Nueva hipótesis para explicar el giro de los planetas al derredor del sol, las figuras oblicudades e irregularidades de sus orbitas, el movimiento de rotación de los mismos plantas y algunos otros fenómenos por J. de Jesús Dabila y Prieto

UANL

Experiencia de la desaparición en Lumpérica de Diamela Eltit, Los planetas de Sergio Chejfec y Los rubios de Albertina Carri

Cette thèse analyse l’articulation de l’expérience de la perte d’expérience à laquelle donnent lieu les dictatures et les post-dictatures au Chili et en Argentine dans Lumpérica (1983) de Diamela Eltit, Los planetas (1999) de Sergio Chejfec, et Los rubios (2003) d’Albertina Carri. Les dernières dictatures militaires dans le Cône sud latino-américain imposent ou préparent le terrain pour l’implantation d’un nouvel ordre néolibéral qui s’intensifie sous les régimes démocratiques postérieurs. Au cours de cette transition, le terrorisme d’État au moyen duquel les gouvernements militaires visent à éliminer toute forme de résistance à la reconfiguration de la société nécessaire à la mise en place de politiques néolibérales, donne lieu à une expérience inédite, difficile à communiquer. De plus, autant les dictatures que les démocraties post-dictatoriales mettent en oeuvre des mécanismes d’oubli du passé, soit par la répression, le consensus politique ou les moyens de communication de masse. C’est dans ce contexte que l’expérience disparaît. Le questionnement sur l’expérience de la perte d’expérience est basé principalement sur deux axes théoriques: le concept de transition de l’État au Marché dans le Cône sud latino-américain développé par des intellectuels tels que Willy Thayer, Idelber Avelar ou Brett Levinson, parmi d’autres, ainsi que sur les réflexions sur l’expérience dictatoriale de Sergio Rojas et sur la crise de l’expérience dans la modernité de Walter Benjamin. Le premier chapitre, dédié à Lumpérica, interprète le rituel nocturne où la protagoniste, une femme appelée L. Iluminada, séduit le protagoniste masculin du roman, un panneau électrique appelé “el luminoso” qui projette des messages publicitaires au milieu d’une place publique de Santiago, pour que celui-ci la blesse et marque sa peau, comme la mise en scène d’un “désir photographique” de garder une empreinte de la transition que d’autres moyens de communication tendent à effacer. Le deuxième chapitre traite de la figuration de l’excès dans Los planetas et analyse comment l’écriture, la photographie et l’espace urbain, en assumant une fonction de suppléments de la voix et de la présence de M, séquestré et disparu pendant la dictature argentine, rendent compte de l’expérience de la perte de l’expérience d’une plénitude. Après avoir exposé le rôle des jouets dans la polémique générée par Los rubios, le troisième chapitre analyse comment le film de Carri sur la mémoire de ses parents disparus transmet l’expérience des générations post-dictatoriales et fait face à l’héritage du passé par le jeu.

El sistema solar, els cometes, els meteorits i els asteroides, els planetes. 'El sistema solar, los cometas, los meteoritos y los asteroides, los planetas'.

Cuaderno didáctico sobre el sistema solar, los cometas, los meteoritos, los asteroides y los planetas. Forma parte de una carpeta didáctica centrada en temas de astronomía que cuenta también con un planisferio celeste y un poster de la luna.

Planetas, luces y estrellas.

Resumen de las autoras

A la búsqueda de nuevos planetas.

Programa emitido el 25 de abril de 1996

Planetas, luces y estrellas.

Se presenta una secuencia didáctica llevada a cabo con niños de 4 años en torno a las estrellas y los planetas. Se realiza una visita al Planetario de Madrid y se desarrollan actividades en torno al área de expresión plástica.

Interação estrela planeta: sobre o magnetismo de planetas gigantes gasosos

In this thesis we analyze the effects that the presence of a near gas giant planet can cause in its host star. It has been argued that the star planet interaction can cause changes in the coronal and chromospheric stellar activity. With this in mind, we analyze a sample of 53 extrasolar planets orbiting F, G and K main sequence stars, among them three super-Earths. In this analysis, we look for evidence of changes in the chromospheric activity due to the proximity of the giant planet. We show that, so far, there is not enough evidence to support such a hypothesis. Making use of the same sample and also taking in account available data for the Solar System, we revisit the so-called magnetic Bode s law. This law proposes the existence of a direct relationship between magnetism and rotation. By using estimations for the stellar and planetary magnetic momentM and the angular momentumL, we construct a Blackett s diagram (logL 􀀀logM). In this diagram is evident that the magnetic Bode s law is valid for both the Solar System and the new planetary systems

Um estudo sobre o momentum angular total de estrelas com planetas

Since Michel Mayor and his student Didier Queloz s pioneer announcement, in 1995, of the existence of a planet orbiting the star 51 Peg, up to present date, 695 extrasolar planets orbiting stars of spectral type F, G, K and M have been discovered. A study on the behavior of the total angular momentum of the planetary systems known up to present date becomes relevant when we know that about 98% of the angular momentum of the solar system is associated with the planets, although they represent only 0.15 percent of the mass of the whole system. In this dissertation we study the behavior of stellar angular momentum, orbital angular momentum and total angular momentum in a sample of 282 stars harboring planets, including 40 multiple systems. We observed that planetary systems containing more than one known planet have both higher orbital angular momentum and total angular momentum compared to those who have only one planet. This analysis shows that multiplanet systems tend to have higher momenta, suggesting that the planets in such systems that contribute to the greater portion momenta have been found. Thus, planetary systems with lower values for the momenta represent the best candidates to the discovery of new planets

Propriedades físicas de planetas extrasolares

ROTATION is one the most important aspects to be observed in stellar astrophysics. Here we investigate that particularly in stars with planets. This physical parameter supplies information about the distribution of angular momentum in the planetary system, as well as its role on the control of dierent phenomena, including coronal and cromospherical emission and on the ones due of tidal effects. In spite of the continuous solid advances made on the study of the characteristics and properties of planet host stars, the main features of their rotational behavior is are not well established yet. In this context, the present work brings an unprecedented study about the rotation and angular momentum of planet-harbouring stars, as well as the correlation between rotation and stellar and planetary physical properties. Our analysis is based on a sample of 232 extrasolar planets, orbiting 196 stars of dierent luminosity classes and spectral types. In addition to the study of their rotational behavior, the behavior of the physical properties of stars and their orbiting planets was also analyzed, including stellar mass and metallicity, as well as the planetary orbital parameters. As main results we can underline that the rotation of stars with planets present two clear features: stars with Tef lower than about 6000 K have slower rotations, while among stars with Tef > 6000 K we and moderate and fast rotations, though there are a few exceptions. We also show that stars with planets follow mostly the Krafts law, namely < J > / v rot. In this same idea we show that the rotation versus age relation of stars with planets follows, at least qualitatively, the Skumanich and Pace & Pasquini laws. The relation rotation versus orbital period also points for a very interesting result, with planet-harbouring stars with shorter orbital periods present rather enhanced rotation

Caracterização infravermelho e distribuição espectral de energia para as estrelas com planetas

Neste trabalho estudamos o comportamento das estrelas pertencentes a sistemas planetários no que diz respeito às suas características infravermelho e à distribuição espectral de energia (SED). Nosso estudo tem como base uma análise detalhada do comportamento da emissão no infravermelho de 48 estrelas com planetas, classificadas como estrelas da seqüência principal, subgigantes ou gigantes. Foram analisados dados de fotometria infravermelho nas bandas 12, 25 e 60µm do catálogo de fontes IRAS puntiformes (IPSC) e nas bandas JHK do projeto 2 Micron All Sky Survey (2MASS). A partir do cálculo da discrepância na posição de apontamento da fonte e do cálculo do índice de cor, selecionamos e localizamos os objetos no diagrama de cor-cor do IRAS. Este diagrama permite-nos identificar possíveis objetos detentores de disco de poeira. Fizemos também uma análise da distribuição espectral de energia onde observamos também traços de excesso de fluxo no infravermelho, com isso, confirmarmos a presença do disco de poeira nos objetos identificados no diagrama de cor. Apesar da atual amostra de estrelas com planetas incluir apenas um subconjunto de estrelas com planetas detectadas na vizinhança solar, a presente análise do fluxo infravermelho nesses objetos oferecem uma possibilidade única de estudar as características infravermelho das estrelas pertencentes aos sistemas planetários extra-solar. Neste contexto, nosso estudo aponta resultados interessantes, entre outros destacamos o fato de algumas estrelas com planetas apresentarem um peculiar fluxo IRAS [60-25], indicando a co-existência de poeira juntamente com os planetas destes sistemas extra solar

Atividade cromosférica induzida por planetas extrasolares gigantes

In the present work, we have analyzed the behavior of the chromospheric activity of stars with planets, as a function of different planetary parameters, searching for possible effects of planets on the chromosphere of the hosting star. For this study we have selected a sample of 73 main sequence stars with planets, of spectral types F, G and K. Our analysis shows that among stars with planets presenting semi-major axis smaller than 0.15 AU, a few ones present enhanced CaII emission flux, paralleling recent results found in the literature for coronal X-ray flux. Nevertheless, in contrast to Kashyap et al. (2008), who claim that enhanced X-ray flux in stars with planets is associated to massive close-in planetary companions, we suggest that such an aspect, at least in the context of CaII emission flux, is rather an effect of stellar sample selection. We have also studied the behavior of the CaII emission as a function of orbital parameters such as orbital period and eccentricity, and no clear trend was found, reinforcing our present suggestion that enhanced chromospheric activity in stars with planets is an intrinsic stellar phenomenon

Parâmetros físico-químicos de estrelas com planetas na missão CoRoT

In the present study we compute the atmospheric parameters (Teff , log g and vmic, [Fe/H]) and chemical abundance of 16 ions (Fe I, Fe II, O I, Si I, Na I, Mg I, Al I, Ca I, Ti I, Co I, Ni I, Rb I, Zr I, Ba II, La II and Cr I) for 16 solar-like stars with masses between 0:8 and 1:2 Mfi aproximatedly, including 10 planet-host stars detected by the CoRoT Space Mission. For this study, we use data from the ESO public archive: (i) high resolution spectra (R 47000) from the UVES spectrograph on the VLT/UT2-ESO (for 7 stars, covering the wavelength range 3450-4515 Å and 5500-9400 Å) and (ii) high resolution spectra from HARPS spectrograph on the La Silla-ESO 3.60 m telescope (for 9 stars, covering the wavelength range 4200-6865 Å). Our spectral analysis is based on MARCS models of atmosphere and Turbospectrum spectroscopic tools. On the base of the computed parameters, the referred abundances appears to follow the same behavior of the solar curve abundances. Further, one observes a signifficant correlation between the abundance ratio [m/Fe] and condensation temperature (Tc) of refractory elements (Tc > 900 K). The behavior of the projected rotational velocity (v sin i) versus the computed abundances [m/Fe] is also analyzed, presenting no clear trends. This study oers additional constraints to trace the evolutive history of solar-like stars with planets, including the search for chemical dierences between stars with and without transit planets and anomalies in the studied abundances

Estudos da formação de planetas terrestres

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

Cálculo diferencial e integral no movimento dos planetas

Pós-graduação em Matemática em Rede Nacional - IBILCE