domingo, 10 de octubre de 2010

Origen de la vida

Llegará el momento en que abordemos el origen de la vida en clase, mientras tanto, podemos abrir boca con esta noticia publicada hace unos días. Nos habla de Titán una de las lunas de Saturno, donde al parecer, podrían darse las condiciones para la aparición de aminoácidos y nucleótidos (moléculas orgánicas imprescindibles para la aparición de la vida). Lo más sorprendente es que eso podría ocurrir en la atmósfera, cuando siempre hemos supuesto que eso sólo podría ocurrir en los océanos.

It's unlikely that the process produced Titanians, but experiments simulating the chemistry of the dense air on Saturn's biggest moon have yielded some of the basic buildings blocks of life. Scientists described how they used radio-frequency radiation—a more convenient substitute for ultraviolet sunlight—to turn methane, nitrogen, and carbon monoxide (the main constituents of Titan's atmosphere) into glycine and alanine, the two smallest amino acids. The experiments also produced cytosine, adenine, thymine, and guanine, the four most basic components of DNA. And they created uracil, a precursor of RNA. The researchers said that because they achieved the reactions without the presence of liquid water, it's possible life could have sprung forth on Earth not in the seas, as commonly assumed, but perhaps in the planet's early atmosphere—a considerably thinner version of the fog enveloping Titan today.

lunes, 4 de octubre de 2010

El pionero de la fecundación in vitro gana el premio Nobel de medicina 2010

The Nobel prize in physiology or medicine has been awarded this year to Robert G. Edwards, an English biologist who with a physician colleague, Patrick Steptoe, developed the in vitro fertilization procedure for treating human infertility.
Since the birth of the first test tube baby, Louise Brown, on July 25, 1978, some four million babies worldwide have been conceived by mixing eggs and sperm outside the body and returning the embryo to the womb to resume the normal development. The procedure overcomes many previously untreatable causes of infertility and is used in 3 percent of all live births in developed countries.
Dr. Edwards, a physiologist who spent much of his career at Cambridge University in England, devoted more than 20 years to solving a series of problems in getting eggs and sperm to mature and successfully unite outside the body. His colleague, Dr. Steptoe, was a gynecologist and pioneer of laparoscopic surgery, the method used to extract eggs from the prospective mother.
Though in vitro fertilization is now widely accepted, the birth of the first test tube baby was greeted with intense concern that the moral order was subverted by unnatural intervention in the mysterious process of creating a human being. Dr. Edwards was well aware of the ethical issues raised by his research and took the lead in addressing them.
The objections gradually died away, except on the part of the Catholic church, as it became clear that the babies born by in vitro fertilization were healthy and that their parents were overjoyed to be able to start a family. Long-term follow-ups have confirmed the essential safety of the technique.

domingo, 3 de octubre de 2010

¿Un planeta con vida?

Astronomers Find Most Earth-like Planet to Date


Este es el descubrimiento científico de la semana: un planeta que "podría" presentar las condiciones imprescindibles para albergar vida. La distancia a su estrella, Gliese 581, podría dotarle de una temperatura superficial compatible con la existencia de agua líquida, mientras que su masa, 3 veces superior a la de la Tierra, generaría un campo gravitatorio suficiente para retener una atmósfera protectora. Aun así, las incógnitas son más que las certezas, después de todo, así es la ciencia.

Astronomers may have found the most Earth-like alien planet to date, and it's located only a short distance away, cosmically speaking. The team says that the planet's proximity to its sun, coupled with the ease with which it was detected, suggests that the galaxy could be teeming with habitable worlds.
Most of the 500 or so planets astronomers have found orbiting other stars have fallen into the gas-giant class: very large worlds, some much bigger than Jupiter, that can't support life, because they lack solid surfaces, and because they orbit either too far from or much too close to their suns. The few rocky worlds discovered so far also orbit too near or far from stars to fall into what planetary scientists call the "habitable zone," in which liquid water—and therefore life—could exist.
But Gliese 581g looks like a game-changer. Detected from the minuscule amount of gravitational influence it exerts on its star, the planet lives a mere 20 light-years away. Gliese 581g is the sixth world discovered around its sun—and the fourth most distant. Yet its orbit brings it closer to its parent star than Mercury is to our sun. Still, it's squarely within the habitable zone, because the planet's star, which is a type known as a red dwarf, contains only about 30% of the sun's mass and shines with only about 1% of its brightness, the researchers will report in an upcoming issue of the Astrophysical Journal.
That said, if Gliese 581g harbors any kind of life, the creatures would inhabit a world quite different from our own.  Just like our moon, the length of Gliese 581g's day precisely matches the length of its year. Consequently, the planet rotates so that it always shows the same face to its sun. Another difference is that the star casts Gliese 581g in a soft, red light that would give the appearance of a perpetual sunset.
On the other hand, the perpetual days or nights would mean that the planet could develop highly stable habitats. Although the most comfortable areas for humans would lie along the so-called terminator—the zone between the world's dayside and nightside—other creatures with preferences for hotter or colder temperatures could find tolerable conditions elsewhere on the surface.
The key is whether liquid water exists on the surface. The planet is about 3.1 times more massive than Earth—bulky enough to hold onto an atmosphere and to keep liquid water from evaporating into space. And on Earth, anywhere you find liquid water you have life.
Planetary scientist Jack Lissauer of NASA says: "It's a big breakthrough. Gliese 581g could be a big, rocky planet with oceans on its surface warmed by the faint but nearby red-dwarf star, or it could be a mini-Neptune, hosting a massive atmosphere above a surface that is far too hot for life as we know it. But however it turns out, the discovery promises even more exciting news in the near future."

viernes, 1 de octubre de 2010

INVITACIONES

Los 7 grupos que este curso formáis 1º de bachillerato B habéis recibido una invitación para publicar en este blog. Sólo tenéis que aceptarla y, a partir de ese momento, podréis aportar a este foro común todo lo que queráis. Parte será obligatorio: el resumen de vuestras exposiciones y vuestra propuesta de examen, pero otra parte es voluntaria y termina siendo vital para quienes aspiran a la mejor calificación posible. Ánimo a todos.

jueves, 23 de septiembre de 2010

UN NUEVO CURSO

Hoy estrenamos este blog. En una próxima entrada explicaremos el uso que queremos darle.