How will comet K2’s journey end soon… Know the details of its approach to the sun…

Thank you for reading the news: How will comet K2’s journey end soon? I know the details of its approach to the sun…

Basrawi News Encyclopedia – I wrote: Nermin Salem Comet K2 passed close to Earth, and it will become brighter during the summer as it will approach its closest point to the sun in December, and it was first observed in 2017 by the Panoramic Survey Telescope and Rapid Response System (PanSTARRS) in The outer regions of the solar system.

According to the American “space” website, K2 is now continuing its journey to the sun and will take its closest approach to the star that orbits around it, the so-called perihelion in December, and the comet, which can be seen these days by large amateur telescopes, may shine in the warmer environment near the sun.

The first observations of the comet revealed a potentially large nucleus and a huge envelope of gas and dust, and at that time, the comet was located between the orbits of Saturn and Uranus, about 1.49 billion miles (2.4 billion km) from the sun, which is about 16 times farther from Earth than from the sun. .

The fact that K2 did indeed melt at the frigid temperatures in the depths of the Solar System surprised us that comets, made mostly of water ice, are supposed to be static and dead like rocks.

Scientists are still debating the comet’s size, and the Canada-France-Hawaii Telescope (CFHT) suggested that K2’s nucleus could be between 18 and 100 miles (30 to 160 km) wide, but data from the Hubble Space Telescope showed that it could be 11 miles wide. 18 km) only.

Comet activity is always difficult to predict, as we can’t say exactly how the Sun’s heat will affect K2 or whether it will survive at all.

The comet now rests at about 7 or 8 on the Richter scale, and the comet will remain visible in telescopes for at least the rest of the summer.

The comet was getting brighter as it moved towards the inner solar system, so the comet may become brighter in the coming weeks so that more people can see it far from the images coming from larger observatories and may completely dissolve as it approaches the sun and end its journey that began from the depths of the solar system.

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