Menu

M47

NGC 2422

산개성단 최고의 관측 대상 (88/100)
M47 OpenCluster Puppis 관측 가능 난이도 2 Small telescope (4") - Wide field preferred
성도 목록에 추가 계획에 추가
카탈로그로 돌아가기

특성

등급 4.4
각크기 19.8′
거리 1600 ly
Open Cluster [Distance: 1600 ly]

위치 & 식별자

RA 07h 36m 36.0s
Dec -14° 30' 00.0"
별자리 Puppis
카탈로그 M47

가시성

사용자 설정에서 관측지를 설정하세요 가시성 데이터를 확인할 수 있습니다.

서베이 이미지

서베이 이미지 로드 중…

M47 소개

설명

M47 is a bright, coarse open cluster in Puppis, about 1,600 light-years from Earth. It contains roughly 50 stars spread across about 12 light-years, with an age of 78 million years. The cluster's brightest members are blue-white B-type stars, and it includes several attractive double stars.

관측 팁

Located about 1 degree west of M46. Visible to the naked eye as a hazy patch about the size of the full Moon. Binoculars show a bright scattering of about 20 stars. A telescope at low power (30-50x) provides the best view, revealing bright stars with nice color contrasts. The pairing with M46 in a wide-field view is one of the finest double-cluster sights in the sky. Best observed from January through April.

역사

Known since antiquity — likely the object recorded by Giovanni Battista Hodierna before 1654. Charles Messier cataloged it in 1771, but with an error in position that caused it to be 'lost' for over a century until identified with NGC 2422 by Oswald Thomas in 1934.

재미있는 사실

M47 was a 'lost' Messier object for over 160 years due to a sign error in Messier's coordinates. The error made the recorded position point to empty sky. Canadian astronomer T.F. Morris confirmed its identity in 1959. M47 and M46 together make a superb visual pair, demonstrating the difference between a nearby bright cluster and a distant rich one.

커뮤니티 사진 (1)

Credit: NOIRLab / NSF / AURA. License: CC BY 4.0. (Wikimedia Commons)

Credit: NOIRLab / NSF / AURA. License: CC BY 4.0. (Wikimedia Commons)

Skybred Feb 28, 2026