本站提供正體中文版。切換到正體中文本站提供简体中文版。切换到简体中文このサイトには日本語版があります。日本語で表示이 사이트는 한국어로도 제공됩니다.한국어로 보기Diese Website ist auch auf Deutsch verfügbar.Auf Deutsch ansehenEste sitio web también está disponible en español.Ver en españolQuesto sito è disponibile anche in italiano.Visualizza in italianoCe site est également disponible en français.Afficher en françaisEste site também está disponível em português.Ver em portuguêsDeze website is ook beschikbaar in het Nederlands.In het Nederlands bekijkenЭтот сайт также доступен на русском языке.Смотреть на русскомयह वेबसाइट हिन्दी में भी उपलब्ध है।हिन्दी में देखेंهذا الموقع متاح أيضًا باللغة العربية.عرض بالعربيةSitus ini juga tersedia dalam bahasa Indonesia.Lihat dalam bahasa IndonesiaBu site Türkçe olarak da mevcut.Türkçe görüntüleTa strona jest dostępna także po polsku.Wyświetl po polskuTrang web này cũng có phiên bản tiếng Việt.Xem bằng tiếng Việtاین وب‌سایت به فارسی هم در دسترس است.مشاهده به فارسی
NGC 1333 Embryo Nebula

NGC 1333 Embryo Nebula

2025
Type
Nebula
Acquisition
Sharpstar 13028HNT · ToupTek ATR2600M
Integration
32h

NGC 1333, also known as the Embryo Nebula, is a reflection nebula located in the constellation Perseus, approximately 1,000 light-years from Earth. Situated in the western part of the Perseus molecular cloud, it is an active star-forming region containing a large number of newborn stars less than one million years old. The star formation activity within NGC 1333 is highly dynamic, featuring numerous Herbig-Haro objects—emission regions formed by the interaction of high-velocity gas ejected from young stars with the surrounding material. Additionally, the region hosts many brown dwarfs and planetary-mass objects, highlighting the nebula’s diversity and complexity.

LDN 1448 (Lynds Dark Nebula 1448) is a dark nebula in the constellation Perseus, located adjacent to NGC 1333. This nebula also exhibits active star formation, containing multiple young stars and molecular outflows. Research indicates that the young stars within LDN 1448 eject high-velocity molecular gas, forming distinct molecular outflow structures. These outflows have been clearly detected in near-infrared observations at the H₂ 2.12-micron wavelength.

Sharpstar13028HNT
ToupTek2600MM
Sky-WatcherAZ-EQ6 GT
Antlia 36mm Lx144, RGBx80, 300sec
Location: Liaoning, China