1998 SF36 from the 2001 apparition cam-paign, and we discuss the corresponding physical model. The asteroid’s photometric behaviour is consistent with an S-type object, it has a retrograde pole at λ = 355, β = −84 5, and its sidereal rotation period is P = 12.132 0.0005 hours. 1998 SF36 is elongated, with rough global dimension ratios a/b = 2.0, b/c = 1.3, but the elongation is not due to a bifurcated shape. The surface is not likely to contain major concavities. No significant albedo variegation was detected. Key words. solar system: minor planets, asteroids – techniques: photometric – methods: numerica
International audienceContext: Asteroid 2867 Steins is the first target of the Rosetta space mission...
Aims. Very small asteroids (VSAs, objects with diameters smaller than about 150 m) can be spun up by...
Context. Near-Earth asteroid 162173 (1999 JU3) is a potential target of two asteroid sample return m...
International audienceWe present photometric observations of the near-Earth asteroid (25143) 1998 SF...
We present photometric observations of the near-Earth asteroid (25143) 1998 SF36 from the 2001 appar...
2003) carried out at six observatories are presented. Using all available lightcurves, the spin vect...
Gaia will make accurate photo- and astrometric observa-tions of thousands of asteroids in sparse epo...
Aims.We observed a near-Earth asteroid 2004 RZ164 to study its rotational properties. The object was...
The term “homeland security”, seems to have become synonymous with terrorism in the minds of the gen...
Texto completo: acesso restrito. p. 1804-1811On October 6, 2008, a small F-class asteroid 2008 TC3 w...
Copyright ESO. The original version is available at www.aanda.org.International audienceThe larger n...
Aims. We investigated the physical properties and dynamical evolution of near-Earth asteroid (NEA) (...
Context. The shapes and spin states of asteroids observed with photometric techniques can be reconst...
We present new observations and models of the shapes and rotational states of the eight near-Earth A...
Context. Asteroid 2867 Steins is the first target of the Rosetta space mission with a flyby schedule...
International audienceContext: Asteroid 2867 Steins is the first target of the Rosetta space mission...
Aims. Very small asteroids (VSAs, objects with diameters smaller than about 150 m) can be spun up by...
Context. Near-Earth asteroid 162173 (1999 JU3) is a potential target of two asteroid sample return m...
International audienceWe present photometric observations of the near-Earth asteroid (25143) 1998 SF...
We present photometric observations of the near-Earth asteroid (25143) 1998 SF36 from the 2001 appar...
2003) carried out at six observatories are presented. Using all available lightcurves, the spin vect...
Gaia will make accurate photo- and astrometric observa-tions of thousands of asteroids in sparse epo...
Aims.We observed a near-Earth asteroid 2004 RZ164 to study its rotational properties. The object was...
The term “homeland security”, seems to have become synonymous with terrorism in the minds of the gen...
Texto completo: acesso restrito. p. 1804-1811On October 6, 2008, a small F-class asteroid 2008 TC3 w...
Copyright ESO. The original version is available at www.aanda.org.International audienceThe larger n...
Aims. We investigated the physical properties and dynamical evolution of near-Earth asteroid (NEA) (...
Context. The shapes and spin states of asteroids observed with photometric techniques can be reconst...
We present new observations and models of the shapes and rotational states of the eight near-Earth A...
Context. Asteroid 2867 Steins is the first target of the Rosetta space mission with a flyby schedule...
International audienceContext: Asteroid 2867 Steins is the first target of the Rosetta space mission...
Aims. Very small asteroids (VSAs, objects with diameters smaller than about 150 m) can be spun up by...
Context. Near-Earth asteroid 162173 (1999 JU3) is a potential target of two asteroid sample return m...