Koronalny wyrzut masy uderza w sondę kosmiczną na orbicie słonecznej przed wspomaganym grawitacyjnie przelotem Wenus

W niedzielę 4 września we wczesnych godzinach porannych Solar Orbiter unosił się nad nim[{” attribute=””>Venus

On August 30, 2022, a large coronal mass ejection erupted from the Sun in the direction of Venus. Not long later, the powerful storm arrived at the second planet from the Sun. As the data continues to come in from Solar Orbiter, this strike reveals why ‘in situ’ monitoring of space weather and its effects on the bodies, and spacecraft, of the Solar System are so important.

Artist’s impression of Solar Orbiter making a flyby at Venus. Credit: ESA/ATG medialab

Fortunately, there was no damage or no negative effects on the spacecraft. Indeed, the ESA-NASA solar observatory is designed to withstand and in fact measure violent outbursts from our star – although Venus doesn’t always get off so lightly. Coronal mass ejections have a tendency of eroding Venus’ atmosphere, stripping off gasses as they blast by.

Fly high with Venus fly by

Currently, Solar Orbiter is a quarter of the way through its decade-long mission to observe the Sun up close and get a good look at its mysterious poles. Its orbit was chosen to be in close resonance with Venus, meaning it returns to the planet’s proximity every few orbits to use its gravity to alter or tilt its orbit.

Do tej pory orbiter słoneczny był ograniczony do tej samej płaszczyzny, co planety, ale od lutego 2025 r. każde spotkanie z Wenus zwiększy jej nachylenie orbity, powodując, że będzie ona „skakać” z płaszczyzny Układu Słonecznego, by zobaczyć widok. Tajemnicze polarne regiony Słońca.

Ten trzeci lot Wenus odbył się w niedzielę o 01:26[{” attribute=””>UTC (Saturday at 9:26 p.m. EDT), when Solar Orbiter passed 12,500 km (7,800 miles) from the planet’s center, which is very roughly 6,000 km (3,700 miles) from its gassy ‘surface’. In other words, it passed a distance half the width of Earth.

Its distance from Venus, angle of approach, and velocity were all carefully planned to get the precise desired effect from the planet’s large gravitational pull – getting the spacecraft closer to the Sun than ever before.

Solar Orbiter Flight Control Team during pre-launch simulations in 2020. Credit: ESA

“The close approach went exactly to plan, thanks to a great deal of planning from our colleagues in Flight Dynamics and the diligent care of the Flight Control Team,” explains Jose-Luis Pellon-Bailon, Solar Orbiter Operations Manager.

“By trading ‘orbital energy’ with Venus, Solar Orbiter has used the planet’s gravity to change its orbit without the need for masses of expensive fuel. When it returns to the Sun, the spacecraft’s closest approach will be about 4.5 million km (2.8 million miles) closer than before.”

Understanding particles that pose a radiation risk

Data beamed back to Earth since Solar Orbiter encountered the solar storm shows how its local environment changed as the large CME whooshed by. Although some instruments had to be turned off during its close approach to Venus, in order to protect them from stray sunlight reflected off of the planet’s surface, Solar Orbiter’s ‘in situ’ instruments remained on, recording an increase in solar energetic particles, among other things.

This composite image shows a SOHO image of the Sun and an artist’s impression of Earth’s magnetosphere. Credit: Magnetosphere: NASA, the Sun: ESA/NASA – SOHO

Particles, mostly protons and electrons, but also some ionized atoms like Helium, are constantly emitted by the Sun. When particularly large flares and ejections of plasma are blasted from the Sun, these particles are picked up and carried with them, accelerated to near relativistic speeds. It is these particles that pose a radiation risk to astronauts and spacecraft.

Improving our understanding of CMEs and tracking their progress as they sail through the Solar System is a big part of the Solar Orbiter’s mission. By observing CMEs, the solar wind, and the Sun’s magnetic field, the spacecraft’s ten science instruments are delivering new insight into how the 11-year cycle of solar activity works. Ultimately, these findings will help us better forecast periods of stormy space weather and protect planet Earth from the Sun’s violent outbursts.

Solar Orbiter’s suite of ten science instruments that will study the Sun. There are two types: in situ and remote sensing. The in situ instruments measure the conditions around the spacecraft itself. The remote-sensing instruments measure what is happening at large distances away. Together, both sets of data can be used to piece together a more complete picture of what is happening in the Sun’s corona and the solar wind. Credit: ESA-S.Poletti

Goodbye, halo?

This recent CME illustrates a difficulty in space weather observations. As seen in this footage from SOHO, a ‘full halo’ is seen when a CME is either coming straight at Earth, or in this case heading directly away, from the ‘far side’ of the Sun.

Large coronal mass ejection (CME) was recorded by the Solar and Heliospheric Observatory (SOHO) on August 30, 2022. The CME struck ESA’s Solar Orbiter spacecraft as it performed a flyby of Venus. Credit: ESA/NASA SOHO

It is tricky to determine if coronal mass ejections are coming towards Earth or moving away when viewed from Earth, because in both cases it appears to be expanding. One of the many benefits of the coming Vigil mission is that by combining the images taken from Earth’s direction and Vigil’s position at the ‘side’ of the Sun, the fifth Lagrange point, it will be easy and reliable to distinguish between an oncoming or departing storm.

Space weather gets deep

The Sun wields its influence on all the bodies of the Solar System. It’s the reason why no life could survive on the inner planets, as the sun makes their temperatures too hot and stripped away their atmospheres long ago.

As we venture from Earth to the Moon, it’s vital that we understand how space weather can affect human bodies, robots, communication systems, and plants and animals.

Solar Orbiter’s stellar views hint at Vigil’s future. Credit: ESA

As well as a wide range of tools to understand the Sun’s effect on Earth’s infrastructure, ESA’s Space Weather Service Network currently alerts teams flying missions throughout the Solar System of extreme space weather, with forecasts for Mercury, Venus, and Mars freely available via the Network’s Portal. Forecasts for Jupiter are on the way.

“Gathering data on events like this is crucial to understanding how they arise, improving our space weather models, forecasts, and early-warning systems,” explains Alexi Glover, ESA Space Weather Service Coordinator.

“Solar Orbiter is providing us with an excellent opportunity to compare our forecasts with real observations and test how well our models and tools perform for these regions.”