#umcp

[of-stars-and-dust]

Astronomy Picture of the Day

2025 January 22

The North America Nebula

A star field is dominated by a red and blue glowing nebula. This nebula appears, to some, to have the shape of North America and so is called the North America Nebula.

Image Credit & Copyright: Dimitris Valianos

The North America nebula on the sky can do what the North America continent on Earth cannot -- form stars. Specifically, in analogy to the Earth-confined continent, the bright part that appears as the east coast is actually a hot bed of gas, dust, and newly formed stars known as the Cygnus Wall. The featured image shows the star forming wall lit and eroded by bright young stars and partly hidden by the dark dust they have created. The part of the North America nebula (NGC 7000) shown spans about 50 light years and lies about 1,500 light years away toward the constellation of the Swan (Cygnus).

Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)

NASA Official: Amber Straughn

A service of: ASD at NASA / GSFC,

NASA Science Activation

& Michigan Tech. U.

[starstrucktoby]

Swift’s UV Portrait of the Andromeda Galaxy

NASA's Neil Gehrels Swift Observatory viewed the spiral galaxy Andromeda. (Also called M31, in Ultraviolet light). The image is composed of 330 images from Swift's Ultraviolet Optical Telescope. 20,000 ultraviolet sources are visible in the photo, including M32, which is a small galaxy in orbit around M31.

Image Credits: NASA/Swift/Stefan Immler (GSFC) and Erin Grand (UMCP)

[world-beauty]

The Arms of NGC 4258

Credits: UMCP, et al., NASA, CXC, DSS, NASA, JPL-Caltech, NRAO, AUI, NSF

[discovercosmos]

2024 May 17

Aurora Banks Peninsula

Image Credit & Copyright: Kavan Chay

Explanation: This well-composed composite panoramic view looks due south from Banks Peninsula near Christchurch on New Zealand's South Island. The base of a tower-like rocky sea stack is awash in the foreground, with stars of the Southern Cross at the top of the frame and planet Earth's south celestial pole near center. Still, captured on May 11, vibrant aurora australis dominate the starry southern sea and skyscape. The shimmering southern lights were part of extensive auroral displays that entertained skywatchers in northern and southern hemispheres around planet Earth, caused by intense geomagnetic storms. The extreme spaceweather was triggered by the impact of coronal mass ejections launched from powerful solar active region AR 3664.

Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)

[getupmychain]

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[of-stars-and-dust]

Astronomy Picture of the Day

2025 March 9

Cyclones at Jupiter's North Pole

The image shows the north pole of Jupiter in red (infrared) light. Many cyclonic swirls surround the pole.

Image Credit: NASA, JPL-Caltech, SwRI, ASI, INAF, JIRAM

Why are there so many cyclones around the north pole of Jupiter? The topic is still being researched. NASA's robotic Juno mission orbiting Jupiter took data in 2018 that was used to construct this stunning view of the curious cyclones at Jupiter's north pole. Measuring the thermal emission from Jovian cloud tops, the infrared observations are not restricted to the hemisphere illuminated by sunlight. They reveal eight cyclonic features that surround a cyclone about 4,000 kilometers in diameter, just offset from the giant planet's geographic north pole. Similar data show a cyclone at the Jovian south pole with five circumpolar cyclones. The south pole cyclones are slightly larger than their northern cousins. Oddly, data from the once Saturn-orbiting Cassini mission has shown that Saturn's north and south poles each have only a single cyclonic storm system.

Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)

NASA Official: Amber Straughn

A service of: ASD at NASA / GSFC,

NASA Science Activation

& Michigan Tech. U.

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[world-beauty]

The Arms of NGC 4258

Credits: UMCP, et al., NASA, CXC, DSS, NASA, JPL-Caltech, NRAO, AUI, NSF

[discovercosmos]

2024 May 21

CG4: The Globule and the Galaxy

Image Credit: CTIO, NOIRLab, DOE, NSF, AURA; Processing: T. A. Rector (U. Alaska Anchorage/NSF’s NOIRLab), D. de Martin & M. Zamani (NSF’s NOIRLab)

Explanation: Can a gas cloud eat a galaxy? It's not even close. The "claw" of this odd looking "creature" in the featured photo is a gas cloud known as a cometary globule. This globule, however, has ruptured. Cometary globules are typically characterized by dusty heads and elongated tails. These features cause cometary globules to have visual similarities to comets, but in reality they are very much different. Globules are frequently the birthplaces of stars, and many show very young stars in their heads. The reason for the rupture in the head of this object is not yet known. The galaxy to the left of the globule is huge, very far in the distance, and only placed near CG4 by chance superposition.

Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)

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[heliocoseno]

Caros Leitores;

Crédito da imagem: WISE , IRSA , NASA ; Processamento e direitos autorais : Francesco Antonucci Explicaç��o: Este é realmente o famoso aglomerado estelar das Plêiades? Conhecido por suas icônicas estrelas azuis , as Plêiades são mostradas aqui em luz infravermelha, onde a poeira ao redor ofusca as estrelas. Aqui, três cores infravermelhas foram mapeadas em cores visuais (R=24, G=12, B=4,6 mícrons ). As imagens de base foram tiradas pela nave espacial Wide Field Infrared Survey Explorer (WISE) da NASA. Catalogado como M45 e apelidado de Sete Irmãs , o aglomerado estelar das Plêiades está por acaso situado em uma nuvem de poeira passageira . A luz e o vento das estrelas massivas das Plêiades repelem preferencialmente partículas menores de poeira , fazendo com que a poeira se estratifique em filamentos , como visto. A imagem em destaque abrange cerca de 20 anos-luz à distância das Plêiades , que fica a cerca de 450 anos-luz de distância em direção à constelação do Touro ( Touro ). 

< | Arquivo | Submissões | Índice | Pesquisa | Calendário | RSS | Educação | Sobre APOD | Discutir | >

Autores e editores: Robert Nemiroff ( MTU ) e Jerry Bonnell ( UMCP 

Oficial da NASA: Amber Straughn Direitos específicos se aplicam . Privacidade , acessibilidade e avisos da NASA Web ; Um serviço de: ASD na NASA / GSFC , NASA Science Activation e Michigan Tech. U.

Para saber mais, acesse o link>

Fonte: NASA /  Publicação 29/09/2024

Obrigado pela sua visita e volte sempre!

Web Science Academy; Hélio R.M.Cabral (Economista, Escritor e Divulgador de conteúdos da Astronomia, Astrofísica, Astrobiologia e Climatologia).Participou do curso (EAD) de Astrofísica, concluído em 2020, pela Universidade Federal de Santa Catarina (UFSC).

Autor do livro: “Conhecendo o Sol e outras Estrelas” e "Conhecendo a Energia produzida no Sol".

Acompanha e divulga os conteúdos científicos da NASA (National Aeronautics and Space Administration), ESA (European Space Agency) e outras organizações científicas e tecnológicas.

Participa do projeto S`Cool Ground Observation (Observações de Nuvens) que é integrado ao Projeto CERES (Clouds and Earth´s Radiant Energy System) administrado pela NASA. A partir de 2019, tornou-se membro da Sociedade Astronômica Brasileira (SAB), como astrônomo amador.

Participa também do projeto The Globe Program / NASA Globe Cloud, um Programa de Ciência e Educação Worldwide, que também tem o objetivo de monitorar o Clima em toda a Terra. Este projeto é patrocinado pela NASA e National Science Fundation (NSF), e apoiado pela National Oceanic and Atmospheric Administration (NOAA) e U.S Department of State.

>Autor de cinco livros, que estão sendo vendidos nas livrarias Amazon, Book Mundo e outras.

Acesse abaxo, os links das Livrarias>

Site: https://www.orionbook.com.br/e-mail: heliocabral@coseno.com.brPage: http://pesqciencias.blogspot.com.br Page: http://livroseducacionais.blogspot.com.br