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Officially known as C/2022 E3 (ZTF), the comet orbits the Sun every 50,000 years and is expected to approach our planet on February 1, 2023.

E3 was discovered in March, but scientists recently took the first detailed image to reveal it.

While the comet is too faint to see without a telescope, it should be visible to the unaided eye when it’s about 26 million miles away.

And in early March, astronomers discovered comet C/2022 E3 (ZTF) using the Zwicky Transit Facility’s Wide Field Survey Camera.

The comet is currently 117 million miles from Earth and is expected to reach the sun on Jan. 1, orbit it, and make its closest approach to our planet.

E3 will be the first comet seen with the naked eye by NEOWISE in July 2020.

However, NEOWISE has left a long, fuzzy tail and E3 will likely appear as a gray streak in the night sky.

E3 should be visible by January 26, but peaks on February 1.

And this comet isn’t the only cosmic show scheduled for 2023, as it will start the year with the annual quadruple meteor show and end with the impressive Geminid meteor in December.

The Quadrantid is one of the most spectacular meteor showers of the year, and you don’t need specialized equipment to see it.

While the meteor shower technically started today, it will peak on the night of Jan. 3 and the morning of Jan. 4.

However, at the extremes, up to 200 bright stars can be seen per hour, but this depends on ideal conditions and ideal location on Earth.

As the year 2023 draws to a close, the Geminid meteor will light up the sky from December 13-14.

Meteorites are mostly white but can be yellow, green, red or blue.

While most meteor showers are caused by comets, the Geminid meteor shower is unique in that the scene is produced as Earth passes through a trail of debris from an asteroid known as 3200 Phaethon.

Geminids meteor showers were first reported in 1862, but it wasn’t until 1983 that scientists pinpointed the source of 3200 Phaethon.

They are called Geminids because when the Earth passes through the debris, it illuminates the star Castor in the constellation Gemini.

AMD Software, Radeon Software, Adrenalin, and various other names have been used in the past, but regardless of the name, AMD has continued to iterate and improve the software experience for its GPUs. And the version we have now is a big reason why AMD can use the best graphics cards, Digitartlends reported.

The biggest advantage of AMD software is that all your settings are in one place.

It doesn’t seem like a big deal until you actually want to take advantage of the many software features available for Nvidia and AMD graphics cards.

NASA has released new images of a 100-million-year-old globular star cluster about 160,000 light-years away in the constellation Swordfish, according to RT.

And while the new images from the Hubble Space Telescope may look startlingly different, they’re actually images of the same cosmic body called NGC 1850.

Although both images were taken by the same Hubble instrument, different filters with different custom colors were used to study specific wavelengths of light emitted by these objects.

The blue-blurred image includes some near-infrared light along with visible light (what our human eyes can detect), while the red-blurred image covers a much wider range from the near-ultraviolet to the infrared spectrum. primordial infrared.

Observations in the ultraviolet are ideal for detecting the light from hotter, dimmer stars, as seen in this bright starscape.

This globular cluster, which is 100 million years old, is found in the Large Magellanic Cloud, a satellite galaxy of the Milky Way home to billions of stars.

The cluster is located about 160,000 light-years away in the constellation Swordfish. Like other globular clusters of galaxies, NGC 1850 is a densely packed globular cluster of stars bound together by each other’s gravity.

Unlike most globular clusters, the stars in NGC 1850 are relatively young, and in our galaxy, the Milky Way, there are no globular clusters with stars as young as NGC 1850.

Astrophysicists believe that when the first generation of stars were born in NGC 1850, the stars spewed matter such as dust and gas into the surrounding universe.

The density of the newly formed star cluster was so high that this ejected material could not escape the cluster’s gravity, forcing it to remain nearby.

The intense gravity of the cluster draws hydrogen and helium from its surroundings.

These two sources of gas have met to form a second generation of stars, which increases the density and size of this globular cluster.

And in 2021, scientists discovered the presence of a black hole in NGC 1850. They also discovered many brighter blue stars, which burn hotter and die before the age of red stars.

There are also about 200 red giants, which are stars that have run out of hydrogen at their centers and fuse hydrogen away from their cores, causing the outer layers to expand, cool, and glow red.

The cluster is surrounded by a pattern of haze, diffuse dust and gas thought to come from supernova explosions (blue veil-like structures in the first image and red in the second).

NGC 1850’s mass is about 63,000 times the mass of the Sun, and its inner core is about 20 light-years in diameter.

Astronomers used observations from the Hubble Space Telescope over a wide range of wavelengths to view this large star cluster and learn more about star formation.