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What is the Parker Solar Probe?

The Parker Solar Probe is a robotic spacecraft launched by NASA in 2018 to study the Sun and its outer atmosphere. It is the first spacecraft to fly directly into the Sun's corona, the outermost part of its atmosphere. The mission is named after solar astrophysicist Eugene Parker.

The Parker Solar Probe is a spacecraft developed by NASA that was launched in August 2018. Its mission is to study the Sun up close and gather valuable data about its outer atmosphere, known as the corona. This information will help scientists better understand the processes occurring within the corona and the solar wind, which is the stream of charged particles coming from the Sun.

To find more details about the Parker Solar Probe, you can follow these steps:

1. Open a web browser on your computer or mobile device.
2. Type "Parker Solar Probe" in the search bar and press Enter.
3. Look for results from reliable sources such as NASA's official website, scientific journals, or reputable news outlets.
4. Click on the relevant links to access the information about the Parker Solar Probe.
5. Read the provided content to learn about the probe's objectives, scientific instruments, mission timeline, and any recent discoveries or significant updates.

Remember to evaluate the credibility of the sources you find and cross-reference the information to ensure accuracy.

The Parker Solar Probe is a NASA spacecraft designed to study the Sun at close proximity. Its main mission is to gather valuable data about the solar wind, the phenomenon of energetic particles emitted by the Sun, and to investigate the Sun's outer atmosphere, known as the corona. The spacecraft was launched on August 12, 2018, and it will make a total of 24 close approaches to the Sun over seven years, gradually getting closer with each pass. It will come within about 4 million miles (6 million kilometers) of the Sun's surface, which is closer than any previous spacecraft. The probe is named after Eugene Parker, a physicist who made significant contributions to our understanding of solar wind and solar physics.