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[3] [4] Further, the ALICE spectrograph on Rosetta determined that electrons (within 1 km (0.62 mi) above the comet nucleus) produced from photoionization of water molecules by solar radiation, and not photons from the Sun as thought earlier, are responsible for the degradation of water and carbon dioxide molecules released from the comet ...
The solid, core structure of a comet is known as the nucleus. Cometary nuclei are composed of an amalgamation of rock, dust, water ice, and frozen carbon dioxide, carbon monoxide, methane, and ammonia. [16] As such, they are popularly described as "dirty snowballs" after Fred Whipple's model. [17]
The coma is generally made of ice and comet dust. [1] Water composes up to 90% of the volatiles that outflow from the nucleus when the comet is within 3–4 au (280–370 million mi; 450–600 million km) from the Sun. [1] The H 2 O parent molecule is destroyed primarily through photodissociation and to a much smaller extent photoionization. [1]
Scientists say comet C/2023 A3 Tsuchinshan-ATLAS is visible once every 80,000 years, and people across North America were treated to stunning views. Striking photos show stunning, once-in-a ...
Comets carry and release grains containing volatiles in the ice phase into the inner solar system. Rosetta instruments detected besides the dominant water (H 2 O) molecules also carbon dioxide (CO 2), great variety of CH-, CHN-, CHS-, CHO-, CHO 2 - and CHNO-bearing saturated and unsaturated species, and the aromatic compound toluene (CH 3 –C ...
A rare comet is still glowing over Ohio. Here's how to see it before it's gone, and won't return for 80,000 years.
On Wednesday, the comet made its closest approach to our sun and on Saturday, October 12 at 11:39 a.m. it will be just 43,911,824 miles from Earth (its closest pass).
While the solid nucleus of comets is generally less than 30 km across, the coma may be larger than the Sun, and ion tails have been observed to extend 3.8 astronomical units (570 Gm; 350 × 10 ^ 6 mi). [6] The Ulysses spacecraft made an unexpected pass through the tail of the comet C/2006 P1 (Comet McNaught), on February 3, 2007. [7]