xchgre

The Cassini mission to Saturn is one of the most ambitious efforts in planetary space exploration ever mounted. A joint endeavor of NASA, the European Space Agency (ESA) and the Italian space agency, Agenzia Spaziale Italiana (ASI), Cassini is a sophisticated robotic spacecraft orbiting the ringed planet and studying the Saturnian system in detail. Cassini also carried a probe called Huygens, which parachuted to the surface of Saturn's largest moon, Titan, in January 2005 and returned spectacular results. After two decades in space, NASA's Cassini spacecraft is nearing the end of its remarkable journey of exploration. Having expended almost every bit of the rocket propellant it carried to Saturn, operators are deliberately plunging Cassini into the planet to ensure Saturn's moons will remain pristine for future exploration. Author/Origin/License: Brian Kumanchik, NASA/JPL-Caltech, Public Domain 1. See [assembly.jpg] file to see how model parts are assembled.2. Model is designed to fit together without the need for glue, but a small drop at connection points will help to strengthen it.3. Be sure to print 2 copies of the pins.

Cassini

NASA 3D - CC0 Public Domain

I have converted the original design that was in pieces to be able to print it easily with the Bambu and AMS. I have also included the loose parts.In the attached profile the model is scaled to 50%.

Multi Color Kirby

CC BY - Remixes or Re-shares

I have decided to re-upload the famous Christmas Deer for Bambu printers, I know there are other models on the site but they either have unnecessary supports or they are modified. The profile applies a Brim to the model to avoid adhesion problems and scales it to fit perfectly in the printing size of the machine, specifically, the model is 252 mm high. No Supports are required. The Seam is placed on the back of the reindeer, thus imitating a natural touch. <ul><li>The mother/dad Standing: This model</li><li>The mother/dad Laying: <a target="_blank" href="https://makerworld.com/es/models/25559#profileId-119527" rel="nofollow noopener">https://makerworld.com/es/models/25559#profileId-119527</a></li><li>The Fawn: <a target="_blank" href="https://makerworld.com/es/models/111732#profileId-119629" rel="nofollow noopener">https://makerworld.com/es/models/111732#profileId-119629</a> </li></ul>

Holiday Christmas Deer

Cristrmast Deer - Family

No support needed, feel free to upload print profiles. The Free Pirate is a 3D model of a pirate that is in the public domain.

The Free Pirate

Artistic design - CC0

This is part of the collection <a target="_blank" href="https://makerworld.com/es/u/3064039562/collections/176013" rel="nofollow noopener">List of common 3D test models </a> Suzanne is Blender's alternative to more common test models such as the Utah Teapot and the Stanford Bunny. A <a target="_blank" href="https://en.wikipedia.org/wiki/Low_poly" rel="nofollow noopener">low-polygon model</a> with only 500 faces, Suzanne is included in Blender and often used as a quick and easy way to test materials, animations, rigs, textures, and lighting setups. It is as easily added to a scene as primitives such as a cube or plane. The largest Blender contest gives out an award called the Suzanne Award. This "nice" version has the Subdivision Surface Modifier level 3, making it perfect for printing without a lot of triangles. License: GNU GLP 2+ inherited from Blender. This model here is released under CC BY, but the attribution must be given to Blender.

Suzanne - Monkey

Common 3D test models

Eta Carinae is a star system that contains the most luminous star known in our Galaxy. It radiates energy at a rate that is 5 million times that of the Sun. Observations indicate that Eta Carinae is likely a double star system where matter is rapidly boiling off one star's surface.Some astronomers think that the massive star could explode as a supernova as soon as in the next few decades, or perhaps not for another few million years. Whenever this gigantic explosion happens, it would pose no threat to life here on Earth at a distance of about 7,500 light years away, but it would be quite a show. <img src="https://makerworld.bblmw.com/makerworld/draft/317902/2023-12-28_9righmqf2ei2.png">Eta Carinae, Credit: X-ray: NASA/CXC; Ultraviolet/Optical: NASA/STScI; Combined Image: NASA/ESA/N. Smith (University of Arizona), J. Morse (BoldlyGo Institute) and A. PaganBetween 1837 and 1856 it increased dramatically in intensity to become the brightest star in the sky except for Sirius, despite being eight hundred times farther away than that star. Astronomers think this "Great Eruption," as this 19th-century event is called, was caused by internal radiation pressure in the massive star that somehow triggered an instability, or by interaction with its nearby companion star. After the Great Eruption, Eta Carinae faded to become a relatively dim star that could only be seen through a telescope. Since 1940, it has begun to brighten again, becoming visible to the unaided eye.Modern day observations of Eta Carinae have shown that it is, in fact, a double-star system. The smaller companion is not directly visible in images from even today's most powerful telescopes, but variability in X-rays in the regions close to the star signals the companion star's presence. Astronomers don't know exactly what role the companion has played in the evolution of Eta Carinae, or what it will do in the future.Eta Carinae may be an extreme example of a "luminous blue variable" — a critical stage in the evolution of the most massive stars. These gigantic stars can produce intense amounts of radiation that causes violent instabilities before it explodes as a supernova, or even possibly a "hypernova," a type of super-supernova explosion that has been hypothesized to produce gamma-ray bursts.<h3>Eta Carinae in Different Kinds of Light</h3>Images taken in different wavelengths of light reveal different structures, each providing more information about the outbursts of Eta Carinae.<img src="https://makerworld.bblmw.com/makerworld/draft/317902/2023-12-28_fe6t1993nkb3.png"> Credit: X-ray: NASA/CXC/GSFC/K.Hamaguchi, et al.; Optical: NASA/STScI; Near-Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSFX-rays of Eta Carinae from NASA’s Chandra X-ray Observatory give an important glimpse deep into the nebula where the fastest material is being thrown off by Eta Carinae. The outer, horseshoe-shaped ring, which is about two light years in diameter, provides evidence of another large explosion that occurred over a thousand years ago. Chandra's X-ray image reveals a hot inner core about eight times smaller than the outer ring and a hot central source less than a light month in diameter that may contain this mysterious superstar.All three structures seen in X-rays are thought to represent shock waves produced by matter rushing away from the Eta Carinae at supersonic speeds. The temperature of the shock-heated gas ranges from 60 million degrees Celsius in the central regions to 3 million degrees Celsius on the outer edge.Optical data of Eta Carinae taken by NASA's Hubble Space Telescope reveal two spectacular bubbles of gas expanding in opposite directions away from a central bright region at speeds in excess of a million miles per hour. The inner region visible in the Chandra image appears to be associated with a central disk of high velocity gas rushing out at much higher speeds perpendicular to the bipolar nebula visible in the optical image.Infrared images, such as those from 2MASS (above, right) or NASA's Spitzer Space Telescope (below, depicting a larger field of view), show the surrounding nebula, letting us peer through the dust that obscures our view invisible light to reveal the intricate details and extent of the Carina Nebula around this brilliant star.<img src="https://makerworld.bblmw.com/makerworld/draft/317902/2023-12-28_8x361os0l12f.png"> Author/Origin/License: - File: NASA/Caltech/IPAC/R. Hurt & NASA/CXC/SAO/A. Jubett, Public Domain - Photo: NASA/CXC/SAO/N.Wolk, CC BY

NASA 3D - CC0 Public Domain

CC BY - Remixes or Re-shares

Cristrmast Deer - Family

Artistic design - CC0

Common 3D test models

Chandra X-ray Observatory - CC0