0648 GMT April 02, 2020
The Solar Orbiter, or SolO, probe will put itself inside the orbit of Planet Mercury to train its telescopes on the surface of our star, BBC reported.
Other instruments will sense the constant outflow of particles and their embedded magnetic fields.
Scientists hope the detailed observations can help them understand better what drives the Sun's activity.
This goes up and down on an 11-year cycle. It's sure to be a fascinating endeavor but it's one that has direct relevance to everyone on Earth.
The energetic outbursts from our star have the ability to damage satellites, harm astronauts, degrade radio communications, and even knock power grids offline.
"We're doing this not just for the sake of increasing our knowledge but also for being able to take precautions, for example by putting satellites in safe mode when we know big solar storms are coming or letting astronauts not leave the space station on these days," said Daniel Müller, the European Space Agency (ESA) project scientist on SolO.
The probe was assembled in Stevenage, UK, by Airbus (Britain has invested €220 million in the €1.5 billion project), with the past year spent at the IABG facility in Ottobrunn, Germany, for testing.
The spacecraft has cleared its checks and will now ship out to Florida to be mated with the Atlas rocket that will hurl it toward the Sun in early February.
SolO was first conceived in the late 1990s with the industrial contract to produce it awarded in 2012.
A key challenge has been to mature technologies that can protect a probe that flies to within 43 million kilometers of our star.
Temperatures at this proximity will get up to 600°C.
SolO's plan to survive these conditions involves hiding behind a large titanium shield, and cooling itself with a complex series of radiators.
Sophisticated fault-recovery systems will also ensure SolO stays out of trouble.
"If we de-point, we very quickly run into difficulty thermally," explained Airbus project manager Ian Walters.
"Our requirement is to make sure we recover under any failure scenario within 50 seconds and actually our spacecraft will go back to normal pointing in 22 seconds, all autonomously."
But the probe still needs to observe the star and to do that it must use peepholes in the shield.
These will briefly open to allow the telescopes to grab their observations before closing shut again.
The pictures and movies that come back will be unprecedented in their fine resolution.
Features as small as 70km across will be visible.
"It's amazing; every time we get better resolution we see more and more," said Holly Gilbert, the US space agency's deputy project scientist on the mission.
"The interactions between the Sun's plasma (energetic gas) and its magnetic field are incredibly dynamic, not just on the large scales but on the very, very small scales.
"When the magnetic fields interact in a very explosive process called reconnection — that's a very small region.
"And to see how that leads to eruptions, we need to see the small stuff that's happening."
One of the major differences between this mission and all previous such ventures is that SolO will get to take the first close-up images of our star's polar regions.
The high latitudes are known to be significant locations for magnetic behavior and the generation of the fastest outflows of particles.
"We've never seen the solar poles directly because from Earth we just have a very grazing view," said Frédéric Auchère, a mission principal investigator from the Institut d'Astrophysique Spatiale, Orsay, France.
"But these regions are very important because they are the source of the very fast solar wind and we also know that in the solar interior things are happening at the poles that may be the key to understanding solar activity and the solar cycle."