Best Dorado
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30 Doradus, commonly called the Tarantula Nebula, is a vast ionized-hydrogen region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It contains the dense central cluster R136, whose massive young stars supply much of the radiation that illuminates the surrounding gas. The nebula...
The Cosmic Reef is a nickname for a pair of nebulae, NGC 2014 and NGC 2020, located in the Large Magellanic Cloud. This star-forming region was featured in a highly detailed composite image released to celebrate the 30th anniversary of the Hubble Space Telescope in 2020. NGC 2014 is a massive red ne...
The Tarantula Nebula, formally NGC 2070, is a prominent emission nebula situated in the Large Magellanic Cloud. It’s notable as the most active starburst region within our Local Group of galaxies. This dense cloud is approximately 160,000 light-years distant and exhibits intense star formation, far...
TOI-700 is a red dwarf star of spectral class M located approximately 101 light-years from Earth in the constellation Dorado. The star is host to at least three confirmed exoplanets, discovered by NASA's Transiting Exoplanet Survey Satellite (TESS) mission. TOI-700 d, the outermost planet, orbits wi...
The SN 1987A remnant is a glowing nebula formed by the explosion of a star in the Large Magellanic Cloud. This supernova event, occurring in 1987, created a vast cloud of expanding gas and dust—the most studied supernova remnant to date. It’s notable for its complex structure and provides valuable i...
The N11 Nebula is the Large Magellanic Cloud's second-largest star-forming complex after 30 Doradus and contains several generations of young stars.
30 Doradus C is a superbubble in the Large Magellanic Cloud, inflated by massive stars and supernovae within the larger Tarantula Nebula complex.
The N79 Nebula is a major star-forming complex in the Large Magellanic Cloud, notable for forming massive stars in a relatively unexplored region.
N44 is a superbubble complex in the Large Magellanic Cloud, where winds and supernovae from massive stars have carved a vast cavity in the gas.
The Dragon's Head Nebula, NGC 2035, is an emission nebula in the Large Magellanic Cloud, sculpted by winds from young massive stars.
Gamma Doradus is a white-yellow main-sequence star located in the southern constellation of Dorado. It serves as the prototype for the class of Gamma Doradus variable stars, which exhibit brightness fluctuations caused by non-radial gravity-mode pulsations. These types of stars are typically slightl...
AB Doradus is a young, rapidly rotating K-type main-sequence star in the southern constellation Dorado, roughly 49 light-years from the Sun. Its strong magnetic activity produces prominent starspots, flares, and coronal emission, while its rotation period is much shorter than the Sun's. It is the na...
N70 is a roughly circular superbubble in the Large Magellanic Cloud whose shell was excavated by stellar winds and one or more supernovae.
The brightest supernova remnant in the Large Magellanic Cloud, notable for hosting soft gamma repeater SGR 0526-66 and displaying an asymmetric, filamentary shock shell.
A supernova remnant in the Large Magellanic Cloud and one of its brightest X-ray sources, embedded within the active star-forming complex N63.
