NGC 62 is a barred spiral galaxy in the constellation Cetus. NGC 62 is its New General Catalogue designation. It has an apparent magnitude of 13.2. [4]

Near the outskirts of the Small Magellanic Cloud, a satellite galaxy roughly 200 000 light-years from Earth, lies the young star cluster NGC 602, which is featured in this new image from the NASA/ESA/CSA James Webb Space Telescope. This image includes data from Webb’s NIRCam (Near-InfraRed Camera) and MIRI (Mid-InfraRed Instrument).

Steve's Notes ===== NGC 62 17.5" (8/20/88): fairly faint, small, oval WSW-ENE, weak concentration. Located between mag 7.2 SAO 147195 9' WNW and mag 6.5 SAO 147208 13' E.

NGC 602 is a young, bright open cluster of stars located in the Small Magellanic Cloud (SMC), a satellite galaxy to the Milky Way. It was discovered on 1 August 1826 by Scottish astronomer James Dunlop. [6]

2008年3月23日 · Near the outskirts of the Small Magellanic Cloud, a satellite galaxy some 200 thousand light-years distant, lies the young star cluster NGC 602. Surrounded by natal gas and dust, NGC 602 is featured in this Hubble image of the region.

NGC 602 The star cluster NGC 602 as seen by the James Webb Space Telescope. Most of the stars in the cluster are visible just left of center. Partially obscured clouds of gas and dust surround the area, and the background is dotted with galaxies. ESA / Webb, NASA & CSA, P. Zeidler, E. Sabbi, A. Nota, M. Zamani (ESA / Webb)

English: NGC 62 is a spiral galaxy in the constellation Cetus. It is located at RA 00 h 17 m 05.4 s, dec −13° 29′ 15″ ( J2000 ), and has an apparent magnitude of 14.

2024年10月23日 · Near the outskirts of the Small Magellanic Cloud, a satellite galaxy roughly 200 000 light-years from Earth, lies the young star cluster NGC 602, which is featured in this new image from the NASA/ESA/CSA James Webb Space Telescope. This image includes data from Webb’s NIRCam (Near-InfraRed Camera) and MIRI (Mid-InfraRed Instrument).

NGC 62[4][5][6] este o galaxie spirală din constelația Balena. Este localizată la RA 00h 17m 05.4s, dec −13° 29′ 15", și are o magnitudine aparentă de 13,5.

Messier 62 or M62, also known as NGC 6266 or the Flickering Globular Cluster, is a globular cluster of stars in the south [a] of the equatorial constellation of Ophiuchus. It was discovered in 1771 by Charles Messier, [b] then added to his catalogue eight years later. [11] M62 is about 21.5 kly[3] from Earth and 5.5 kly from the Galactic Center ...