Astronet Астронет: Астрономическая картинка дня Изменяющийся ионный хвост кометы Понса-Брукса
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APOD: 2024 April 8 Б The Changing Ion Tail of Comet Pons Brooks
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APOD: 2024 April 8 Б The Changing Ion Tail of Comet Pons Brooks
Credit & Copyright: Shengyu Li & Shaining
Explanation: How does a comet tail change? It depends on the comet. The ion tail of Comet 12P/PonsБBrooks has been changing markedly, as detailed in the featured image sequenced over nine days from March 6 to 14 (top to bottom). On some days, the comet's ion tail was relatively long and complex, but not every day. Reasons for tail changes include the rate of ejection of material from the comet's nucleus, the strength and complexity of the passing solar wind, and the rotation rate of the comet. Over the course of a week, apparent changes even include a change of perspective from the Earth. In general, a comet's ion tail will point away from the Sun, as gas expelled is pushed out by the Sun's wind. Today, Pons-Brooks may become a rare comet suddenly visible in the middle of the day for those able to see the Sun totally eclipsed by the Moon.

NASA Coverage: Today's Total Solar Eclipse
Total Eclipse Imagery: Notable Submissions to APOD

Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

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Based on Astronomy Picture Of the Day

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