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Carina
Latin Name for the Keel constellation, part of the heavenly waters group, visible in the southern hemisphere.
NGC 3324
Open star cluster, ~12 million years old, massive stars concentrated in the center, located northeast of the Carina Nebula.
V1057 Cygni
Binary system with a FU Orionis variable star, still forming, periodic brightening due to accretion, F type, few million years old.
Dorado
Constellation representing the swordfish, located in the southern hemisphere, home to the Tarantula Nebula and Large Magellanic Cloud.
HD 141569
Young main sequence star, isolated Herbig Ae/Be star of spectral class A2Ve, 364 light years away.
Musca
Constellation representing the fly, part of the Johann Bayer family, contains HD 100546, a B8-A0 star in the pre-main sequence stage.
Ophiuchus
Constellation known as the serpent bearer, contains Barnard 68, a molecular cloud, and seven Messier objects.
Barnard 68
Dark molecular cloud, 500 light-years away, important for star formation, discovered by Edward E. Barnard in 1919.
Orion
Constellation discovered by Christiaan Huygens, contains FU Orionis, a pre-main-sequence star with extreme variability.
HOPS 383
Class 0 protostar, 100,000 years old, located about 1,400 light years from Earth, known for having an outburst.
Messier 42
The Orion Nebula, a cloud of dust and gas where new stars are formed, discovered by Christiaan Huygens, 1,344 light years away.
Pegasus
Constellation in the Northern Hemisphere, part of the Perseus family, discovered by Ptolemy, contains Messier 15 and stars with confirmed planets.
Stephan's Quintet
Visual grouping of five galaxies, four forming the first compact galaxy group discovered.
Stephan's Quintet
A group of interacting galaxies that trigger star formation in each other, providing insights into fundamental galactic processes.
NGC 1333
A reflection nebula in Perseus containing young stars less than a million years old, hidden by stardust, offering a glimpse into early stellar evolution.
Hickson Compact Group 92 (HCG 92)
Refers to the four galaxies clumped closely together in Stephan's Quintet, serving as a unique astronomical system for study.
Baby Boom Galaxy
A massive elliptical starburst galaxy undergoing intense star formation, emitting light primarily in the infrared spectrum.
HL Tauri
A T Tauri star in Taurus, representing an early stage in stellar evolution with a mass similar to the Sun, crucial for understanding star formation.
L1527
A class 0 protostar located 460 light-years away, providing a rare example of such objects and aiding in the study of stellar evolution.
NGC 1555
Also known as Hind's Variable Nebula, a variable nebula illuminated by T Tauri, showcasing early stellar evolution and Herbig–Haro objects.
T Tauri
The first young star discovered with a mass similar to the Sun, representing a class of very young stars characterized by erratic brightness changes.
HH 46/47
Herbig–Haro objects located in Vela, offering insights into early star formation processes and emitting light in specific sections of the electromagnetic spectrum.
RCW 38
An HII region in Vela containing a massive star cluster, crucial for studying star formation with O type stars and forming insights into early stellar evolution.
Objects in Volans
Notable deep sky objects in Volans include the Lindsay-Shapley Ring (AM0644-741), the Meathook Galaxy (NGC 2442), the spiral galaxy NGC 2397, and the galaxy cluster SMACS 0723.
Discovery of Volans objects
Discovered in the late 16th century by Pieter Dirkszoon Keyser and Frederick de Houtman.
J122051+491255
A green pea galaxy.
Green pea galaxy
A small, green-blue galaxy with high luminosity due to intense star formation.
Importance of green pea galaxies
They exhibit high rates of star formation.
Spectral uniqueness of green pea galaxies
They have low oxygen levels compared to the Milky Way, making them chemically primitive.
Distance from Earth
Located 170 million light-years away.
Best electromagnetic spectrum for viewing
UV spectrum.
Discovery of green pea galaxies
Discovered in 2009 by volunteers working on Galaxy Zoo.