domingo, 8 de enero de 2017
The amateur astronomer and visual observer of comets, J.P.Navarro Pina, has discovered a burst of brightness or outburts in a comet near Earth, the comet in particular is called 45P / HONDA-MRKOS-PAJDUSAKOVA, it is a periodical comet, Whose orbit around the sun is every 5 years, currently this comet should be in visual magnitude +7, but on the night of January 5, 2017, the astronomer Murcia, J.P.Navarro Pina, measured the visual magnitude of the comet in 6, is To say 1 magnitude visual more brilliant than it was in previous nights, the discovery of the outburts by Navarro Pina, has put in alert to the international astronomical community, since now the comet could be visible to the naked eye since Any dark place and to be as bright as the comet Halley in 1986, various observers of world comets have confirmed the explosion of brilliance of the Spanish astronomer, comets, are fragile stars, that are composed mostly by water, dust, and rock, From time to time, some of them break or suffer gas and dust eruptions, causing sudden increases in brightness, which make them more spectacular in the night sky. J.P.Navarro Pina, a veteran astronomer from Murcia, and an observer of comet visuals, with more than 30 years of astronomical observations behind him, specialized in Comets, he has participated and collaborated with different astronomical centers and world observatories with his Measures of comets.Adjunt light visual curve of COBS database .
domingo, 25 de diciembre de 2016
My analysis of the visual light curve of Comet C / 2016 U1 NEOWISE indicates that the comet based on its abosolute magnitude of m0 = 11.0 would have an estimated core diameter of D = 1.15 kms (Navarro 2016) based on the formula Of Sosa & Fdez, 2011, and a core radius of Rn = 0.575 km, and an estimated mass of M = 0.3x10 ^ 12 kg (Navarro 2016), my initial conclusions show that this is a small fragment of new comet Of the Oort cloud with very volatile "ice volatiles", the images show a very gaseous and little dusty comet, where the sublimation of gas is greater than the dust, probably a fragment of giant comet detached.
domingo, 6 de noviembre de 2016
viernes, 29 de abril de 2016
MASS , DIAMETER , WATER PRODUCTION , AND ANALYSIS OF THE LIGHT VISUAL CCD OF COMET C/2013 US10 CATALINA
Recent update of the light visual ccd curve based in 2430 ccd's-visual observations frome the database MPC/IAU , i calculated the new photometrical's parameters and i have discovered 3 different photometric laws that dominate the general curve photometric comet , the water rate production max. is 4000 kg/sec. log Q ( H2O ) = 10^29.6 mol sec , the mass estimated is log M (kg ) =11.2 , M = 1.1x10^11 kg , diameter calculated D(kms ) = 0.96 . graphic and analysis down . The general rate production of comet C/2013 US10 CATALINA , ( Jorda et al. 2008 ) [ log Q = -0.8 / n * m0 + C , Result log Q = -3.721 + C ]
domingo, 24 de abril de 2016
I am pleased to announce that I have posted as co-author's work astrophysics comet C / 2011 J2 LINEAR, in collaboration with a group of international researchers in the prestigious journal Astrophysics of Planetary and Space Science publisher Elsevier. You can access the following link to see it: http://www.sciencedirect.com/science/article/pii/S0032063316300265
miércoles, 6 de enero de 2016
My last and personal analysis of the light visual curve ccd+visual , show the data of recent outburts confirmed for multiples observers , the first notice of alert is one message of Stephen McCann UK in the yahoogroups.com comets-ml the 3.87/Jan./2016, the observer alert increment brightness of m1=+8.5 , the last visuals magnitudes from the data indicate range of visual's magnitudes of 9.5 < m1 < 10.5 , the visuals magnitudes : 8.0 , 8.8 , 8.5 and the last recent 7.9 ( Neil Norman , UK ) in the 3 , 4 and 5 January 2016 . The photometric law visual indicate visual magnitude max. of m1~ +5.0 in 20/06/2016 , based in formula m1 = +2.2 + 5 log (d) + 18.2 log (r) , the power law is high n=7.3 , based in R^ (-7.3) .
viernes, 1 de enero de 2016
The motion of dust particles in a cometary environment is a complex process, and a precise description of the trajectories of grains within the coma requires adavnced hydrodynamic models, taking into account the interaction between gas and dust released from the surface. In the tail, dust and gas are decoupled and the only significant forces affecting the grain trajectories are the solar gravity and radiation pressure. Both forces depend on the square of the heliocentric distance but work in opposite directions. Their sum can be seen as a reduced solar gravity, and the equation of motion is simply m*a=(1-beta)*solar_gravity, where beta is the ratio radiation_pressure/solar_gravity, and is inversely proportional to the size of the grains for particles larger than 1 micron. From this relation, Finson & Probstein (1968) proposed a model which describes the full tail geometry with a grid of synchrones and syndynes; lines representing respectively the locations of particles released at a same time, or with the same beta. This model is simple because it considers only particles released in the orbital plane of the comet, and with zero initial velocity, but it provides a very good approximation of the shape of the tail, and has been used successfully to study many comets. One of the many strengths of this model is the possibility to date events in the tail. For instance, one can understand if regions of higher density are related to outbursts of the nucleus, or are a result of fragmentation of large chunks of material within the trail. It can also be used to disentangle between continuous activity, short outbursts, or impacts, when all these events produce a feature which at first look like a normal cometary tail.