#dust ionizer

[kyodoindia]

Medical Equipment Suppliers in Delhi | Quick Mold Change System: Kyodo India

In the dynamic and critical industry of medical equipment supply, selecting the correct partner can have a considerable impact on the efficiency and efficacy of healthcare services. Among the leading players in this business, Kyodo India stands out as a top choice for medical equipment suppliers in Delhi. Kyodo India has built out a niche in the competitive market by focusing on innovation, quality, and client happiness. This article explores what makes Kyodo India a market leader in medical equipment supply, including revolutionary technology such as the Quick Mold Change System and Quick DIE Change System.

Why Kyodo India is a Top Medical Equipment Supplier in Delhi

1. Comprehensive Product Range

Kyodo India is well-known for its vast range of medical equipment, which caters to a variety of needs in the healthcare sector. The company provides high-quality items across several categories, such as diagnostic equipment, medicinal devices, and surgical instruments. Their extensive product line guarantees that healthcare facilities may obtain all of the necessary equipment from a single reliable provider, reducing procurement processes and increasing operational efficiency.

2. Commitment to Quality and Compliance

One of the main things that distinguishes Kyodo India from other medical equipment suppliers in Delhi is its continuous commitment to quality. Kyodo India’s products meet high quality and regulatory criteria. The company assures that its medical equipment fulfills worldwide quality standards, delivering dependable and safe solutions to healthcare practitioners.

Kyodo India’s commitment to these standards is critical in an industry where precision and dependability are essential. By upholding high quality standards, Kyodo India not only improves patient safety but also fosters trust among healthcare professionals and institutions.

3. Innovative Technologies: Quick Mold Change System and Quick DIE Change System

Kyodo India is in the forefront of integrating cutting-edge technology into its products. Two of the company’s notable technologies are the Quick Mold Change System and the Quick DIE Change System. These technologies are especially useful for increasing the efficiency of medical equipment manufacturing and maintenance.

Quick Mold Change System

Kyodo India created the Quick Mold Change System to expedite the manufacturing process by considerably lowering the time necessary to change molds. This technique is especially beneficial in the manufacturing of medical equipment, where precision and quick turnaround are essential.

The Quick Mold Change System offers the following advantages:

● Increased Productivity: By lowering mold change times, the technology enables more efficient production cycles, resulting in higher output and less downtime.

● Enhanced Flexibility: The system allows for quick adaptability to changing manufacturing requirements, making it easier to convert between different medical equipment models.

● Cost Efficiency: Faster mold changes lead to cheaper production costs and greater resource usage.

Quick DIE Change System

Kyodo India’s Quick DIE changing System, like the Quick Mold Change System, is designed to optimize the die changing process in manufacturing. This technology is critical for sectors that require frequent die replacements, such as those that manufacture sophisticated medical devices.

Key advantages of the Quick DIE Change System include:

● Reduced Changeover Time: The technology reduces the time required to swap dies, which improves overall production efficiency.

● Improved Accuracy: Quick DIE changes keep manufacturing operations precise and consistent, which is essential for high-quality medical equipment.

● Operational Flexibility: The system enables quick adjustments to meet changing production demands, improving the responsiveness of manufacturing operations.

4. Customer-Centric Approach

Kyodo India’s success as a major medical equipment supplier is also due to its customer-centric approach. The organization emphasizes knowing and meeting its clients’ individual demands. This technique involves the following:

● Personalized Service: Kyodo India offers bespoke solutions to address the specific needs of various healthcare facilities. Their team works closely with clients to ensure that the equipment delivered meets their operational requirements.

● Kyodo India provides full support, from pre-sales consultations to post-sales support, to guarantee that their equipment is integrated and used smoothly.

● Training and Maintenance: The organization educates healthcare workers on the proper use of equipment and provides maintenance services to ensure long-term performance and reliability.

5. Strong Industry Reputation

Kyodo India has established a solid name in the medical equipment business by delivering consistent results and exceeding customer expectations. The company’s commitment to providing high-quality products and innovative solutions has gained it the trust of several healthcare facilities in Delhi and elsewhere.

This reputation is evident in the good feedback and long-term connections that Kyodo India has built with its clients. The company’s dedication to excellence is demonstrated by its ability to continually meet and exceed client expectations.

Kyodo India is the Right Choice!

In the competitive landscape of medical equipment suppliers in Delhi, Kyodo India stands out for its diverse product offering, dedication to quality, and innovative technologies. The Quick Mold Change System and Quick DIE Change System are excellent examples of how the company uses sophisticated technology to improve manufacturing productivity and suit the changing needs of the healthcare sector.

For healthcare professionals looking for a dependable and forward-thinking medical equipment supplier, Kyodo India is an excellent alternative. Their commitment to quality, customer service, and technical innovation has positioned them as an industry leader.

Visit Kyodo India’s website to learn about their vast selection of medical equipment and technological solutions. Learn how Kyodo India can provide your healthcare facility with high-quality equipment and exceptional services.

[x-heesy]

Lagoon Cocoon by geckzilla on Flickr. (Judy Schmidt)

[nasa]

A Tour of Cosmic Temperatures

We often think of space as “cold,” but its temperature can vary enormously depending on where you visit. If the difference between summer and winter on Earth feels extreme, imagine the range of temperatures between the coldest and hottest places in the universe — it’s trillions of degrees! So let’s take a tour of cosmic temperatures … from the coldest spots to the hottest temperatures yet achieved.

First, a little vocabulary: Astronomers use the Kelvin temperature scale, which is represented by the symbol K. Going up by 1 K is the same as going up 1°C, but the scale begins at 0 K, or -273°C, which is also called absolute zero. This is the temperature where the atoms in stuff stop moving. We’ll measure our temperatures in this tour in kelvins, but also convert them to make them more familiar!

We’ll start on the chilly end of the scale with our CAL (Cold Atom Lab) on the International Space Station, which can chill atoms to within one ten billionth of a degree above 0 K, just a fraction above absolute zero.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Just slightly warmer is the Resolve sensor inside XRISM, pronounced “crism,” short for the X-ray Imaging and Spectroscopy Mission. This is an international collaboration led by JAXA (Japan Aerospace Exploration Agency) with NASA and ESA (European Space Agency). Resolve operates at one twentieth of a degree above 0 K. Why? To measure the heat from individual X-rays striking its 36 pixels!

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Resolve and CAL are both colder than the Boomerang Nebula, the coldest known region in the cosmos at just 1 K! This cloud of dust and gas left over from a Sun-like star is about 5,000 light-years from Earth. Scientists are studying why it’s colder than the natural background temperature of deep space.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Let’s talk about some temperatures closer to home. Icy gas giant Neptune is the coldest major planet. It has an average temperature of 72 K at the height in its atmosphere where the pressure is equivalent to sea level on Earth. Explore how that compares to other objects in our solar system!

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

How about Earth? According to NOAA, Death Valley set the world’s surface air temperature record on July 10, 1913. This record of 330 K has yet to be broken — but recent heat waves have come close. (If you’re curious about the coldest temperature measured on Earth, that’d be 183.95 K (-128.6°F or -89.2°C) at Vostok Station, Antarctica, on July 21, 1983.)

We monitor Earth's global average temperature to understand how our planet is changing due to human activities. Last year, 2023, was the warmest year on our record, which stretches back to 1880.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

The inside of our planet is even hotter. Earth’s inner core is a solid sphere made of iron and nickel that’s about 759 miles (1,221 kilometers) in radius. It reaches temperatures up to 5,600 K.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

We might assume stars would be much hotter than our planet, but the surface of Rigel is only about twice the temperature of Earth’s core at 11,000 K. Rigel is a young, blue star in the constellation Orion, and one of the brightest stars in our night sky.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger 

We study temperatures on large and small scales. The electrons in hydrogen, the most abundant element in the universe, can be stripped away from their atoms in a process called ionization at a temperature around 158,000 K. When these electrons join back up with ionized atoms, light is produced. Ionization is what makes some clouds of gas and dust, like the Orion Nebula, glow.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

We already talked about the temperature on a star’s surface, but the material surrounding a star gets much, much hotter! Our Sun’s surface is about 5,800 K (10,000°F or 5,500°C), but the outermost layer of the solar atmosphere, called the corona, can reach millions of kelvins.

Our Parker Solar Probe became the first spacecraft to fly through the corona in 2021, helping us answer questions like why it is so much hotter than the Sun's surface. This is one of the mysteries of the Sun that solar scientists have been trying to figure out for years.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Looking for a hotter spot? Located about 240 million light-years away, the Perseus galaxy cluster contains thousands of galaxies. It’s surrounded by a vast cloud of gas heated up to tens of millions of kelvins that glows in X-ray light. Our telescopes found a giant wave rolling through this cluster’s hot gas, likely due to a smaller cluster grazing it billions of years ago.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Now things are really starting to heat up! When massive stars — ones with eight times the mass of our Sun or more — run out of fuel, they put on a show. On their way to becoming black holes or neutron stars, these stars will shed their outer layers in a supernova explosion. These layers can reach temperatures of 300 million K!

Credit: NASA's Goddard Space Flight Center/Jeremy Schnittman

We couldn’t explore cosmic temperatures without talking about black holes. When stuff gets too close to a black hole, it can become part of a hot, orbiting debris disk with a conical corona swirling above it. As the material churns, it heats up and emits light, making it glow. This hot environment, which can reach temperatures of a billion kelvins, helps us find and study black holes even though they don’t emit light themselves.

JAXA’s XRISM telescope, which we mentioned at the start of our tour, uses its supercool Resolve detector to explore the scorching conditions around these intriguing, extreme objects.

Credit: NASA's Goddard Space Flight Center/CI Lab

Our universe’s origins are even hotter. Just one second after the big bang, our tiny, baby universe consisted of an extremely hot — around 10 billion K — “soup” of light and particles. It had to cool for a few minutes before the first elements could form. The oldest light we can see, the cosmic microwave background, is from about 380,000 years after the big bang, and shows us the heat left over from these earlier moments.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

We’ve ventured far in distance and time … but the final spot on our temperature adventure is back on Earth! Scientists use the Large Hadron Collider at CERN to smash teensy particles together at superspeeds to simulate the conditions of the early universe. In 2012, they generated a plasma that was over 5 trillion K, setting a world record for the highest human-made temperature.

Want this tour as a poster? You can download it here in a vertical or horizontal version!

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Explore the wonderful and weird cosmos with NASA Universe on X, Facebook, and Instagram. And make sure to follow us on Tumblr for your regular dose of space!

[spacevoyagerx]

Veil Nebula

The Veil Nebula is a stunning supernova remnant located in the constellation Cygnus, often referred to as the "Wings of the Swan" .

It is approximately 1,500 light-years away from Earth and spans about 110 light-years across.

The nebula is composed of ionized gas and dust, and it is known for its intricate and delicate filaments, which are the remnants of a massive star that exploded around 8,000 years ago.

The Veil Nebula is divided into several parts, with the most prominent sections being the Eastern Veil (NGC 6992) and the Western Veil (NGC 6960).

Credits: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

[apod]

2024 December 13

M51: Tidal Streams and H-alpha Cliffs Image Credit & Copyright: The Deep Sky Collective - Tim Schaeffer, Carl Björk, Steeve Body, Fabian Neyer, Aki Jain, Ryan Wierckx, Paul Kent, Brian Valente, Antoine & Dalia Grelin, Nicolas Puig, Stephen Guberski, Mike Hamende, Julian Shapiro, John Dziuba, Mikhail Vasilev, Bogdan Borz, Adrien Keijzer

Explanation: An intriguing pair of interacting galaxies, M51 is the 51st entry in Charles Messier's famous catalog. Perhaps the original spiral nebula, the large galaxy with whirlpool-like spiral structure seen nearly face-on is also cataloged as NGC 5194. Its spiral arms and dust lanes sweep in front of its smaller companion galaxy, NGC 5195. Some 31 million light-years distant, within the boundaries of the well-trained constellation Canes Venatici, M51 looks faint and fuzzy to the eye in direct telescopic views. But this remarkably deep image shows off stunning details of the galaxy pair's striking colors and fainter tidal streams. The image includes extensive narrowband data to highlight a vast reddish cloud of ionized hydrogen gas recently discovered in the M51 system and known to some as the H-alpha cliffs. Foreground dust clouds in the Milky Way and distant background galaxies are captured in the wide-field view. A continuing collaboration of astro-imagers using telescopes on planet Earth assembled over 3 weeks of exposure time to create this evolving portrait of M51.

∞ Source: apod.nasa.gov/apod/ap241213.html

[all-roads-are-now-bent]

Caldwell 33//NGC 6992//Eastern Veil Nubula. Photo taken and processed by me.

A cloud of heated and ionized dust located 2,400ly from earth. Part of the Cygnus Loop, this is the remnant of a star 20 times more massive than our sun that went supernova 10,000–20,000 years ago. At the time, the resulting explosion would have appeared brighter than Venus in the night sky and would have been visible during the daytime.

[shaythempronouns]

IC 5146 - the Cocoon Nebula (HaRGB)

An especially fun target to shoot, because it's a combination emission and reflection nebula. The red in its center is ionized hydrogen, which emits a deep red glow, but the areas around the nebula with fewer stars are filled with dust, which reflects nearby starlight to produce the pale blue glow at the nebula's apparent edges.

Shot at 1600mm with a 200mm RC telescope and a ZWO ASI533MM Pro. 2h of Ha integrated exposure time, plus 1h each of RGB data.

All images on my blog, unless noted, are shot from my backyard in Bortle 7 skies.

[mindblowingscience]

The sun warms the Earth, making it habitable for people and animals. But that's not all it does, and it affects a much larger area of space. The heliosphere, the area of space influenced by the sun, is over a hundred times larger than the distance from the sun to the Earth. The sun is a star that constantly emits a steady stream of plasma—highly energized ionized gas—called the solar wind. In addition to the constant solar wind, the sun also occasionally releases eruptions of plasma called coronal mass ejections, which can contribute to the aurora, and bursts of light and energy, called flares. The plasma coming off the sun expands through space, along with the sun's magnetic field. Together they form the heliosphere within the surrounding local interstellar medium—the plasma, neutral particles and dust that fill the space between stars and their respective astrospheres. Heliophysicists like me want to understand the heliosphere and how it interacts with the interstellar medium.

Continue Reading.

[brightestofcentaurus]

Orion Nebula

"The dusty side of the Sword of Orion is illuminated in this striking infrared image from the European Space Agency's Hershel Space Observatory. This immense nebula is the closest large region of star formation, situated about 1,500 light years away in the constellation of Orion. The parts that are easily observed in visible light, known alternatively as the Orion Nebula or Messier 42, correspond to the light blue regions. This is the glow from the warmest dust, illuminated by clusters of hot stars that have only recently been born in this chaotic region.

The red spine of material running from corner to corner reveals colder, denser filaments of dust and gas that are scattered throughout the Orion nebula. In visible light this would be a dark, opaque feature, hiding the reservoir of material from which stars have recently formed and will continue to form in the future.

Herschel data from the PACS instrument observations, at wavelengths of 100 and 160 microns, is displayed in blue and green, respectively, while SPIRE 250-micron data is shown in red.

Within the inset image, the emission from ionized carbon atoms (C+), overlaid in yellow, was isolated and mapped out from spectrographic data obtained by the HIFI instrument."

Image and information from NASA.

[thepastisalreadywritten]

The Year’s Most Spectacular Photos from the James Webb Telescope

By Jeffrey Kluger

December 22, 2023

Close to 1,500 light years from Earth lie a pair of baby stellar twins known as Herbig-Haro 46/47 — which are barely a few thousand years old.

A star the size of our sun, by contrast, takes an average of 50 million years to reach even the stellar equivalent of young adulthood It's Herbig-Haro 46/47's extreme youth that gives the formation more of a blob-like appearance than the stellar duo it is.

Young stars are buried in clouds of dust and gas, which they absorb as they grow. Sometimes, however the infant stars ingest too much material too fast.

When that happens, dust and gas erupts from both sides of the formation, giving the young pair their misshapen look.

But if you have patience — 50 million years worth of patience — what is a blob today will be stars tomorrow.

NASA, ESA, CSA. Image Processing: Joseph DePasquale (STScI)

A pair of brilliant stellar nurseries located 1,600 light years from Earth, the Orion Nebula and Trapezium Cluster are home to a relative handful of very young but very bright stars.

Four of the stars are easy to see with a simple, amateur, four-inch telescope.

One of the four — the beast of the young litter — is especially visible, a full 20,000 times brighter than our sun.

Apart from their four main stars, the Orion Nebula and Trapezium cluster contain approximately 700 additional young stars at various stages of gestation.

NASA, ESA, CSA/Science leads and image processing: M. McCaughrean, S. Pearson, CC BY-SA 3.0 IGO

(L): It’s not easy being a Wolf-Rayet star, like this specimen imaged by the Webb telescope at a distance of 15,000 light years.

A rare species of stellar beast — NASA estimates there are only 220 of them in a Milky Way galaxy with at least 100 billion stars — the Wolf-Rayet burns hot and burns fast, with temperatures 20 to 40 times the surface of the sun.

All of that rapidly expended energy causes the star to lose its hydrogen envelope quickly and expose its helium core.

The result: a very early and very violent death.

A star like our sun burns for about 10 billion years. As for a Wolf-Rayet? Just a few hundred thousand before it dissolves into cosmic dust.

NASA, ESA, CSA, STScI, Webb ERO Production Team

(R): If the Wolf-Rayet star dies an ugly and violent death, the celebrated Ring Nebula, photographed by the Webb at a distance of 2,000 light years from Earth, has been expiring beautifully.

The glowing remains of a sun-like star, the nebula was discovered in 1779 by the French astronomer Antoine Darquier de Pellepoix.

As the nebula throws off its outer layers of ionized gas, it reveals its characteristic blue interior, composed of hydrogen and oxygen that have not yet been expelled off by the nebula’s stellar wind.

ESA/Webb, NASA, CSA, M. Barlow (University College London), N. Cox (ACRI-ST), R. Wesson (Cardiff University)

Dwarf galaxy NGC 6822 lives up to to its name — home to just 10 million stars, compared to the minimum of 100 billion in the Milky Way.

But what NGC 6822 lacks in numbers, it makes up in spectacle — which the keen eye of the Webb telescope has revealed.

Discovered in 1884 by American astronomer E.E Barnard, NGC 6822, is now known to have a prodigious dust tail measuring 200 light years across..

What's more, it's home to a dense flock of stars that glow 100,000 times brighter than our sun.

ESA/Webb, NASA & CSA, M. Meixnev

Spiral galaxies are often defined by uneven — and even ragged — arms.

But not galaxy M51, which lies 27 million light years from Earth and is defined by the tautness of its arms and the compactness of its structure.

M51 isn't alone in space. Nearby lies the companion galaxy NGC 5195.

The two galaxies are engaged in something of a gravitational tug of war — one that the NGC 5195 is winning.

NGC's constant gravitational pull is thought to account for both the tightly woven structure of M51's arms and for tidal forces that are thought lead to the creation of new stars in the arms.

ESA/Webb, NASA & CSA, A. Adamo (Stockholm University) and the FEAST JWST team

Just below Orion’s belt lies one of the most celebrated objects in the night sky: the Orion Nebula, a stellar nursery that is home to about 700 young stars.

This Webb image focuses not on the entirety of the nebula but on a structure in the lower left-hand quadrant known as the Orion Bar.

So named because of its diagonal, ridge-like appearance, the bar is shaped by the powerful radiation of the hot, young stars surrounding it.

ESA/Webb, NASA, CSA, M. Zamani (ESA/Webb), and the PDRs4All ERS Team

A baby by stellar standards, the IC 348 Star cluster is just five million years old and located about 1,000 light years from Earth.

Composed of an estimated 700 stars, IC 348 has a structure similar to wispy curtains, created by dust that reflects the light of the stars.

The conspicuous loop in the right hand side of the image is likely created by the gusting of solar winds blowing in the direction that, from Earth, would be west to east.

NASA, ESA, CSA, STScI, Kevin Luhman (PSU), Catarina Alves de Oliveira (ESA)

When it comes to galaxies, there's big and then there's huge and by any measure, Pandora's Cluster — more formally, known as Abell 2744 — qualifies as the latter.

Not just a galaxy, and not even a cluster of galaxies, Abell 2744 is a cluster of four clusters, which long ago collided with one another.

Located 3.5 billion light years from Earth, Pandora's Cluster measures a staggering 350 million years across.

The cluster's massive collective gravity allows astronomers to use it as a gravitational lens, bending and magnifying the light of foreground objects, making them easier to study.

NASA, ESA, CSA, I. Labbe (Swinburne University of Technology) and R. Bezanson (University of Pittsburgh). Image processing: Alyssa Pagan (STScI)

Webb was built principally to look at the oldest and most distant objects in the universe, some of 13.4 billion light years away.

But doesn't prevent the telescope from peering into its own back yard.

This image of Saturn and some of its 146 moons, rivals the images obtained by the Pioneer and Voyager probes.

NASA, ESA, CSA, STScI, Matt Tiscareno (SETI Institute), Matt Hedman (University of Idaho), Maryame El Moutamid (Cornell University), Mark Showalter (SETI Institute), Leigh Fletcher (University of Leicester), Heidi Hammel (AURA). Image processing: J. DePasquale (STScI)

Infant stars are born all over the universe, but the closest stellar birthing suite to Earth is the Rho Ophiuchi cloud complex, located just 460 light years distant.

A turbulent — even violent — place, Rho Ophiuchi is defined by jets of gas roaring from young stars.

Most of the stars in this comparatively modest nursery are more or less the size of the sun.

But one, known as S1, is far bigger — so much so that it is self-immolating, carving a great cavity around itself with its stellar wind, the storm of charged particle's all stars emit, though few with the gale-force power of S1.

NASA, ESA, CSA, STScI, Klaus Pontoppidan (STScI)

[thespacewirednews]

Eye see you… 👁

Back in 1996, Nasa Hubble revealed the hourglass shape of this young planetary nebula located about 8,000 light-years away. In previous images taken from the ground, the nebula looked like a pair of large outer rings with a smaller central one, but the finer details could not be seen.

Planetary nebulae are created by the death of Sun-like stars: the star collapses to form a dense and hot white dwarf star. At the same time, the dying star throws off its outer layers of material, forming an elaborate cloud of gas and dust known as a planetary nebula. This isn’t an uncommon phenomenon, and yet, this “eye” star is a little unique: it should be at the center of the nebula, but it’s off center.

Hubble also revealed other new and unexpected features in the nebula. For example, there is a pair of intersecting elliptical rings in the central region, which appear to be the rims of a smaller hourglass. There are also the intricate patterns of the etchings on the hourglass walls. There are a few possible explanations for the arc-like etchings – for instance, they could be the remnants of shells ejected from the star when it was younger.

This picture was composed of three separate images taken by Hubble’s Wide Field and Planetary Camera 2 in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly ionized oxygen (blue).

Image description: This nebula has an interesting appearance: what looks like a turquoise blue eye stares right at you from the center of a red-orange hourglass-like shape made from two interlocking circles – like a Venn diagram turned on its side. The circles each have arcs within them. The darkness of space forms the backdrop of this image.

Credit: NASA/JPL-Caltech/ESA, the Hubble Heritage Team STScI/AURA

[rwby-soh]

“Wild Oat”

Sex: Female

Race: Human

Height: 5’7”

Age (circa 99 AGW): 18

Aura Density: Low

Aura Reserves: Below Average

Aura Color: Violet

Semblance: Retrocognition

Weapon: Morgan

Jacques Gele's youngest daughter. The oldest among the four Schnee family soap opera girls at Beacon and the leader of team BGEL. She puts up a bitchy and arrogant front in order to cover up her various insecurities, such as the loneliness she feels from how most of her extended family doesn’t want anything to do with her, the sense of abandonment she feels over her parents leaving her with a family friend to actually raise her, the fact that she’s a bastard child, how she feels useless because her Semblance (Retrocognition - the ability to read people’s memories by touching them) has next-to-no practical use in combat, or how she’s the weakest member of her team in both skill and strength. Belka’s weapon is a laser rifle-naginata combo named Morgan that can use specialized, exuberantly expensive Dust cores fuel and modify the attributes of the beams it shoots (such as using an ice dust core to create freeze rays, or a lighting dust core to ionize the beam). She’s unfortunately bullied by the hands of team SLVR, especially Alaska. Belka’s name and weapon of choice are references to the Belkan Federation and the Belkan War from Ace Combat.

[spacevoyagerx]

Cat’s Eye Nebula

The Cat's Eye Nebula, also known as NGC 6543, is one of the most well-known planetary nebulae located in the constellation Draco.

It is approximately 3,000 light-years away from Earth and is notable for its intricate structure and vibrant colors.

The Cat's Eye Nebula is formed from the outer layers of a dying star that has shed its material during the late stages of its evolution.

The central star, which is a hot white dwarf, is responsible for the intense ultraviolet radiation that ionizes the surrounding gas, causing it to glow.

One of the most striking features of the Cat's Eye Nebula is its "eyes," which are formed by the concentric shells of gas and dust that create a visually captivating appearance.

Credits: NASA, ESA, HEIC, and the Hubble Heritage Team (STScI/AURA) Acknowledgment: R. Corradi (Isaac Newton Group of Telescopes, Spain) and Z. Tsvetanov (NASA)

[apod]

2024 November 25

The Horsehead Nebula Image Credit & Copyright: Alex Lin (Chilescope)

Explanation: One of the most identifiable nebulas in the sky, the Horsehead Nebula in Orion, is part of a large, dark, molecular cloud. Also known as Barnard 33, the unusual shape was first discovered on a photographic plate in the late 1800s. The red glow originates from hydrogen gas predominantly behind the nebula, ionized by the nearby bright star Sigma Orionis. The darkness of the Horsehead is caused mostly by thick dust, although the lower part of the Horsehead's neck casts a shadow to the left. Streams of gas leaving the nebula are funneled by a strong magnetic field. Bright spots in the Horsehead Nebula's base are young stars just in the process of forming. Light takes about 1,500 years to reach us from the Horsehead Nebula. The featured image was taken from the Chilescope Observatory in the mountains of Chile.

∞ Source: apod.nasa.gov/apod/ap241125.html

[thefirststarr]

SPACEMAS DAY 11 ✨🪐🌎☄️☀️🌕

Ridges of glowing interstellar gas and dark dust clouds inhabit the turbulent Lagoon Nebula. Also known as M8, The bright star forming region is about 5,000 light-years away. It makes for a popular stop on telescopic tours of the constellation Sagittarius which lies toward the center of our Milky Way Galaxy. It is dominated by the red emission of ionized hydrogen atoms that are recombining with stripped electrons. This view of the Lagoon's central region reaches about 40 light-years across. The bright hourglass shape near the center of the frame is gas ionized by radiation and extreme stellar winds from a massive young star.

Image Credit: Josep Drudis

[quiltofstars]

De Mairan's Nebula, M43 // Seokhee Kim

No, this is not necessarily a repeat! Instead of on the beautiful Orion Nebula, focus your attention at the small star-forming region in the top left of the image. That is De Mairan's Nebula, separated from the larger Orion Nebula by just a dark dust lane.

Discovered by Jean-Jacques d'Ortous de Mairan (1678-1771) some time before 1731, this star-forming region is ionized by a single star system, which you can see in the image! The main star is about 1,300 light years away, and is radiating over 26,000 times the Sun's luminosity. It's unknown why Messier considered this star-forming region to be separate from Orion, but the earlier discovery which Messier knew about likely helped.