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Portrait in bust of Jérôme Lalande in 1802
Portrait in bust of Jérôme Lalande in 1802
Combined optical and infrared image of VY CMa. The bright star at the upper right is τ Canis Majoris. (ESO/Digitized Sky Survey 2)
Combined optical and infrared image of VY CMa. The bright star at the upper right is τ Canis Majoris. (ESO/Digitized Sky Survey 2)
VLBA used to derive VY CMa's 2011 distance estimate
VLBA used to derive VY CMa's 2011 distance estimate
(July 2008, outdated). Relative sizes of the planets in the Solar System and several stars, including VY Canis Majoris: 1. Mercury < Mars < Venus < Ea
(July 2008, outdated). Relative sizes of the planets in the Solar System and several stars, including VY Canis Majoris: 1. Mercury < Mars < Venus < Earth 2. Earth < Neptune < Uranus < Saturn < Jupiter 3. Jupiter < Proxima Centauri < Sun < Sirius 4. Sirius < Pollux < Arcturus < Aldebaran 5. Aldebaran < Rigel < Antares < Betelgeuse 6. Betelgeuse < Mu Cephei < VV Cephei A < VY Canis Majoris.
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UGC 5797, an emission-line galaxy where massive bright blue stars are formed
UGC 5797, an emission-line galaxy where massive bright blue stars are formed
Artist's impression of a Y-dwarf
Artist's impression of a Y-dwarf
Image of the carbon star R Sculptoris and its striking spiral structure
Image of the carbon star R Sculptoris and its striking spiral structure
Sirius A and B (a white dwarf of type DA2) resolved by Hubble
Sirius A and B (a white dwarf of type DA2) resolved by Hubble