LRI4616740: The sibylle of Delphi Detail of a vault of the Sistina Chapel (Sistina) Fresco by Michelangelo Buonarroti called Michel Ange (Michelangelo or Michelangelo, 1475-1564) Michelangelo (Michelangelo or Michelangelo, 1475 - 1564). 1536-1541. Sistine Chapel Wall, Musei Vaticani. Rome Italy, Buonarroti, Michelangelo (1475-1564) / Bridgeman Images
FLO4616888: Young French woman with a little boy, 18th century, by an engraving by Philibert Debucourt (1755-1832) - Lithography after an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1834-1899 67, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images
FLO4616957: Portuguese peasant of the 16th century - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “” Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images
PIX4618377: Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud / Bridgeman Images
PIX4618480: Rosette and Cone Nebulae - The Cone and Rosette region - Large field image of the Cone nebula (centre left) and the Rosette nebula (top right), in the constellation Unicorn. This wide field image shows the rich colorful Cone nebula region (at the center - left of the image) and the Rosette Nebula (at the top right). They are both located in the Monoceros constellation, very close to the better known Orion constellation / Bridgeman Images
PIX4618301: Tarantula Nebula in the Great Magellan Cloud - Tarantula nebula (NGC 2070) in Dorado - NGC 2070, the Tarantula Nebula is a vast star-forming region located north of the Great Magellan Cloud galaxy, in the southern hemisphere about 170,000 years - light from Earth. Image obtained by combining light through different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min). The largest emission nebula in the sky, the Tarantula Nebula (also known as NGC 2070 or 30 Doradus) is located in the Large Magellanic Cloud (LMC) in the southern hemisphere at about 170,000 light year from Earth. Image obtained with different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min) / Bridgeman Images
OMG4618637: The Musee de la Vie Romantique, 16 rue Chaptal in Paris 9e. Private hotel rented by brothers painters Ary (1795-1858) and Henri (1798-1862) Scheffer. Acquired in 1987 by the City of Paris, the Musee de la Vie Romantique presents collections of souvenirs and objects of art legues in the city, recalling two great figures of the 19th century: writer George Sand (Amantine Aurore Lucile Dupin, Baroness Dudevant, 1804-1876) and Ary Scheffer. / Bridgeman Images
PIX4609916: Barree spiral galaxy NGC 1559 and supernova - Barred spiral galaxy NGC 1559 with a supernova - The galaxy NGC 1559 is a galaxy of Seyfert located about 50 million years ago - light in the constellation Reticule. In this image obtained in 2005 by the Kueyen European telescope of the VLT in Chile, a bright star is visible just above the galaxy, a supernova of type Ia named SN 2005df. On the night of August 4, 2005, an amateur astronomer and supernovae discoverer Reverend Robert Evans discovered a supernova just North of this galaxy. This supernova is classified as a somewhat unusual type Ia supernova, caught probably 10 days before it reached its maximum brightness. Such a supernova is thought to be the result of the explosion of a small and dense star - a white dwarf - inside a binary system. As its companion was continuously spilling matter onto the white dwarf, the white dwarf reached a critical mass, leading to a fatal instability. NGC 1559 is a SBc (s) - type spiral galaxy located about 50 million light - years away, that weighs the equivalent of about 10,000 million of suns, and is about 7 times smaller than our Milky Way. Receding from us at a speed of about 1,300 km/s, it is a galaxy of the Seyfert type. Such galaxies are characterized by a bright nucleus that radiates strongly in the blue and in the ultraviolet. Astronomers think that about 2 solar masses of gas per year are transformed into stars in this galaxy. Like most galaxies, NGC 1559 probably contains a black hole in its centre, which should have a mass that is equivalent to 300,000 suns. Colour composite image obtained with the multi - mode FORS1 instrument on ESO's 8.2m VLT. The supernova, SN 2005df, is visible as the bright star just above the galaxy / Bridgeman Images