PIX4569327: Sundial - Invalides - Paris - Sundial in Paris - Hotel des Invalides: The sundials of the western facade of the monument of the Hotel des Invalides. In the court of honour, the hour was given on each facade: to the north, by a clock and on the other three facades, by seven solar dials. If the clock is missing, the dials are still visible / Bridgeman Images
PIX4569354: La Meridienne de la Pitie-Salpetriere - Paris - Sundial in Paris - Hospital de la Pitie-Salpetiere: Outside the chapel of the Pitie-Salpetiere Hospital (75013), a Meridian is visible just above the door. It has the motto: Ultima Latet (the last one is hidden). This simple Meridian features the 11 am, 12 pm and 1 pm hour lines, plus the half-hours on either side of noon. Portions of daytime arches are traced and marked by the signs of the Zodiac / Bridgeman Images
PIX4570101: Comete Hyakutake - Comet Hyakutake - Comete Hyakutake March 1996. This is the spectacular Comet Hyakutake as it passed closest to Earth in March of 1996. The solid portion or nucleus of a comet is made up of ice, frozen gases, dust and small rock. And it is relatively small - less than 15 miles in diameter. As its orbit takes it closer to the sun, this frozen mass begins to melt and a coma, which is a gaseous cloud, develops around the nucleus. This coma can grow to be tens of thousands of miles in diameter. Finally a tail also develops which can become millions of miles long. This color photo reveals the blue - green glow around the coma, the yellow - red shroud of a dust tail, and the many long blue streamers of the ion tail / Bridgeman Images
PIX4570920: Comete 17P/Holmes 29/10/2007 - Comet 17P/Holmes October 29 2007 - On October 24, 2007, Comete 17P/Holmes suddenly increased luminosite and became visible to the naked eye. In this image obtained a few days later in France, the comete is visible near the constellation of Persee (in the center of the image). In late October 2007, Comet Holmes amazingly brightened 15 magnitude (about million times). On October 29, Holmes is easily visible in the sky in the center of image / Bridgeman Images
PIX4572495: Different types of brown dwarves - Artist's view - Different types of brown dwarves. Artwork - From left to right: brown dwarf type M, the youngest and most massive, temperature between 200 and 3000 degres Kelvin; brown dwarf type L, between 1500 and 2000 degres Kelvin; brown dwarf type T, between 1200 and 1500 degres Kelvin; brown dwarf type T but colder, from 1200 to 600 degres Kelvin; brown dwarf type still indefinite, less than 600 degres Kelvin; finally, on the right, Jupiter for size comparison. From left to right: a brown dwarf of type M (the youngest and most massive brown dwarves), a brown dwarf of type L, then a type T, another type T but colder, then another brown dwarf with a type unidentified yet which is colder, at last Jupiter for comparison / Bridgeman Images
PIX4572541: Brown dwarf & debris ring from an oblique perspective - Artist's view of a brown dwarf star about 60 times the mass of Jupiter, surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet enlighted by the star. A small, barren planet orbits obliquely to the plane of a massive set of concentric dust rings surrounding a brown dwarf of about 60 Jupiter masses. These rings are evocative of Saturn's famous rings of rock and ice, however there is likely no ice in the rings around this dwarf. Recent observations have revealed that some brown dwarfs may be surrounded by rings of dust. While the origin of these rings, and the brown dwarfs themselves, is unclear, it's thought that material from these rings may even coalesce into planets, providing some brown dwarfs with their own solar systems / Bridgeman Images
PIX4571099: Comet Lulin (C2007/N3) - View of Comet Lulin (C2007/N3), February 21, 2009. Comet Lulin (C/2007 N3) on February 21, 2009 from 05:41 UT to 06:20 UT. The faint blue ion tail is seen to the upper right, and the anti - tail stretches to the lower left. Composite of 19 two - minute exposures that has been enhanced in Photoshop to bring out faint details in the tails / Bridgeman Images
PIX4571179: Comet C/2009 P1 Garrad - September 2011 - Comet C/2009 P1 Garrad seen near the Hanger cluster (or Brocchi cluster), an asterism located in the constellation Little Fox. September 4, 2011. Comet C/2009 P1 Garrad is seen in the vicinity of the Coathanger asterism, also known as Brocchi's cluster, Al Sufi's cluster or Collinder. September 4, 2011 / Bridgeman Images