What is the primary goal of the Proba-3 mission?

The primary goal of the Proba-3 mission is to study the solar corona with unprecedented detail by creating an artificial solar eclipse using two satellites flying in precise formation.

How dose Proba-3 achieve such detailed observations of the solar corona?

Proba-3 achieves detailed observations by using two satellites flying 144 meters apart in millimeter-accurate formation, creating an artificial eclipse that allows for the study of the low solar corona.

What makes proba-3 diffrent from previous solar observation missions?

Unlike previous missions where the shading disc and binoculars were on the same probe, Proba-3 separates these components onto two different devices, allowing for observations of the low solar corona.

What kind of data is being gathered about the solar corona?

Proba-3 is gathering scientific data from the least explored part of the solar atmosphere, the low corona, which is just above the edge of the solar disk.According to ESA, the mission will give as much detailed observations of the solar corona within one six-hour observation window as we get in one century during the complete eclipse of the Sun.

who are some of the key contributors to the Proba-3 mission?

Key contributors include The Czech Republic, with coordination led by Dr. Stanislav Gunar and Prof. Petr Heinzel. The optical components of the ASPIICS coronograph were designed and produced by the Toptec Centre, and Serenum developed the protective doors for the coronograph.

When was Proba-3 launched, and where did the launch take place?

Proba-3 was launched in December from the Cosmodrome on the shore of the Gulf of Bengal, using the Indian launcher PSLV-XL.

Proba-3 Mission unveils Unprecedented Solar Corona Observations, Revolutionizing Space Weather Studies

A Groundbreaking European Space Agency (ESA) mission is set to transform our understanding of the Sun’s corona through innovative technology. The Proba-3 mission, utilizing two satellites flying in precise formation, has achieved unprecedented detailed observations of the solar corona. Initial data suggests that a mere six-hour window of observation by Proba-3 will yield as much detailed details as a century’s worth of observations during total solar eclipses.

Innovative Technology Behind the Mission

The Proba-3 mission employs a unique approach using breakthrough technology for satellite flights in highly accurate formation. This innovative technique enables the creation of a giant space coronograph known as ASPIICS (Associated Project for In-situ and Space-based Investigation of the Corona).

ASPIICS is distributed across two satellites: one bearing a disc that acts as an artificial moon to block the sun’s light, and the other carrying a coronograph to observe the faint corona. Separated by 144 meters and maintained in millimeter-accurate mutual position,ASPIICS can observe the solar corona under conditions that mimic a total solar eclipse. These conditions are far more controlled and stable than those achieved during a natural eclipse.

Did You Know? According to Nasa, the solar corona’s temperature can reach millions of degrees Fahrenheit, far hotter than the sun’s surface. The reasons for this extreme heat are still a mystery, making missions like Proba-3 crucial.

Czech Republic’s Critical Contribution

The Czech Republic has played a vital role in the Proba-3 mission since 2009. The Astronomical Institute of the Academy of Sciences of the Czech Republic, under the leadership of Dr. Stanislav Gunar and Professor Petr Heinzel, has coordinated the Czech participation. The Toptec Center, a part of the Institute of Plasma Physics of the ASCR, designed and produced the optical components for the ASPIICS coronograph.

Serenum is responsible for developing and manufacturing the protective doors for the coronograph, ensuring its sensitive instruments are safe during the mission. This international collaboration highlights the importance of shared expertise in advancing space exploration.

Exploring the low Corona

Scientists are notably excited about the opportunity to study the low corona. “This gives us scientific data from the area of low corona just above the edge of the solar disk. This area is the least explored part of the solar atmosphere,” explained Dr. Stanislav Gunar. This region is critical for understanding the origins of solar wind and coronal mass ejections, which can significantly impact space weather and affect Earth.

image of the solar corona captured by the ASPIICS coronograph — The green colour from the ASPIICS coronagraph captures a portion of the solar corona, which we could not observe in high resolution except during total solar eclipses. the solar disk is marked in yellow, and the high corona in red.

The official presentation of data from the ASPIICS coronograph took place at the Salon International de l’Aéronautique et de l’Espace, the world’s largest Air and space Technology Fair held biennially at Le Bourget Airport in Paris.ESA highlighted this achievement on its official website.

Comparing Proba-3 to Previous Missions

While previous satellites,including ACE,the NASA Solar Orbiter,and the SOHO observatory,have created artificial solar eclipses,Proba-3’s unique configuration sets it apart. In earlier missions,the shading disc and observing instruments were housed on the same probe. Proba-3’s separation of these components onto two distinct devices allows for unprecedented precision in observing the low corona.

Pro Tip: Observing the solar corona is crucial for predicting space weather events that can disrupt satellite communications,GPS systems,and even power grids on Earth. Space weather forecasting relies heavily on understanding coronal activity.

Mission	Focus	Unique Feature
Proba-3	Detailed observation of the low solar corona	Two satellites flying in precise formation with separated shading disc and coronograph.
ACE, Solar Orbiter, SOHO	Solar observation	Shading disc and observing instruments on the same probe.

The Proba-1 satellite, launched in 2001, tested the behavior of technology in space and concluded its mission in 2022. Proba-2,launched in 2009 and still operational,studies the Sun’s influence on our planet and explores space weather.

The Significance of Studying the Solar Corona

the Sun’s corona is the outermost part of the solar atmosphere, a region characterized by extreme heat and low density. Understanding the corona is vital for several reasons:

space weather Prediction: Coronal mass ejections (CMEs) and solar flares originating in the corona can cause notable disruptions to Earth’s magnetosphere, affecting satellite operations, interaction systems, and power grids.
Solar Wind Origins: The corona is the source of the solar wind, a continuous stream of charged particles that permeates the solar system. Understanding how the solar wind is accelerated from the corona is a fundamental question in astrophysics.
Coronal Heating Problem: The corona is millions of degrees hotter than the Sun’s surface. understanding this extreme heating mechanism remains one of the greatest challenges in solar physics.

Frequently Asked Questions About the Proba-3 mission

What is the primary goal of the Proba-3 mission?: The primary goal of the Proba-3 mission is to study the solar corona with unprecedented detail by creating an artificial solar eclipse using two satellites flying in precise formation.
How does Proba-3 achieve such detailed observations of the solar corona?: Proba-3 achieves detailed observations by using two satellites flying 144 meters apart in millimeter-accurate formation, creating an artificial eclipse that allows for the study of the low solar corona.
What makes Proba-3 different from previous solar observation missions?: Unlike previous missions where the shading disc and binoculars were on the same probe, Proba-3 separates these components onto two different devices, allowing for observations of the low solar corona.
What kind of data is being gathered about the solar corona?: Proba-3 is gathering scientific data from the least explored part of the solar atmosphere, the low corona, which is just above the edge of the solar disk. According to ESA, the mission will give as much detailed observations of the solar corona within one six-hour observation window as we get in one century during the complete eclipse of the Sun.
Who are some of the key contributors to the Proba-3 mission?: Key contributors include The Czech Republic, with coordination led by Dr. Stanislav Gunar and Prof. Petr Heinzel. The optical components of the ASPIICS coronograph were designed and produced by the Toptec Center, and Serenum developed the protective doors for the coronograph.
When was Proba-3 launched, and where did the launch take place?: Proba-3 was launched in December from the Cosmodrome on the shore of the Gulf of Bengal, using the Indian launcher PSLV-XL.

How do you think these new observations of the solar corona will change our understanding of space weather? What other mysteries of the Sun do you hope future missions will uncover?

Share your thoughts and join the discussion below!

European Space Agency (ESA)

Czechs & the First Artificial Solar Eclipse