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Mint Machine #23786

Introducing World App, the first wallet for the Worldcoin ecosystem.

It’s designed by TFH to be simple, and you can use it to authenticate with World ID to prove you’re a real person, get your Worldcoin tokens and send digital money anywhere.

We're excited to celebrate this milestone with the Worldcoin community.

world.app

Introducing World App 26039

dYdX

This !fundrop pass is a non-transferable NFT that allows the holder to participate in !fundrop and get !fun rewards for minting NFTs. Mint your own !fundrop pass at https://mint.fun/fundrop.

!fundrop pass

Ethereum, Evolved: Shanghai is a collection of two art NFTs celebrating the Shanghai/Capella upgrade, a technological milestone on the Ethereum roadmap that will simultaneously upgrade the blockchain’s execution and consensus layers to enable staked ETH withdrawals. The open edition depicts the theme of decentralization, a benefit of the Shanghai/Capella upgrade. By encouraging participation of larger numbers of validators, the Shanghai/Capella upgrade improves the network’s security by increasing decentralization.

Shanghai: Open Edition

To Ethereum, with Love

An exclusive drop to celebrate the launch of 'Subscribe to Mint.' Mirror's new feature built on thirdweb

thirdweb x Mirror | Subscribe to Mint

This Party Card represents your contribution of 0.010 ETH to the Kui-Doodles-18 crowdfund. When the crowdfund concludes, you can use this Party Card to claim your ETH or activate your membership in the Party. During the crowdfund, Party Cards are non-transferable. Head to https://partybid.app/join/0x03659512ee808f16ad889fe05e26d3ffe77effcd to see more.

0.010 ETH Contribution

Aztec

The first NFT drop for the Mirror community.

Mirror Genesis

The Egg is not just an ordinary Egg! Join Eggi NFT, and become the first of its prestigious elite club of owners. 
Eggi is a collection of eggs growing in the beginning of metaverse - a generative collection of unlimited supply of Eggs that live on the Ethereum Blockchain. 
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↳imagination_creation
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❍ 001

'I don't listen to what art critics say. I don't know anybody who needs a critic to find out what art is.' 1111 collection inspired by Jean-Michel Basquiat.

Introducing Safe{Core}

Build the future of account abstraction at https://core.safe.global

Thousands of galaxies flood this near-infrared image of galaxy cluster SMACS 0723. High-resolution imaging from NASA’s James Webb Space Telescope combined with a natural effect known as gravitational lensing made this finely detailed image possible.

First, focus on the galaxies responsible for the lensing: the bright white elliptical galaxy at the center of the image and smaller white galaxies throughout the image. Bound together by gravity in a galaxy cluster, they are bending the light from galaxies that appear in the vast distances behind them. The combined mass of the galaxies and dark matter act as a cosmic telescope, creating magnified, contorted, and sometimes mirrored images of individual galaxies.

Clear examples of mirroring are found in the prominent orange arcs to the left and right of the brightest cluster galaxy. These are lensed galaxies – each individual galaxy is shown twice in one arc. Webb’s image has fully revealed their bright cores, which are filled with stars, along with orange star clusters along their edges.

Not all galaxies in this field are mirrored – some are stretched. Others appear scattered by interactions with other galaxies, leaving trails of stars behind them.

Webb has refined the level of detail we can observe throughout this field. Very diffuse galaxies appear like collections of loosely bound dandelion seeds aloft in a breeze. Individual “pods” of star formation practically bloom within some of the most distant galaxies – the clearest, most detailed views of star clusters in the early universe so far.

One galaxy speckled with star clusters appears near the bottom end of the bright central star’s vertical diffraction spike – just to the right of a long orange arc. The long, thin ladybug-like galaxy is flecked with pockets of star formation. Draw a line between its “wings” to roughly match up its star clusters, mirrored top to bottom. Because this galaxy is so magnified and its individual star clusters are so crisp, researchers will be able to study it in exquisite detail, which wasn’t previously possible for galaxies this distant.

The galaxies in this scene that are farthest away – the tiniest galaxies that are located well behind the cluster – look nothing like the spiral and elliptical galaxies observed in the local universe. They are much clumpier and more irregular. Webb’s highly detailed image may help researchers measure the ages and masses of star clusters within these distant galaxies. This might lead to more accurate models of galaxies that existed at cosmic “spring,” when galaxies were sprouting tiny “buds” of new growth, actively interacting and merging, and had yet to develop into larger spirals. Ultimately, Webb’s upcoming observations will help astronomers better understand how galaxies form and grow in the early universe.

NIRCam was built by a team at the University of Arizona and Lockheed Martin’s Advanced Technology Center.

For a full array of Webb’s first images and spectra, including downloadable files, please visit: https://webbtelescope.org/news/first-images 

Credits:
IMAGE: NASA, ESA, CSA, STScI

On-chain proof of knowledge gained and skills acquired on RabbitHole

What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA’s James Webb Space Telescope, this image reveals previously obscured areas of star birth.

Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The high-energy radiation from these stars is sculpting the nebula’s wall by slowly eroding it away.  

NIRCam – with its crisp resolution and unparalleled sensitivity – unveils hundreds of previously hidden stars, and even numerous background galaxies. Several prominent features in this image are described below.

-- The “steam” that appears to rise from the celestial “mountains” is actually hot, ionized gas and hot dust streaming away from the nebula due to intense, ultraviolet radiation. 

-- Dramatic pillars rise above the glowing wall of gas, resisting the blistering ultraviolet radiation from the young stars.

-- Bubbles and cavities are being blown by the intense radiation and stellar winds of newborn stars.

-- Protostellar jets and outflows, which appear in gold, shoot from dust-enshrouded, nascent stars.

-- A “blow-out” erupts at the top-center of the ridge, spewing gas and dust into the interstellar medium. 

-- An unusual “arch” appears, looking like a bent-over cylinder.

This period of very early star formation is difficult to capture because, for an individual star, it lasts only about 50,000 to 100,000 years – but Webb’s extreme sensitivity and exquisite spatial resolution have chronicled this rare event.

Located roughly 7,600 light-years away, NGC 3324 was first catalogued by James Dunlop in 1826. Visible from the Southern Hemisphere, it is located at the northwest corner of the Carina Nebula (NGC 3372), which resides in the constellation Carina. The Carina Nebula is home to the Keyhole Nebula and the active, unstable supergiant star called Eta Carinae. 

NIRCam was built by a team at the University of Arizona and Lockheed Martin’s Advanced Technology Center.

For a full array of Webb’s first images and spectra, including downloadable files, please visit: https://webbtelescope.org/news/first-images 

Credits:
IMAGE: NASA, ESA, CSA, STScI

We do a little CC0 enjoying

Shout out tjo for the inspo 🫡

A free to mint NFT for the first subscribers of UFO. Minting closes after 72 hours.

The Coinage Subscriber NFT is Coinage’s entry-level tier. The Subscriber NFT unlocks the ability to watch Coinage videos early and ad-free, and it lets you weigh in on what we cover, which guests we talk to, and more. It also opens priority access to future drops. Join the community now, or sign up for our upcoming drop at [coinage.media](https://www.coinage.media).

We've launched a new integration between Paragraph and Highlight, enabling native Highlight embeds directly in Paragraph posts & newsletters.

Writing has come a long way.

A vibrant and dynamic on-chain social networking experience for Syndicate’s earliest community members


The official NFT of We Do A Little Season 0

This NFT grants access to a private WDAL discord channel where the Season 0 episodes will be released early in both audio and video format

Please read the terms of this NFT here: https://arweave.net/j325x0ugFCRf7zF8Sd-e9YoORrgZ3iaevhtUEpZrVKc

Yats 🖖 are emoji usernames that become your universal Internet identity 🗿, website URL 💻, payment address 🤑, and more. By owning a Yat – let’s say 💾📱💻📡 – it’s yours forever. Get inspired and join our amazingly creative Yat Community at Y.at.

083010.eth

$87.03

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