Will Parker Solar Probe set a new speed record during its closest Sun approach on December 24, 2024?
Yes • 50%
No • 50%
NASA press release or official mission updates
NASA's Parker Solar Probe to Make Historic Closest Approach to Sun at 3.8 Million Miles on Christmas Eve
Dec 22, 2024, 05:30 PM
NASA's Parker Solar Probe is set to achieve a historic milestone on Christmas Eve, December 24, 2024, by flying closer to the sun than any human-made object ever has. The spacecraft, on its 22nd orbit around the star, will approach within 3.8 million miles (6.1 million kilometers) of the sun's surface, marking the first of its three final closest flybys. Launched in 2018, the probe has been designed to withstand extreme temperatures up to 1,371 degrees Celsius and will travel at a speed of 430,000 mph (690,000 kph) during its closest approach. The mission aims to study the sun's corona and solar wind, providing insights into why the corona is significantly hotter than the sun's surface and how solar activity impacts Earth. Communication with the probe will be lost during the flyby, with mission managers expecting to receive a health update on December 27.
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430,000 mph or more • 25%
Less than 410,000 mph • 25%
Between 410,000 and 419,999 mph • 25%
Between 420,000 and 429,999 mph • 25%
Exceeds 430,000 mph • 25%
Between 420,000 and 430,000 mph • 25%
Between 410,000 and 420,000 mph • 25%
Below 410,000 mph • 25%
Less than 430,000 mph • 25%
430,000 mph • 25%
More than 430,000 mph • 25%
Exact speed unknown • 25%
800,000 km/h • 25%
750,000 km/h • 25%
700,000 km/h • 25%
No new record • 25%
Successful approach, no data collected • 25%
No confirmation received • 25%
Unsuccessful approach • 25%
Successful approach and data collection • 25%
More than 440,000 mph • 25%
Less than 420,000 mph • 25%
420,000 to 430,000 mph • 25%
430,000 to 440,000 mph • 25%
Yes • 50%
No • 50%
No • 50%
Yes • 50%
New insights on solar wind origins • 25%
Data not yet analyzed • 25%
Confirms previous solar wind models • 25%
No significant new information • 25%
Confirmation of existing theories • 25%
Technical issues prevented data collection • 25%
Significant new insights into solar corona • 25%
Inconclusive data • 25%