A frequency approach to identifying asteroid families II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances

Aims. In an earlier paper we introduced a new method for determining asteroid families where families were identified in the proper frequency domain (n, g, g + s) ( where n is the mean-motion, and g and s are the secular frequencies of the longitude of pericenter and nodes, respectively), rather than in the proper element domain (a, e, sin(i)) (semi-major axis, eccentricity, and inclination). Here we improve our techniques for reliably identifying members of families that interact with nonlinear secular resonances of argument other than g or g + s and for asteroids near or in mean-motion resonant configurations. Methods. We introduce several new distance metrics in the frequency space optimal for determining the diffusion in secular resonances of argument 2g - s, 3g - s, g - s, s, and 2s. We also regularize the dependence of the g frequency as a function of the n frequency (Vesta family) or of the eccentricity e (Hansa family). Results. Our new approaches allow us to recognize as family members objects that were lost with previous methods, while keeping the advantages of the Carruba & Michtchenko (2007, A& A, 475, 1145) approach. More important, an analysis in the frequency domain permits a deeper understanding of the dynamical evolution of asteroid families not always obtainable with an analysis in the proper element domain.

Dynamic picture of the inner asteroid belt: implications for the density, size and taxonomic distributions of real objects

In this paper, we construct a dynamic portrait of the inner asteroidal belt. We use information about the distribution of test particles, which were initially placed on a perfectly rectangular grid of initial conditions, after 4.2 Myr of gravitational interactions with the Sun and five planets, from Mars to Neptune. Using the spectral analysis method introduced by Michtchenko et al., the asteroidal behaviour is illustrated in detail on the dynamical, averaged and frequency maps. On the averaged and frequency maps, we superpose information on the proper elements and proper frequencies of real objects, extracted from the data base, AstDyS, constructed by Milani and Knezevic. A comparison of the maps with the distribution of real objects allows us to detect possible dynamical mechanisms acting in the domain under study; these mechanisms are related to mean-motion and secular resonances. We note that the two- and three-body mean-motion resonances and the secular resonances (strong linear and weaker non-linear) have an important role in the diffusive transportation of the objects. Their long-lasting action, overlaid with the Yarkovsky effect, may explain many observed features of the density, size and taxonomic distributions of the asteroids.

Secular dynamics and family identification among highly inclined asteroids in the Euphrosyne region

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

The stable archipelago in the region of the Pallas and Hansa dynamical families

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Dynamical erosion of asteroid groups in the region of the Phocaea family

In a previous paper, the current state of knowledge of the region containing the Phocaea dynamical family was revised. Here, the dynamical evolution and possible origin of the Phocaea dynamical family and asteroid groups in the region are investigated. First, I study the case of asteroids at high eccentricity (e > 0.31). I find that these objects are unstable because of encounters with Mars on time-scales of up to 270 Myr. The minimum time needed by members of the Phocaea classical family to reach the orbital locations of these objects, 370 Myr, can be used to set a lower limit on the age of the Phocaea family.Next, attention is focused on the chaotic layer previously identified near the nu(6) secular resonance border. Using analytical and numerical tools, I find that the presence of the nu(6) secular resonance forces asteroids with vertical bar g-g(6)vertical bar < 2.55 arcsec yr(-1) to reach eccentricities high enough to allow them to experience deep, close encounters with Mars. Results of the analytical model of Yoshikawa and of my numerical simulations fully explain the low-inclination chaotic region found by Carruba.Finally, I investigate the long-term stability of the minor families and clumps identified in the previous paper, with particular emphasis on a clump only identifiable in the domain of proper frequencies (n, g, g - s) around (6246) Komurotoru. I find that while the clumps identified in the space of proper elements quickly disperse when the Yarkovsky effect is considered, the family around (19536) is still observable for time-scales of more than 50 Myr. The (6246) clump, characterized by its interaction with the nu(5) + nu(16) and 2 nu(6) - nu(16) secular resonances, is robust on time-scales of 50 Myr. I confirm that this group may be the first clump ever detected in the frequency domain that can be associated with a real collisional event.

Chaotic diffusion caused by close encounters with several massive asteroids The (4) Vesta case

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

An analysis of the region of the Phocaea dynamical family

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

On the first nu(6) anti-aligned librating asteroid family of Tina

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Chaotic diffusion caused by close encounters with several massive asteroids: II. the regions of (10) Hygiea, (2) Pallas, and (31) Euphrosyne

Context. Close encounters with (1) Ceres and (4) Vesta, the two most massive bodies in the main belt, are known to be a mechanism of dynamical mobility able to significantly alter proper elements of minor bodies, and they are the main source of dynamical mobility for medium-sized and large asteroids (D > 20 km, approximately). Recently, it has been shown that drift rates caused by close encounters with massive asteroids may change significantly on timescales of 30 Myr when different models (i.e., different numbers of massive asteroids) are considered. Aims. So far, not much attention has been given to the case of diffusion caused by the other most massive bodies in the main belt: (2) Pallas, (10) Hygiea, and (31) Euphrosyne, the third, fourth, and one of the most massive highly inclined asteroids in the main belt, respectively. Since (2) Pallas is a highly inclined object, relative velocities at encounter with other asteroids tend to be high and changes in proper elements are therefore relatively small. It was thus believed that the scattering effect caused by highly inclined objects in general should be small. Can diffusion by close encounters with these asteroids be a significant mechanism of long-term dynamical mobility? Methods. By performing simulations with symplectic integrators, we studied the problem of scattering caused by close encounters with (2) Pallas, (10) Hygiea, and (31) Euphrosyne when only the massive asteroids (and the eight planets) are considered, and the other massive main belt asteroids and non-gravitational forces are also accounted for. Results. By finding relatively small values of drift rates for (2) Pallas, we confirm that orbital scattering by this highly inclined object is indeed a minor effect. Unexpectedly, however, we obtained values of drift rates for changes in proper semi-major axis a caused by (10) Hygiea and (31) Euphrosyne larger than what was previously found for scattering by (4) Vesta. These high rates may have repercussions on the orbital evolution and age estimate of their respective families. © 2013 ESO.

An analysis of the Hygiea asteroid family orbital region

(10) Hygiea is the fourth largest asteroid of the main belt, by volume and mass, and it is the largest member of its family, that is made mostly by low-albedo, C-type asteroids, typical of the outer main belt. Like many other large families, it is associated with a 'halo' of objects, that extends far beyond the boundary of the core family, as detected by traditional hierarchical clustering methods (HCM) in proper element domains. Numerical simulations of the orbital evolution of family members may help in estimating the family and halo family age, and the original ejection velocity field. But, in order to minimize the errors associated with including too many interlopers, it is important to have good estimates of family membership that include available data on local asteroid taxonomy, geometrical albedo and local dynamics. For this purpose, we obtained synthetic proper elements and frequencies of asteroids in the Hygiea orbital region, with their errors. We revised the current knowledge on asteroid taxonomy, including Sloan Digital Sky Survey-Moving Object Catalog 4th release (SDSS-MOC 4) data, and geometric albedo data from Wide-field Infrared Survey Explorer (WISE) and Near-Earth Object WISE (NEOWISE). We identified asteroid family members using HCM in the domain of proper elements (a, e, sin (i)) and in the domains of proper frequencies most appropriate to study diffusion in the local web of secular resonances, and eliminated possible interlopers based on taxonomic and geometrical albedo considerations. To identify the family halo, we devised a new hierarchical clustering method in an extended domain that includes proper elements, principal components PC1, PC2 obtained based on SDSS photometric data and, for the first time, WISE and NEOWISE geometric albedo. Data on asteroid size distribution, light curves and rotations were also revised for the Hygiea family. The Hygiea family is the largest group in its region, with two smaller families in proper element domain and 18 families in various frequencies domains identified in this work for the first time. Frequency groups tend to extend vertically in the (a, sin (i)) plane and cross not only the Hygiea family but also the near C-type families of Themis and Veritas, causing a mixture of objects all of relatively low albedo in the Hygiea family area. A few high-albedo asteroids, most likely associated with the Eos family, are also present in the region. Finally, the new multidomains hierarchical clustering method allowed us to obtain a good and robust estimate of the membership of the Hygiea family halo, quite separated from other asteroids families halo in the region, and with a very limited (about 3 per cent) presence of likely interlopers. © 2013 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society.

Mobilidade asteroidal induzida por encontros próximos com vários asteroides massivos

Pós-graduação em Física - FEG

Dinâmica e origem de asteroides de alta inclinação

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

A multidomain approach to asteroid families' identification

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Control of gene expression in melanocytes and RPE by conserved distal regulatory elements

Résumé Durant le développement embryonnaire, les cellules pigmentaires des mammifères se développent à partir de deux origines différentes : les melanocytes se développent à partir de la crête neurale alors que les cellules de la rétine pigmentaire (RP) ont une origine neuronale. Un grand nombre de gènes sont impliqués dans la pigmentation dont les gènes de la famille tyrosinase à savoir Tyr, Tyrp1 et Dct. Certaines études ont suggéré que les gènes de la pigmentation sont régulés de manière différentielle dans les mélanocytes et dans la RP. Dans ce travail, les gènes de la famille tyrosinase ont été étudiés comme modèle de la régulation des gènes de la pigmentation par des éléments régulateurs agissant à distance. II a été montré que le promoteur du gène Tyrp1pouvait induire l'expression d'un transgène uniquement dans la RP alors que ce gène est aussi exprimé dans les mélanocytes comme le montre le phénotype des souris mutantes pour Tyrp1. Ce résultat suggère que les éléments régulateurs du promoteur sont suffisants pour l'expression dans la RP mais pas pour l'expression dans les mélanocytes. J'ai donc cherché à identifier la séquence qui régule l'expression dans les mélanocytes. Un chromosome artificiel bactérien (CAB) contenant le gène Tyrp1 s'est avéré suffisant pour induire l'expression dans les mélanocytes, comme démontré par la correction du phénotype mutant. La séquence de ce CAB contient plusieurs régions très conservées qui pourraient représenter de nouveaux éléments régulateurs. Par la suite, j'ai focalisé mon analyse sur une séquence située à -I5 kb qui s'est révélée être un amplificateur spécifique aux mélanocytes comme démontré par des expériences de cultures cellulaire et de transgenèse. De plus, une analyse poussée de cet élément a révélé que le facteur de transcription Sox 10 représentait un transactivateur de cet amplificateur. Comme pour Tyrp1, la régulation du gène tyrosinase est contrôlée par différents éléments régulateurs dans les mélanocytes et la RP. Il a été montré que le promoteur de tyrosinase n'était pas suffisant pour une forte expression dans les mélanocytes et la RP. De plus, l'analyse de la région située en amont a révélé la présence d'un amplificateur nécessaire à l'expression dans les mélanocytes à la position -15 kb. Cet amplificateur n'est toutefois pas actif dans la RP mais agit comme un répresseur dans ces cellules. Ces résultats indiquent que certains éléments nécessaires à l'expression dans les deux types de cellules pigmentaires sont absents de ces constructions. Comme pour Tyrp1, j'ai en premier lieu démontré qu'un CAB était capable de corriger le phénotype albinique, puis ai inséré un gène reporter (lacZ) dans le CAB par recombinaison homologue et ai finalement analysé l'expression du reporter en transgenèse. Ces souris ont montré une expression forte du lacZ dans les mélanocytes et la RP, ce qui indique que le CAB contient les séquences régulatrices nécessaires à l'expression correcte de tyrosinase. Afin de localiser plus précisément les éléments régulateurs, j'ai ensuite généré des délétions dans le CAB et analysé l'expression du lacZ en transgenèse. La comparaison de séquences génomiques provenant de différentes espèces a permis par la suite d'identifier des régions représentant de nouveaux éléments régulateurs potentiels. En utilisant cette approche, j'ai identifié une région qui se comporte comme un amplificateur dans la RP et qui est nécessaire à l'expression de tyrosinase dans ce tissu. De plus, j'ai identifié les facteurs de transcription Mitf et Sox10 comme transactivateurs de l'amplificateur spécifique aux mélanocytes situé à -15 kb. L'identification et la caractérisation des ces éléments régulateurs des gènes tyrosinase et Tyrp1confirme donc que la régulation différentielle des gènes dans les mélanocytes et la RP est liée à des éléments régulateurs séparés. Summary Pigment cells of mammals originate from two different lineages: melanocytes arise from the neural crest, whereas cells of the retinal pigment epithelium (RPE) originate from the optic cup of the developing forebrain. A large set of genes are involved in pigmentation, including the members of the tyrosinase gene family, namely tyrosinase, Tyrp1 and Dct. Previous studies have suggested that pigmentation genes are differentially regulated in melanocytes and RPE. In this work, the tyrosinase gene family was used as a model for studying the involvement of distal regulatory elements in pigment cell-specific gene expression. The promoter of the Tyrp1 gene has been shown to drive detectable transgene expression only to the RPE, even though the gene is also expressed in melanocytes as evident from Tyrp1-mutant mice. This indicates that the regulatory elements responsible for Tyrp1 gene expression in the RPE are not sufficient for expression in melanocytes. I thus searched for a putative melanocyte-specific regulatory sequence and demonstrate that a bacterial artificial chromosome (BAC) containing the Tyrp1 gene and surrounding sequences is able to target transgenic expression to melanocytes and to rescue the Tyrp1 b (brown) phenotype. This BAC contains several highly conserved non-coding sequences that might represent novel regulatory elements. I further focused on a sequence located at -15 kb which I identified as amelanocyte-specific enhancer as shown by cell culture and transgenic mice. In addition, further functional analysis identified the transcription factor Sox10 as being able to bind and transactivate this enhancer. As for Tyrp1, tyrosinase gene regulation is mediated by different cis-regulatory elements in melanocytes and RPE. It was shown that the tyrosinase promoter was not sufficient to confer strong and specific expression in melanocytes and RPE. Moreover, analysis of tyrosinase upstream sequence, revealed the presence of a specific enhancer at position -15 kb which was necessary to confer strong expression in melanocytes. This enhancer element however failed to act as an enhancer in the RPE, but rather repressed expression. This indicates that some regulatory elements required for tyrosinase expression in both RPE and melanocytes are still missing from these constructs. As for Tyrp1, I first demonstrated that a BAC containing the Tyr gene is able to rescue the Tyr c (albino) phenotype in mice, then I inserted a lacZ reporter gene in the BAC by homologous recombination, and finally analysed the pattern of lacZ expression in transgenic mice. These mice showed strong lacZ expression in both RPE and melanocytes, indicating that the BAC contains the regulatory sequences required for proper tyrosinase expression. In order to localize more precisely these regulatory elements, I have then generated several deletions in the BAC and analysed lacZ expression in transgenic mice. Multi-species comparative genomic analysis then allowed identifying conserved sequences that potentially represent novel regulatory elements. Using this experimental approach, I identified a region that behaves as a RPE-specific enhancer and that is required for tyrosinase expression in the retina] pigment epithelium. In addition, I identified the transcription factors Mitf and Sox l0 as being transactivators of the melanocyte-specific enhancer located at -l5 kb. The identification and characterization of these tyrosinase and Tyrp1 distal regulatory element supports the idea that separate regulatory sequences mediate differential gene expression in melanocytes and RPE.

Information Discovery in Distributed Systems-A Novel Concept Based on Modelling of Information Elements

Sharing of information with those in need of it has always been an idealistic goal of networked environments. With the proliferation of computer networks, information is so widely distributed among systems, that it is imperative to have well-organized schemes for retrieval and also discovery. This thesis attempts to investigate the problems associated with such schemes and suggests a software architecture, which is aimed towards achieving a meaningful discovery. Usage of information elements as a modelling base for efficient information discovery in distributed systems is demonstrated with the aid of a novel conceptual entity called infotron.The investigations are focused on distributed systems and their associated problems. The study was directed towards identifying suitable software architecture and incorporating the same in an environment where information growth is phenomenal and a proper mechanism for carrying out information discovery becomes feasible. An empirical study undertaken with the aid of an election database of constituencies distributed geographically, provided the insights required. This is manifested in the Election Counting and Reporting Software (ECRS) System. ECRS system is a software system, which is essentially distributed in nature designed to prepare reports to district administrators about the election counting process and to generate other miscellaneous statutory reports.Most of the distributed systems of the nature of ECRS normally will possess a "fragile architecture" which would make them amenable to collapse, with the occurrence of minor faults. This is resolved with the help of the penta-tier architecture proposed, that contained five different technologies at different tiers of the architecture.The results of experiment conducted and its analysis show that such an architecture would help to maintain different components of the software intact in an impermeable manner from any internal or external faults. The architecture thus evolved needed a mechanism to support information processing and discovery. This necessitated the introduction of the noveI concept of infotrons. Further, when a computing machine has to perform any meaningful extraction of information, it is guided by what is termed an infotron dictionary.The other empirical study was to find out which of the two prominent markup languages namely HTML and XML, is best suited for the incorporation of infotrons. A comparative study of 200 documents in HTML and XML was undertaken. The result was in favor ofXML.The concept of infotron and that of infotron dictionary, which were developed, was applied to implement an Information Discovery System (IDS). IDS is essentially, a system, that starts with the infotron(s) supplied as clue(s), and results in brewing the information required to satisfy the need of the information discoverer by utilizing the documents available at its disposal (as information space). The various components of the system and their interaction follows the penta-tier architectural model and therefore can be considered fault-tolerant. IDS is generic in nature and therefore the characteristics and the specifications were drawn up accordingly. Many subsystems interacted with multiple infotron dictionaries that were maintained in the system.In order to demonstrate the working of the IDS and to discover the information without modification of a typical Library Information System (LIS), an Information Discovery in Library Information System (lDLIS) application was developed. IDLIS is essentially a wrapper for the LIS, which maintains all the databases of the library. The purpose was to demonstrate that the functionality of a legacy system could be enhanced with the augmentation of IDS leading to information discovery service. IDLIS demonstrates IDS in action. IDLIS proves that any legacy system could be augmented with IDS effectively to provide the additional functionality of information discovery service.Possible applications of IDS and scope for further research in the field are covered.