Orbit Determination of Binary Asteroids     

Daniel Hestroffer  Frédéric Vachier  Benjamin Balat 《Earth, Moon, and Planets》2005,97(3-4):245-260

In addition to the detection of an asteroid moon or a binary asteroid, the knowledge of the satellite’s true orbit is of high importance to derive fundamental physical parameters of the binary system such as its mass and to shed light on its possible formation history and dynamical evolution (prograde/retrograde orbit, large/small eccentricity or inclination, etc.). A new methodology for preliminary orbit determination of binary asteroids – and visual binaries in general – is proposed. It is based on Thiele–Innes method combined with a ‘trial and error’ Monte-Carlo technique. This method provides the full set of solutions (bundle of orbits, with the 7 orbital elements) even for a reduced number of observations. The mass is a direct by-product of this orbit determination, from which one can next infer the bulk-density and porosity. In addition to the bundle of orbits, the method provides the marginal probability densities of the foreseen parameters. Such error analysis – since it avoids linear approximation – can be of importance for the prediction of the satellite’s position in the plane-of-sky during future stellar occultations or subsequent observations, but also for the analysis of the orbit’s secular evolution. After briefly describing the method, we present the algorithm and its application to some practical cases, with particular emphasis on asteroids binaries and applications on orbital evolution.  相似文献   

Ccd Photometry of the Neglected Contact Binaries V344 Lac and V1191 Cyg     

Theodor Pribulla  Martin Vaňko  DrahomÍr Chochol  Štefan Parimucha  Daniel Baluďanský 《Astrophysics and Space Science》2005,296(1-4):281-284

New photoelectric and CCD observations of the eclipsing contact binary systems V344 Lac and V1191 Cyg are presented and analyzed. All available times of minimum light were used to study period changes of the systems and determine up-to-date ephemerides. The orbital period of V1191 Cyg is found to be increasing at a very fast rate. The photometric elements were determined using the new light curve, radial-velocity curve and broadening function fitting code ROCHE.  相似文献   

The Hubble Deep Field-North SCUBA Super-map – IV. Characterizing submillimetre galaxies using deep Spitzer imaging     

Alexandra Pope  Douglas Scott  Mark Dickinson  Ranga-Ram Chary  Glenn Morrison  Colin Borys  Anna Sajina  David M. Alexander  Emanuele Daddi †  David Frayer  Emily MacDonald  Daniel Stern 《Monthly notices of the Royal Astronomical Society》2006,370(3):1185-1207

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Mutual Potential of Homogeneous Polyhedra   总被引：2，自引：0，他引：2  

Robert A. Werner  Daniel J. Scheeres 《Celestial Mechanics and Dynamical Astronomy》2005,91(3-4):337-349

The mutual gravitational potential between a pair of homogeneous polyhedra is expressed using an infinite series. The nested volume integrals are evaluated analytically and result in simple tensor expressions containing no special functions. However, complexity increases as O(6 ⁿ ), where n is the term degree. An alternate formulation due to Liebenthal is also presented.  相似文献   

Rejuvenation of spiral bulges     

Daniel Thomas  Roger L. Davies 《Monthly notices of the Royal Astronomical Society》2006,366(2):510-520

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The 6dF Galaxy Survey: samples, observational techniques and the first data release     

D. Heath Jones  Will Saunders  Matthew Colless  Mike A. Read  Quentin A. Parker  Fred G. Watson  Lachlan A. Campbell  Daniel Burkey  Thomas Mauch  Lesa Moore  Malcolm Hartley  Paul Cass  Dionne James  Ken Russell  Kristin Fiegert  John Dawe  John Huchra  Tom Jarrett  Ofer Lahav  John Lucey  Gary A. Mamon  Dominique Proust  Elaine M. Sadler  Ken-ichi Wakamatsu 《Monthly notices of the Royal Astronomical Society》2004,355(3):747-763

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Study of a Moon's artificial satellite dynamics valid for all eccentricities and inclinations     

Daniel Steichen 《Celestial Mechanics and Dynamical Astronomy》1993,57(1-2):245-246

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Radar observations of asteroid 1998 ML14     

Steven J. OSTRO  R. Scott HUDSON  Lance A. M. BENNER  Michael C. NOLAN  Jon D. GIORGINI  Daniel J. SCHEERES  Raymond F. JURGENS  Randy ROSE 《Meteoritics & planetary science》2001,36(9):1225-1236

Abstract— Goldstone and Arecibo delay‐Doppler radar imaging of asteroid 1998 ML 14 shortly after its discovery reveals a 1 km diameter spheroid with prominent topography on one side and subdued topography on the other. The object's radar and optical properties are typical for S‐class near‐Earth asteroids. The gravitational slopes of a shape model derived from the images and assumed to have a uniform density are shallow, exceeding 30° over only 4% of the surface. If 1998 ML14's density distribution is uniform, then its orbital environment is similar to a planetary body with a spheroidal gravitational field and is relatively stable. Integration of a radar‐refined orbit reveals that the 1998 apparition was the asteroid's closest approach to Earth since at least 1100 and until 2283, when it approaches to within 2.4 lunar distances. Outside of that time interval, orbit uncertainties based on the present set of observations preclude reliable prediction.  相似文献   

Instantaneous Phase and Amplitude Correlation in the Solar Cycle     

Mininni  Pablo D.  Gomez  Daniel O.  Mindlin  Gabriel B. 《Solar physics》2002,208(1):167-179

In the present study we address the issue of discerning between deterministic and stochastic paradigms in order to understand the behavior of the solar cycle. To this end we show the degree of correlation between the instantaneous amplitude and frequency in the sunspot number time series by the use of the Gabor analytic signal. We compare this correlation with those arising from two theoretical models: (a) the Barnes model of widespread use in the literature and (b) a spatial truncation of the MHD equations. We show that comparisons between the correlation observed in the sunspot time series with those arising from theoretical models can be used to refute one of the models.  相似文献   

Under the shadow of the Magellanic Bridge: A measurement of the extragalactic background at ∼ 0.7 keV     

Q.Daniel Wang  Ye Taisheng 《New Astronomy》1996,1(3):245-253

We measured the extragalactic 0.7 keV X-ray background by observing the X-ray shadow of a neutral gas cloud in the Magellanic Bridge region. Two ROSAT PSPC observations of total 104 ks were complemented by a detailed H I mapping of the cloud with both the Parkes 64 m telescope and the Australia Telescope Compact Array. From the detected anti-correlation between the observed background intensity and the H I column density of the cloud, we derived the unabsorbed extragalactic background intensity as ∼ 28 keV s⁻¹ cm⁻² keV⁻¹ sr⁻¹ at ∼ 0.7 keV. The 95% confidence lower limit 18 keV s⁻¹ cm⁻² keV⁻¹ sr⁻¹ is greater than the expected point-like source contribution ? 14 keV s⁻¹ cm⁻² keV⁻¹ sr⁻¹, constrained by the mean source spectrum together with the total background intensity in the 1-2 keV band. A significant fraction of the 0.7 keV background likely arises in a diffuse hot intergalactic medium of a few million degrees, as has been predicted in hydrodynamic simulations of cosmological structure formation.Richard McCray  相似文献