Detecting a habitable planet is an enormous challenge due to the brightness of the planetary system's host star, which tends to overwhelm the relatively dim planets.
Not exact matches
Such gargantuan telescopes would build on the technologies now being developed by Breakthrough and other organizations, and would offer hope of
detecting biosignatures and other gases in
planets» atmospheres to reveal whether they are
habitable — or even inhabited.
A new find from NASA's Kepler orbiting observatory is the first Earth - sized
planet to be
detected in the
habitable zone of a star
The organization was designed to
detect potentially
habitable planets in our Milky Way galaxy.
The huge size of the E-ELT should allow METIS to
detect and study exoplanets the size of Mars orbiting Alpha Centauri, if they exist, as well as other potentially
habitable planets around other nearby stars.
The researchers set up a grid system for the Alpha Centauri system and asked, based on the spectrographic analysis, «If there was a small, rocky
planet in the
habitable zone, would we have been able to
detect it?»
The «
habitable zone» is the region around a star in which water on a
planet's surface is liquid and signs of life can be remotely
detected by telescopes.
The oldest
detected Kepler
planets (exoplanets found using NASA's Kepler telescope) are about 11 billion years old, and the planetary diversity suggests that around other stars, such initially frozen worlds could be the size of Earth and could even provide
habitable conditions once the star becomes older.
The findings have direct implications for future NASA missions, such as the Transiting Exoplanet Survey Satellite and James Webb Space Telescope, which will try to
detect possible
habitable planets and characterize their atmospheres.
Several Earth - like
planets and super-Earths have been
detected in the
habitable zones of their host stars and more than 2300 planetary candidates have been announced.
Recent simulations suggest that an Earth - life
planet could have formed within the
habitable zone around Alpha Centauri B, which can be
detected using the radial - velocity «wobble» method (more).
Had Kepler survived for an extended mission, it would have obtained enough data to directly
detect a handful of Earth - size
planets in the
habitable zones of G - type stars.
Star B was chosen for analysis because efforts are underway to
detect of an Earth - like
planet in or near its
habitable zone (between 0.5 and 0.9 AU) using available technology — more discussion below (Xie et al, 2010; and Jessica Griggs, New Scientist, January 29, 2010).
We are entering a scientific era in which we have the capability to
detect not only giant
planets the size of Jupiter, but Earth - sized
planets in the
habitable zones of their solar systems, the locations where liquid water can exist.
[106] Theoretical studies on the detectability via radial velocity analysis have shown that a dedicated campaign of high - cadence observations with a 1 - meter class telescope can reliably
detect a hypothetical
planet of 1.8 M ⊕ in the
habitable zone of B within three years.
Abstract: The Kepler Mission, launched on Mar 6, 2009 was designed with the explicit capability to
detect Earth - size
planets in the
habitable zone of solar - like stars using the transit photometry method.
Many as... ▽ More The Kepler Mission, launched on Mar 6, 2009 was designed with the explicit capability to
detect Earth - size
planets in the
habitable zone of solar - like stars using the transit photometry method.
Two distinct sets of transit events were
detected: 1) a 152 + / - 4 ppm dimming lasting 1.811 + / - 0.024 hours with ephemeris T [BJD] = 2454964.57375 + N... ▽ More NASA's Kepler Mission uses transit photometry to determine the frequency of earth - size
planets in or near the
habitable zone of Sun - like stars.
Abstract: We present the design concept of the wavelength calibration system for the
Habitable - zone
Planet Finder instrument (HPF), a precision radial velocity (RV) spectrograph designed to
detect terrestrial - mass
planets around M - dwarfs.
I'm pretty darn sure that long before 50 years from now Kepler or some other mission will have
detected earth - size
planets in the
habitable zones of their stars and we will have been able to look remotely for biosignatures.
Three, possibly four, super-Earths have been
detected in the
habitable zone around Star C (more), view of daytime sky from
planet «d» as imagined by Kormmesser.
However, our exoplanet surveys have only just begun to
detect enough
habitable zone
planets to attempt this type of analysis, and our understanding of stellar metallicity and
planet formation is still too limited to make any firm conclusions.
However, the telescope will explore a much larger region of the sky than Kepler, with an emphasis on
detecting rocky
planets on Earth - like orbits that receive a similar amount of radiation as our own
planet (the so - called
habitable zone).
Three - dimensional (3D) planetary general circulation models (GCMs) derived from the models that we use to project 21st Century changes in Earth's climate can now be used to address outstanding questions about how Earth became and remained
habitable despite wide swings in solar radiation, atmospheric chemistry, and other climate forcings; whether these different eras of habitability manifest themselves in signals that might be
detected from a great distance; whether and how
planets such as Mars and Venus were
habitable in the past; how common
habitable exoplanets might be; and how we might best answer this question with future observations.