Mercury’s Comet-like Tail

Jan 27, 2020
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April 29, 2022

By Dr. Tony Phillips

mercury_strip.jpeg

This is NOT a comet, not even a meteor, but the planet Mercury, which is currently very close to the Pleiades,” says Voltmer. “How is the tail formed? The solar wind and micro-meteorites eject sodium atoms from Mercury’s surface. This creates a yellow-orange tail of sodium gas that is around 2.5 million kilometers long.”

People around the world have been watching Mercury climb up the evening sky this month. Some of them are probably wondering “why didn’t I see the tail?”

Answer: A special filter is required. “I used a 589 nm filter tuned to the yellow glow of sodium,” says Voltmer. Without this kind of sodium filter, Mercury’s tail would be invisible.

Dr Votmer setup_strip.jpeg
Dr. Sebastian Voltmer observing Mercury from La Palma on April 27, 2022. Inset is the 589 nm sodium filter. [video]

Voltmer says the tail is so bright, he could see it in individual 30 second exposures. “I can see some very small changes in shape of the tail,” he says, “and the brightness is slightly increasing.”

The nights ahead are excellent times to catch this phenomenon. On April 29th and 30th, Mercury will glide past the Pleiades star cluster for a fantastic photo-op. Then, on May 1st and 2nd, the crescent Moon joins the show.
“Currently I’m imaging Mercury day by day just after sunset from the Canary Islands,” says Voltmer. Stay tuned for more sodium.

See: https://spaceweatherarchive.com/2022/04/30/mercurys-comet-like-tail/

Seeing the planet Mercury with a long tail composed of sodium which is caused by the solar wind and micro-meteorites ejecting sodium atoms from Mercury’s surface when they strike it. The 2.5 million kilometers long yellow-orange tail of sodium gas, trailing the planet closest to the Sun, is an amazing sight when seen with the proper 589nm photographic filter.
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