepiColombo will break new ground by providing unparalleled observations of the planetโs magnetic field and the interaction of the solar wind with the planet at two different locations at the same time.
On course for slingshot
Gravitational flybys require extremely precise deep-space navigation work, ensuring that a spacecraft passes the massive body that will alter its orbit at just the right distance, from the correct angle and with the right velocity. All of this is calculated years in advance but has to be as close to perfect as possible on the day.
Getting into orbit around Mercury is a challenging task. First BepiColombo had to shed the orbital energy it was โbornโ with as it launched from Earth, which meant it first flew in a similar orbit to our home planet โ and shrinking its orbit down to a size more similar to Mercuryโs. BepiColomboโs first flybys of Earth and Venus were thus used to โdumpโ energy and fall closer to the centre of the Solar System, while the series of Mercury flybys are being used to lose more orbital energy, but now with the purpose of being captured by the scorched planet.
For this second of six such flybys, BepiColombo needs to pass Mercury at a distance of just 200 km from its surface, with a relative speed of 7.5 km/s. In doing so, BepiColomboโs velocity in relation to the Sun will be slowed by 1.3 km/s, bringing it closer towards Mercurial orbit.
โWe have three slots available to perform correction manoeuvres from ESAโs ESOC Mission Control in Darmstadt, Germany, in order to be in precisely the right place at the right time to use Mercuryโs gravity as we need it,โ explains Elsa Montagnon, Mission Manager for BepiColombo.
โThe first such slot was used to tune the desired flyby altitude of 200 km over the planet’s surface, ensuring the spacecraft would not be on a collision course with Mercury. Thanks to the meticulous work of our Flight Dynamics colleagues, this first trajectory correction executed very accurately such that further slots were not needed.โ
Selfie-cam is go
During the flybys it is not possible to take high-resolution imagery with the main science camera because it is shielded by the transfer module while the spacecraft is in cruise configuration. However, BepiColomboโs three monitoring cameras (MCAMs) will be taking photos.
Because BepiColomboโs closest approach will be on the planetโs nightside, the first images in which Mercury will be illuminated are expected to be at around five minutes after close approach, at a distance of about 800 km.
The cameras provide black-and-white snapshots in 1024 x 1024 pixel resolution, and are positioned on the Mercury Transfer Module such that they also capture the spacecraftโs solar arrays and antennas. As the spacecraft changes its orientation during the flyby, Mercury will be seen passing behind the spacecraft structural elements.
The first images will be downlinked within a couple of hours after closest approach; the first is expected to be available for public release during the afternoon of 23 June. Subsequent images will be downlinked throughout the remainder of the day and a second image release, comprising multiple new images, is expected by Friday morning. All images are scheduled to be released to the public in the Planetary Science Archive on Monday 27 June.
For the closest images it should be possible to identify large impact craters and other prominent geological features linked to tectonic and volcanic activity such as scarps, wrinkle ridges and lava plains on the planetโs surface. Mercuryโs heavily cratered surface records a 4.6 billion year history of asteroid and comet bombardment, which together with unique tectonic and volcanic curiosities will help scientists unlock the secrets of the planetโs place in Solar System evolution.
Follow the flyby
Follow @Esaoperations and @bepicolombo together with @ESA_Bepi, @ESA_MTM and @JAXA_MMO for updates.
