Sobre Megrez
Descrição
Megrez, Delta Ursae Majoris, is an A-type main-sequence star about 80 light-years away and the faintest of the seven stars of the Big Dipper. It marks the junction where the Dipper's "handle" meets its "bowl." Megrez is about 1.6 times the Sun's mass, twice the radius, and 14 times the luminosity. It is also a suspected debris-disk star, with mid-infrared excess suggesting a surrounding ring of dust.
Dicas de Observação
Megrez's relative faintness (magnitude 3.31) is a classic sky-quality check — if you can see Megrez clearly with the naked eye, you have a reasonably dark site. From light-polluted suburban skies, the Big Dipper looks "incomplete" because Megrez disappears first. Use a pair of binoculars to confirm its white color and position at the corner of the Dipper's bowl, at the base of the handle. Circumpolar from all of the northern hemisphere.
História
The name Megrez comes from the Arabic "al-maghriz," meaning "the root of the tail" — referring to the tail-root of the great bear. All seven Dipper stars carry Arabic-derived names. Megrez's relatively modest brightness puzzled pre-modern astronomers; some ancient records refer to it being "fainter than expected," possibly due to observer uncertainty about the star's real appearance.
Curiosidades
Megrez is part of the Ursa Major Moving Group, a loose cluster of stars that share a common origin and are drifting through the galaxy together — including most of the other Big Dipper stars (all except Dubhe and Alkaid). The group is about 300 million years old. Megrez is one of the youngest prominent stars in the northern sky; on cosmic timescales it will remain a normal hydrogen-fusing dwarf for another billion years.
Observar
1Propriedades Físicas
2Posição e Identificadores
3Facilidade de observação
| Equipamento | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| Olho nu Olho nu | Fácil | Fácil | Médio+ |
| Buscador 50 mm Buscador 50mm | Fácil | Fácil | Fácil |
| Telescópio 150 mm 150mm telesc. | Fácil | Fácil | Fácil |
Bortle 3 = rural · 4 = suburbano · 5 = urbano
4Visibilidade
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5Imagem de Levantamento
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Explorar
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Comparação de Tamanho
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Comparar Estrelas
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Classificação Espectral
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Diagrama Hertzsprung-Russell
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Ciclo de vida estelar
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Espectro de corpo negro
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Espectro de absorção estelar
Espectro de absorção simulado com base no tipo espectral. Passe o mouse sobre as linhas para identificar os elementos.
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Fusão Estelar
Descobrir
15Notas Estelares
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Máquina do tempo da luz
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Viagem Relativística
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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Conhecimento, ferramentas e histórias relacionadas — sem precisar planejar observação.