Search Publications

A planetary system as the origin of structure in Fomalhaut's dust belt
DOI: 10.1038/nature03601 Bibcode: 2005Natur.435.1067K

Kalas, Paul; Graham, James R.; Clampin, Mark

The Sun and >15per cent of nearby stars are surrounded by dusty disks that must be collisionally replenished by asteroids and comets, as the dust would otherwise be depleted on timescales <107years (ref. 1). Theoretical studies show that the structure of a dusty disk can be modified by the gravitational influence of planets, but t…

2005 Nature
eHST 345
Imaging of Titan from the Cassini spacecraft
DOI: 10.1038/nature03436 Bibcode: 2005Natur.434..159P

Dones, Luke; Porco, Carolyn C.; McEwen, Alfred +33 more

Titan, the largest moon of Saturn, is the only satellite in the Solar System with a substantial atmosphere. The atmosphere is poorly understood and obscures the surface, leading to intense speculation about Titan's nature. Here we present observations of Titan from the imaging science experiment onboard the Cassini spacecraft that address some of …

2005 Nature
Cassini 318
Tropical to mid-latitude snow and ice accumulation, flow and glaciation on Mars
DOI: 10.1038/nature03359 Bibcode: 2005Natur.434..346H

Jaumann, R.; Head, J. W.; Neukum, G. +11 more

Images from the Mars Express HRSC (High-Resolution Stereo Camera) of debris aprons at the base of massifs in eastern Hellas reveal numerous concentrically ridged lobate and pitted features and related evidence of extremely ice-rich glacier-like viscous flow and sublimation. Together with new evidence for recent ice-rich rock glaciers at the base o…

2005 Nature
MEx 291
An upper limit to the masses of stars
DOI: 10.1038/nature03293 Bibcode: 2005Natur.434..192F

Figer, Donald F.

There is no accepted upper mass limit for stars. Such a basic quantity eludes both theory and observation, because of an imperfect understanding of the star-formation process and because of incompleteness in surveying the Galaxy. The Arches cluster is ideal for investigating such limits, being large enough to expect stars at least as massive as ~5…

2005 Nature
eHST 275
Differentiation of the asteroid Ceres as revealed by its shape
DOI: 10.1038/nature03938 Bibcode: 2005Natur.437..224T

Russell, C. T.; Stern, S. A.; Young, E. F. +4 more

The accretion of bodies in the asteroid belt was halted nearly 4.6billion years ago by the gravitational influence of the newly formed giant planet Jupiter. The asteroid belt therefore preserves a record of both this earliest epoch of Solar System formation and variation of conditions within the solar nebula. Spectral features in reflected sunligh…

2005 Nature
eHST 238
The mass of the missing baryons in the X-ray forest of the warm-hot intergalactic medium
DOI: 10.1038/nature03245 Bibcode: 2005Natur.433..495N

Elvis, Martin; Zezas, Andreas; Marshall, Herman +7 more

Recent cosmological measurements indicate that baryons comprise about four per cent of the total mass-energy density of the Universe, which is in accord with the predictions arising from studies of the production of the lightest elements. It is also in agreement with the actual number of baryons detected at early times (redshifts z > 2). Close …

2005 Nature
eHST 189
Release of volatiles from a possible cryovolcano from near-infrared imaging of Titan
DOI: 10.1038/nature03596 Bibcode: 2005Natur.435..786S

Rodriguez, S.; Sotin, C.; Brown, R. H. +23 more

Titan is the only satellite in our Solar System with a dense atmosphere. The surface pressure is 1.5bar (ref. 1) and, similar to the Earth, N2 is the main component of the atmosphere. Methane is the second most important component, but it is photodissociated on a timescale of 107years (ref. 3). This short timescale has led to…

2005 Nature
Cassini 166
Discovery of an aurora on Mars
DOI: 10.1038/nature03603 Bibcode: 2005Natur.435..790B

Bertaux, Jean-Loup; Leblanc, François; Korablev, Oleg +5 more

In the high-latitude regions of Earth, aurorae are the often-spectacular visual manifestation of the interaction between electrically charged particles (electrons, protons or ions) with the neutral upper atmosphere, as they precipitate along magnetic field lines. More generally, auroral emissions in planetary atmospheres ``are those that result fr…

2005 Nature
MEx 166
Complex organic matter in Titan's atmospheric aerosols from in situ pyrolysis and analysis
DOI: 10.1038/nature04349 Bibcode: 2005Natur.438..796I

Steller, M.; Atreya, S. K.; Owen, T. +19 more

Aerosols in Titan's atmosphere play an important role in determining its thermal structure. They also serve as sinks for organic vapours and can act as condensation nuclei for the formation of clouds, where the condensation efficiency will depend on the chemical composition of the aerosols. So far, however, no direct information has been available…

2005 Nature
Cassini 156
An overview of the descent and landing of the Huygens probe on Titan
DOI: 10.1038/nature04347 Bibcode: 2005Natur.438..758L

Lebreton, Jean-Pierre; Witasse, Olivier; Matson, Dennis L. +9 more

Titan, Saturn's largest moon, is the only Solar System planetary body other than Earth with a thick nitrogen atmosphere. The Voyager spacecraft confirmed that methane was the second-most abundant atmospheric constituent in Titan's atmosphere, and revealed a rich organic chemistry, but its cameras could not see through the thick organic haze. After…

2005 Nature
Cassini 153