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Evidence from the Mars Express High Resolution Stereo Camera for a frozen sea close to Mars' equator
Murray JB Muller JP Neukum G Werner SC van Gasselt S Hauber E Markiewicz WJ Head JW Foing BH Page D Mitchell KL Portyankina G;HRSC Co-Investigator Team 《Nature》2005,434(7031):352-356
It is thought that the Cerberus Fossae fissures on Mars were the source of both lava and water floods two to ten million years ago. Evidence for the resulting lava plains has been identified in eastern Elysium, but seas and lakes from these fissures and previous water flooding events were presumed to have evaporated and sublimed away. Here we present High Resolution Stereo Camera images from the European Space Agency Mars Express spacecraft that indicate that such lakes may still exist. We infer that the evidence is consistent with a frozen body of water, with surface pack-ice, around 5 degrees north latitude and 150 degrees east longitude in southern Elysium. The frozen lake measures about 800 x 900 km in lateral extent and may be up to 45 metres deep--similar in size and depth to the North Sea. From crater counts, we determined its age to be 5 +/- 2 million years old. If our interpretation is confirmed, this is a place that might preserve evidence of primitive life, if it has ever developed on Mars. 相似文献
14.
Gehrels N Sarazin CL O'Brien PT Zhang B Barbier L Barthelmy SD Blustin A Burrows DN Cannizzo J Cummings JR Goad M Holland ST Hurkett CP Kennea JA Levan A Markwardt CB Mason KO Meszaros P Page M Palmer DM Rol E Sakamoto T Willingale R Angelini L Beardmore A Boyd PT Breeveld A Campana S Chester MM Chincarini G Cominsky LR Cusumano G de Pasquale M Fenimore EE Giommi P Gronwall C Grupe D Hill JE Hinshaw D Hjorth J Hullinger D Hurley KC Klose S Kobayashi S Kouveliotou C Krimm HA Mangano V 《Nature》2005,437(7060):851-854
Gamma-ray bursts (GRBs) come in two classes: long (> 2 s), soft-spectrum bursts and short, hard events. Most progress has been made on understanding the long GRBs, which are typically observed at high redshift (z approximately 1) and found in subluminous star-forming host galaxies. They are likely to be produced in core-collapse explosions of massive stars. In contrast, no short GRB had been accurately (< 10') and rapidly (minutes) located. Here we report the detection of the X-ray afterglow from--and the localization of--the short burst GRB 050509B. Its position on the sky is near a luminous, non-star-forming elliptical galaxy at a redshift of 0.225, which is the location one would expect if the origin of this GRB is through the merger of neutron-star or black-hole binaries. The X-ray afterglow was weak and faded below the detection limit within a few hours; no optical afterglow was detected to stringent limits, explaining the past difficulty in localizing short GRBs. 相似文献
15.
R W Le Page 《Nature》1967,216(5120):1141-1142
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We experimentally tested a model predicting that colony-level genotypic diversity contributes to colonylevel foraging flexibility in honey bees. We established a colony into which we placed individually marked workers from three genetically distinct groups. The colony was placed in an enclosure that contained feeding stations with pollen and sugar syrup. Foraging resources, stores of pollen and the quantity of brood within the colony were varied temporally. Individual foragers switched between resource types in response to changes in relative resource quality and colony need, demonstrating flexibility in resource choice at the individual level. However, genetic groups within the colony varied in their tendency to collect pollen versus nectar, and in lability of response to changes in foraging stimuli. Our data suggest that within-colony genotypic diversity contributes to a resilient foraging response to environmental variation. 相似文献
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D Vilchez L Boyer I Morantte M Lutz C Merkwirth D Joyce B Spencer L Page E Masliah WT Berggren FH Gage A Dillin 《Nature》2012,489(7415):304-308
18.
Page MJ Symeonidis M Vieira JD Altieri B Amblard A Arumugam V Aussel H Babbedge T Blain A Bock J Boselli A Buat V Castro-Rodríguez N Cava A Chanial P Clements DL Conley A Conversi L Cooray A Dowell CD Dubois EN Dunlop JS Dwek E Dye S Eales S Elbaz D Farrah D Fox M Franceschini A Gear W Glenn J Griffin M Halpern M Hatziminaoglou E Ibar E Isaak K Ivison RJ Lagache G Levenson L Lu N Madden S Maffei B Mainetti G Marchetti L Nguyen HT O'Halloran B Oliver SJ Omont A Panuzzo P Papageorgiou A 《Nature》2012,485(7397):213-216
The old, red stars that constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at remarkable rates and active galactic nuclei (AGN) shone brightly as a result of accretion onto black holes. It is widely suspected, but unproved, that the tight correlation between the mass of the black hole and the mass of the stellar bulge results from the AGN quenching the surrounding star formation as it approaches its peak luminosity. X-rays trace emission from AGN unambiguously, whereas powerful star-forming galaxies are usually dust-obscured and are brightest at infrared and submillimetre wavelengths. Here we report submillimetre and X-ray observations that show that rapid star formation was common in the host galaxies of AGN when the Universe was 2-6 billion years old, but that the most vigorous star formation is not observed around black holes above an X-ray luminosity of 10(44) ergs per second. This suppression of star formation in the host galaxy of a powerful AGN is a key prediction of models in which the AGN drives an outflow, expelling the interstellar medium of its host and transforming the galaxy's properties in a brief period of cosmic time. 相似文献
19.
Gehrels N Norris JP Barthelmy SD Granot J Kaneko Y Kouveliotou C Markwardt CB Mészáros P Nakar E Nousek JA O'Brien PT Page M Palmer DM Parsons AM Roming PW Sakamoto T Sarazin CL Schady P Stamatikos M Woosley SE 《Nature》2006,444(7122):1044-1046
Gamma-ray bursts (GRBs) are known to come in two duration classes, separated at approximately 2 s. Long-duration bursts originate from star-forming regions in galaxies, have accompanying supernovae when these are near enough to observe and are probably caused by massive-star collapsars. Recent observations show that short-duration bursts originate in regions within their host galaxies that have lower star-formation rates, consistent with binary neutron star or neutron star-black hole mergers. Moreover, although their hosts are predominantly nearby galaxies, no supernovae have been so far associated with short-duration GRBs. Here we report that the bright, nearby GRB 060614 does not fit into either class. Its approximately 102-s duration groups it with long-duration GRBs, while its temporal lag and peak luminosity fall entirely within the short-duration GRB subclass. Moreover, very deep optical observations exclude an accompanying supernova, similar to short-duration GRBs. This combination of a long-duration event without an accompanying supernova poses a challenge to both the collapsar and the merging-neutron-star interpretations and opens the door to a new GRB classification scheme that straddles both long- and short-duration bursts. 相似文献
20.
Earth science: the rise and growth of Tibet 总被引:1,自引:0,他引:1