Tweedledee Cluster — Aglomerado Aberto em Ofiúco
NGC 6633
Sobre Tweedledee Cluster
Descrição
NGC 6633 is a large, bright open cluster in the constellation Ophiuchus, about 1,200 light-years from Earth. Commonly known as the Tweedledee Cluster, it is roughly the size of the full Moon and contains about 30 bright blue stars strewn across a rich Milky Way background — a splendid target for any optical aid from binoculars upward. It forms a famous visual pair with the nearby cluster IC 4756 (sometimes called Tweedledum or Graff's Cluster), which lies just 3 degrees to the east; the two are often framed together in low-power surveys along the summer Milky Way. Both clusters share similar age (~700 million years) though they lie at different distances.
Dicas de Observação
An ideal binocular target. NGC 6633 is visible to the naked eye from dark sites as a small misty patch. In 7x50 or 10x50 binoculars it resolves into a striking elongated chain of bright blue stars scattered across a rich Milky Way field — a textbook 'binocular cluster.' A small telescope at 20-30x frames the cluster beautifully but high magnification dilutes its spread-out character. Pair the view with IC 4756 three degrees east for the full 'Tweedledee/Tweedledum' experience. Best observed from June through September when Ophiuchus is high in the evening.
História
Cataloged in 1702 by the German astronomer Philippe Loys de Chéseaux's predecessor Johannes Hevelius, though William Herschel is more commonly credited with its rediscovery in the 1780s. The cluster appears in most 19th-century observing guides. The 'Tweedledee' nickname — a whimsical pair with IC 4756's 'Tweedledum' — appears to have originated in amateur astronomy literature of the 20th century, a nod to Lewis Carroll's characters. The name is informal but widely recognized in modern observing handbooks.
Curiosidades
NGC 6633 is sometimes called the 'Summer Beehive,' though that informal nickname competes with a few other clusters. It lies almost exactly on the celestial equator, making it equally accessible from both hemispheres. Despite its size and brightness, it is often overlooked by deep-sky observers because it has no official Messier or Caldwell designation — one of the reasons it is a quiet favorite among binocular astronomers who keep their own 'should-have-been-in-Messier' lists.
Observar
1Propriedades
Posição e Identificadores
2Facilidade de observação
| Telescópio | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| Refrator 80 mm Refr. 80mm | Fácil | Fácil | Fácil |
| Newton 150 mm Newt. 150mm | Fácil | Fácil | Fácil |
| Celestron C8 (SCT 203 mm) C8 203mm | Fácil | Fácil | Fácil |
Bortle 3 = rural · 4 = suburbano · 5 = urbano
3Visibilidade
Defina um local nas Configurações do Usuário para ver dados de visibilidade.
4
Vista pela Ocular
Tweedledee Cluster · 12.0′ diâmetro · N cima, L esquerda
5
Melhor Ampliação
6Onde este aglomerado se situa no tempo
Aglomerados abertos abrangem mais de quatro ordens de grandeza em idade — de associações OB recém-nascidas a sobreviventes antigos e ricos em metais.
7
Diagrama cor-magnitude
O diagrama cor-magnitude de um aglomerado revela sua idade: quanto mais azul o ponto de virada onde a sequência principal se curva para as gigantes vermelhas, mais jovem o aglomerado.
Cada ponto é um membro do Gaia-DR3. A cor codifica o tipo espectral; o tamanho reflete a probabilidade de pertença.
Explorar
8
Decodificador de Classificação
Imagem de Levantamento
Carregando imagem de levantamento…
Próximos no céu
Outros alvos a poucos graus — mova um pouco o telescópio e continue explorando.
Os scores de visibilidade assumem um Newton de 150 mm com Bortle 4.
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