Checking on the Neighbors: Searching for Planets around Alpha Centauri

The alpha Centauri system - our next door neighbor in space - represents a very attractive target for exoplanet searches. Owing to its proximity, a planet found around any of the three stars in the system would be an ideal target for detailed follow-up studies with next generation ground- and space-based telescopes. In this talk Dr Endl will review past and current planet search efforts that targeted the alpha Centauri system. He will focus on his team's program, an intensive multi-year observing campaign carried out at Mt John University Observatory in New Zealand.

Are Old Galaxies Really Red and Dead?

Galaxies are broadly divided into two classes: spiral and elliptical. Unlike the spirals, the ellipticals, often referred to as early-type galaxies, are largely composed of old stars that give them a reddish color, They typically have little interstellar material with which to form new stars; these galaxies are often referred to as “red and dead.” We will see, however, that a substantial fraction of these galaxies contain surprising amounts of neutral hydrogen and these do form stars, albeit at a reduced rate compared to their spiral cousins.

Astrochemistry: putting the astro in astrobiology

Astrobiology, the study of emergence of life and the its distribution in the Universe, addresses the most fundamental questions in science: "How does life begin ?" and "Are we alone ?" Over the last 20 years, we have discovered that planets are bountiful in the galaxy and that one in every five solar-type stars has a planet in the habitable zone. We have learned that extremophiles have spread to essential every niche – even the seemingly most inhospitable ones – on our planet.

Earth-Sized Planets in the Habitable Zones of Cool Stars

illustration of surface of Kepler-186fAbstract: A primary goal of the Kepler mission is to determine the frequency of Earth-sized planets in the habitable zones of other stars. M dwarfs, stars that are smaller and cooler than the Sun, comprise more than 70% of the stars in our galaxy. Finding that Earth-sized planets around M dwarfs are common, therefore, has big implications for determining the frequency of other Earths.

Why SuperEarths are not Earthlike

Kepler data indicate that there are many planets that could be Earthlike in the sense of having a similar bulk composition. I will explain why such planets are unlikely to be Earthlike in other respects, especially if they are superEarths (three or so Earth masses or more). There are three main points here: (1) SuperEarths will not separate core from mantle because they are likely to be so hot internally that the critical temperature is reached for miscibility of iron alloy and silicate material.

Every Body is an Ark: How the microorganisms we carry will impact long term space travel

germsThe human microbiome is essential to our health and deserves special consideration in the closed environments of space travel. The dynamics of host-microbe interactions will change if normal immune functions are altered during extended space travel. Opportunistic pathogens common in the human microbiome, including those in the genera Candida, Aspergillus, and Staphylococcus, could spread among crewmembers and put them at risk of serious disease.

Refactoring Space Exploration with Soft Machines

T12 robotTo understand how we control motion, we need to understand the physical mechanism being moved. Emerging theories of vertebrate physiology are overturning the traditional bone-centric model of the body in favor of a "tensegrity" model, in which the primary load paths are in the continuous tension network of the soft tissues.

Life before genetics: autogenesis, information, and the outer solar system

moon of giant gas planetThe investigation of the origins of life has been hindered by what we think we know about current living organisms. This includes three assumptions about necessary conditions: 1) that it emerged entirely on Earth, 2) that it is dependent on the availability of liquid water, and 3) that it is coextensive with the emergence of molecules able to replicate themselves.


Subscribe to RSS - Astrobiology