#space_observation

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Hubble’s image of spiral galaxy NGC 6951 shows its bright blue spiral arms, bars, patches of star clusters, and clumps of dust. The galaxy NGC 6951, which lies 78 million light-years from Earth, was captured in a new Hubble image created by the Wide Field Camera (WFC3) and the Advanced Camera for Surveys (ACS). The image shows bright blue spiral arms, star clusters, and a dark orange dust cloud. The history of this galaxy is quite amazing. About 800 million years ago, NGC 6951 was known for its high rate of star formation, but then star formation stopped for 300 million […]

Hubble's image of spiral galaxy NGC 6951 shows its bright blue spiral arms, bars, patches of star clusters, and clumps of dust. The galaxy NGC 6951, which lies 78 million light-years from Earth, was captured in a new Hubble image created by the Wide Field Camera (WFC3) and the Advanced Camera for Surveys (ACS). The image shows bright blue spiral arms, star clusters, and a dark orange dust cloud. [caption id="attachment_64740" align="aligncenter" width="780"] spiral galaxy NGC 6951[/caption] The history of this galaxy is quite amazing. About 800 million years ago, NGC 6951 was known for its high rate of star formation, but then star formation stopped for 300 million years. Over the past 25 years, six powerful supernova explosions have occurred, causing the extinction of some of these stars. The average age of a star cluster in the galaxy is between 200 and 300 million years, but some have reached the age of one billion years. An angle straight to the heart: Hubble captured a detailed image of the spiral galaxy NGC 6951 NGC 6951 is classified as a Type II Seyfert galaxy due to its infrared emission and the presence of a slow-moving gaseous environment at the center. However, some astronomers also consider it to be a low-ionization galaxy with an emission line in the core, implying a cooler and less ionized core. Near the center of the galaxy lies a supermassive black hole, which is surrounded by a ring of stars, gas, and dust with a diameter of about 3,700 light years. This ring is also known as the "central ring" and is thought to have star formation for 1 to 1.5 billion years, with 40% of its mass consisting of stars less than 100 million years old. This image of NGC 6951 is part of NASA's Hubble Photo Sharing Campaign, which features new images taken by the space telescope every day from October 2 to October 7.

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Scientists from Italy and Germany have discovered exoplanet GJ 367b, which is likely composed entirely of iron. Using the HARPS spectrograph and TESS observations, they found that more than 90% of the planet’s mass is made up of its iron core. Researchers from the University of Turin in Italy and the State Star Observatory of Thuringia in Germany have made an interesting discovery: the exoplanet GJ 367b is most likely composed entirely of iron. This makes it the densest known planet with a short orbital period. GJ 367b was first spotted in 2015 by NASA’s TESS (Transiting Exoplanet Survey Satellite) space telescope […]

Scientists from Italy and Germany have discovered exoplanet GJ 367b, which is likely composed entirely of iron. Using the HARPS spectrograph and TESS observations, they found that more than 90% of the planet's mass is made up of its iron core. Researchers from the University of Turin in Italy and the State Star Observatory of Thuringia in Germany have made an interesting discovery: the exoplanet GJ 367b is most likely composed entirely of iron.  This makes it the densest known planet with a short orbital period. GJ 367b was first spotted in 2015 by NASA's TESS (Transiting Exoplanet Survey Satellite) space telescope and has a density 1.85 times that of Earth. [caption id="attachment_69273" align="aligncenter" width="780"] GJ 367b[/caption] Using the European Southern Observatory's HARPS spectrograph and TESS observations, scientists determined that more than 90% of the planet's mass is made up of its iron core. The origin story of GJ 367b remains a mystery, but it may have once been a rocky planet like Earth or Mars. Its two neighboring planets, orbiting further out, are also rocky, indicating that they all formed in a similar way. GJ 367b is an exoplanet consisting only of an iron core However, GJ 367b likely went through a unique series of events that led it to lose its outer rocky layers, leaving only the core. Possible explanations include collisions with another planet closer to the host star. Another possibility is that GJ 367b was intensely irradiated by its star, causing its outer layer to burn away leaving only an iron core. The outer material could turn into gas and then be dispersed into space. It is also possible that GJ 367b underwent a combination of collisions and irradiation to form the metallic planet that astronomers observe today. The question still remains: how did GJ 367b get so close to its star? It is unlikely that it formed there. Scientists believe that gravitational interactions with other planets could have caused it to move away from its original formation site. Further study of GJ 367b could provide valuable insights into the formation and evolution of rocky and short-period planets.