so.. this is my field, me being an astrophysicist.
It's interesting news, but nowadays we get this sort of discoveries quite "often".
There are billions (of billions) of planets out there, and surely on at least one of them there is some form of life.
However, the public tends to get very excited about those exoplanets; more than they should.
Although they are an important discovery and represent a tiny step forward in the understanding of the Universe and its dynamics, the probability that organisms that will communicate to us (or try) will be found is close to zero.
If we do find life, which is undoubtely there somewhere, it will almost surely be just "boring" bacteria.
I say "boring" because they would be boring for the public, because they are not green beings that drive spaceships that travel faster than the speed of light, but they will be the most interesting thing ever for biologists.
Just imagine.. bacteria formed in a different galaxy (or maybe still the Milky Way), in a different solar system, with a different star shining upon the planet, with a different atmosphere to which they had to adapt and maybe also adapted to some other property of the planet still unknown to us.. 
On a similar note, did life on earth have to adapt the environment, did that bacteria or even something pre-bacterial have to process the watermasses and atmosphere before it could evolve past a certain point?
Yes!
First Atmosphere
* Composition - Probably H2, He
* These gases are relatively rare on Earth compared to other places in the universe and were probably lost to space early in Earth's history because
o Earth's gravity is not strong enough to hold lighter gases
o Earth still did not have a differentiated core (solid inner/liquid outer core) which creates Earth's magnetic field (magnetosphere = Van Allen Belt) which deflects solar winds.
* Once the core differentiated the heavier gases could be retained
Second Atmosphere
Produced by volcanic out gassing.
* Gases produced were probably similar to those created by modern volcanoes (H2O, CO2, SO2, CO, S2, Cl2, N2, H2) and NH3 (ammonia) and CH4 (methane)
* No free O2 at this time (not found in volcanic gases).
* Ocean Formation - As the Earth cooled, H2O produced by out gassing could exist as liquid in the Early Archean, allowing oceans to form.
o Evidence - pillow basalts, deep marine seds in greenstone belts.
Addition of O2 to the Atmosphere
Today, the atmosphere is ~21% free oxygen. How did oxygen reach these levels in the atmosphere?
* Oxygen Production
o Photochemical dissociation - breakup of water molecules by ultraviolet
+ Produced O2 levels approx. 1-2% current levels
+ At these levels O3 (Ozone) can form to shield Earth surface from UV
o Photosynthesis - CO2 + H2O + sunlight = organic compounds + O2 - produced by cyanobacteria, and eventually higher plants - supplied the rest of O2 to atmosphere. Thus plant populations
* Oxygen Consumers
o Chemical Weathering - through oxidation of surface materials (early consumer)
o Animal Respiration (much later)
o Burning of Fossil Fuels (much, much later)
Throughout the Archean there was little to no free oxygen in the atmosphere (<1% of presence levels). What little was produced by cyanobacteria, was probably consumed by the weathering process. Once rocks at the surface were sufficiently oxidized, more oxygen could remain free in the atmosphere.
During the Proterozoic the amount of free O2 in the atmosphere rose from 1 - 10 %. Most of this was released by cyanobacteria, which increase in abundance in the fossil record 2.3 Ga. Present levels of O2 were probably not achieved until ~400 Ma.
Evidence from the Rock Record
* Iron (Fe) i s extremely reactive with oxygen. If we look at the oxidation state of Fe in the rock record, we can infer a great deal about atmospheric evolution.
* Archean - Find occurrence of minerals that only form in non-oxidizing environments in Archean sediments: Pyrite (Fools gold; FeS2), Uraninite (UO2). These minerals are easily dissolved out of rocks under present atmospheric conditions.
* Banded Iron Formation (BIF) - Deep water deposits in which layers of iron-rich minerals alternate with iron-poor layers, primarily chert. Iron minerals include iron oxide, iron carbonate, iron silicate, iron sulfide. BIF's are a major source of iron ore, b/c they contain magnetite (Fe3O4) which has a higher iron-to-oxygen ratio than hematite. These are common in rocks 2.0 - 2.8 B.y. old, but do not form today.
* Red beds (continental siliciclastic deposits) are never found in rocks older than 2.3 B. y., but are common during Phanerozoic time. Red beds are red because of the highly oxidized mineral hematite (Fe2O3), that probably forms secondarily by oxidation of other Fe minerals that have accumulated in the sediment.
Conclusion - amount of O2 in the atmosphere has increased with time.
Biological Evidence
* Chemical building blocks of life could not have formed in the presence of atmospheric oxygen. Chemical reactions that yield amino acids are inhibited by presence of very small amounts of oxygen.
* Oxygen prevents growth of the most primitive living bacteria such as photosynthetic bacteria, methane-producing bacteria and bacteria that derive energy from fermentation. Conclustion - Since today's most primitive life forms are anaerobic, the first forms of cellular life probably had similar metabolisms.
* Today these anaerobic life forms are restricted to anoxic (low oxygen) habitats such as swamps, ponds, and lagoons.