Magazine Posts

NASA Astronomy Picture of the Day:

What created this huge space bubble? Blown by the wind from a star, this tantalizing, head-like apparition is cataloged as NGC 7635, but known simply as the Bubble Nebula. Taken from Krakow, Poland, the featured view utilizes a long exposure to reveal the intricate details of this cosmic bubble and its environment. Although it looks delicate, the 10 light-year diameter bubble offers evidence of violent processes at work. Seen here right of the Bubble's center, a bright hot star is embedded in the nebula's reflecting dust. A fierce stellar wind and intense radiation from the star, which likely has a mass 10 to 20 times that of the Sun, has blasted out the structure of glowing gas against denser material in a surrounding molecular cloud. The intriguing Bubble Nebula lies a mere 11,000 light-years away toward the boastful constellation Cassiopeia.

Photo by Paweł Piechnik

Haigerloch, Germany: view of Haigerloch Castle and the castle church with the surrounding valley.

Roman Eisele, CC BY-SA 4.0, via Wikimedia Commons. View source.

James Abbott McNeill Whistler - (1834 - 1903), American painter in oils and watercolor, and printmaker. He lived mostly in the United Kingdom. He was a leading proponent of the credo "art for art's sake"

NASA Astronomy Picture of the Day:

How do clusters of galaxies form? Since our universe moves too slowly to watch, faster-moving computer simulations are created to help find out. One famous effort is TNG50 from IllustrisTNG, an upgrade of the famous Illustris Simulation. The first part of the featured video tracks cosmic gas (mostly hydrogen) as it evolves into galaxies and galaxy clusters from the early universe to today, with brighter colors marking faster moving gas. As the universe matures, gas falls into gravitational wells, galaxies forms, galaxies spin, galaxies collide and merge, all while black holes form in galaxy centers and expel surrounding gas at high speeds. The second half of the video switches to tracking stars, showing a galaxy cluster coming together, complete with stellar streams. The outflow from black holes in TNG50 is surprisingly complex and details are being compared with our real universe. Studying how gas coalesced in the early universe helps humanity better understand how our Earth, Sun, and Solar System originally formed. Explore the Universe: Random APOD Generator

Watch NASA's Astronomy Video of the Day

Magnus Cort in the French Alps on Tour de France 2024. Tour de France will finish today on the Champs-Élysées in Paris.

kallerna, CC BY-SA 4.0, via Wikimedia Commons. View source.

NASA Astronomy Picture of the Day:

The Seas of Tranquility and Serenity are calm today. They're calm most every day though, since they are actually lunar maria, ancient lava flows filling in large impact basins on the Moon. Also known by Latin names Mare Tranquillitatis (right) and Mare Serenitatis, the smooth dark lunar "seas" are in stark contrast to the bright cratered lunar highlands surrounding them in this telescopic view. Of course their names are based on the historical, pre-telescopic designations of lunar maria. Easily visible to the unaided eye, the broad features on the Moon's near side were imagined to be like the expansive oceans of planet Earth. On July 20, 1969, the Apollo 11 lunar module Eagle touched down on the Mare Tranquillitatis (at lower right), establishing Tranquility base and the first human presence on the Moon.

Photo by Tranquility

Soviet FD20 steam locomotive exposed at Zuyevka railway station, Kirov Oblast, Russia.

A.Savin, FAL, via Wikimedia Commons. View source.

Welcome to Kudos365 Weekly History Challenge. Test your history  knowledge and see how many of the history questions you can answer correctly. A new updated History Challenge is released every Saturday.

NASA Astronomy Picture of the Day:

In 185 AD, Chinese astronomers recorded the appearance of a new star in the Nanmen asterism. That part of the sky is identified with part of the southern constellation Centaurus on modern star charts. In fact, the new star was reported to be visible to the naked-eye for months before it faded from view, and is now thought to be the earliest recorded supernova. In this 21st century telescopic image, the wispy outlines of a faint emission nebula recognized as the remnant of that historical stellar explosion can be traced against a starry background. The ragged but roughly circular extent of the nebula, cataloged as RCW 86, represents interstellar gas ionized by the supernova's still expanding shock wave. Space-based images indicate an abundance of the element iron in RCW 86 and the absence of a neutron star or pulsar within the remnant, suggesting that the original supernova was Type Ia. Unlike the core collapse supernova explosion of a massive star, a Type Ia supernova is a thermonuclear detonation on a white dwarf star that has accreted material from its companion in a binary star system. Near the plane of our Milky Way galaxy and larger than the full moon on the sky this supernova remnant is too faint to be seen by eye though. RCW 86 is some 8,000 light-years distant and around 100 light-years across.

Photo by Chinese astronomers

Photograph of Machu Picchu taken in 1912 by Hiram Bingham during the Yale Peruvian Expedition. The site, an important Inca citadel in the Andes of Peru, had been visited earlier by local people such as Agustín Lizárraga in 1902, and was later brought to international attention through Bingham’s expeditions of 1911 and 1912. Today marks the anniversary of Bingham’s 1911 visit, which contributed to its worldwide recognition.

Hiram Bingham III, Public domain, via Wikimedia Commons. View source.