That survey will image the entire visible sky every few nights, gathering data on billions of stars and how some of
those stars change in brightness over time.
Not exact matches
If a planet is indeed the cause of the
change in brightness, the exact same
change should recur days, months, or years later, depending on how long the planet takes to orbit its
star.
At this stage some
stars become luminous blue variables, so called because they go through episodic
changes in brightness, including brilliant outbursts that look a lot like supernovae.
Seventeenth - century astronomers marveled at the
star Mira A, or Omicron Ceti, for its dramatic
changes in brightness every 332 days.
The
change in the burst's
brightness appears to be exactly the same at radio and optical frequencies; this can happen, say Garnavich and his collaborators Avi Loeb and Kris Stanek from the Center for Astrophysics
in Cambridge, Massachusetts, only if part of the expanding ring passed behind a
star located exactly between Earth and the ring itself.
Giammichele and her colleagues used data from NASA's Kepler space telescope, which watched
stars unblinkingly to track periodic
changes in their
brightness.
Mira, a similar but more extreme
star in the constellation Cetus (low
in the west at nightfall this month), can
change in brightness by a factor of 1,500.
«If the
change in brightness was intrinsic to the
star, then its temperature or surface area would have grown dramatically,» says Cook.
«An important next step will be to determine how the color of the
star changes with time, especially during its brief dips
in brightness,» added Shappee.
It's a basic bias
in transiting exoplanet surveys: Larger objects will produce larger
changes in a
star's
brightness, so Kepler is more likely to detect big planets or moons.Another bias is planets with shorter orbits.
Kepler watches for the slight
change in the
brightness of a
star when an exoplanet passes
in front of it, an event called a transit.
Stars do
change in brightness when they begin to exhaust the fuel supply
in their core.
And the 1981 observations were made
in several colours, all of which showed the same pattern of
change — which rules out fluctuation
in the
star's intrinsic
brightness, as this would vary with colour.
That smeared out any short - term
changes in the
star's
brightness — such as a bright flare.
One method involves measuring the
changes in a
star's
brightness that result from the gravitational effects of a primordial black hole passing between Earth and that
star.
Distances for these types of
stars can be effectively determined by following the periodic
changes in their
brightness and spectra.
Such
stars are rich
in carbon, and it is believed that the fall
in brightness is due to the
star's emission of carbon, which then condenses to a dense cloud near the
star, rather than to a
change in luminosity of the
star itself.
These are processed through pipeline software (the modern equivalent of the old «human computer» room) resulting
in huge databases of the
changes in brightnesses of hundreds of millions of
stars.
MOST can see
changes in the
brightness of the
star, or the planet associated with it, down to levels of one part
in a million: that's one ten thousandth of a percent.
The object's core, near the orbiting pair of
stars, showed
changes in the
brightness of its radio emission.
Serpens is one of several
star - forming regions targeted by the Young Stellar Object Variability (YSOVAR) project, which conducted repeated observations
in each area to look for
changes in brightness in the baby
stars.
http://www.agci.org/docs/lean.pdf «Global (and regional) surface temperature fluctuations
in the past 120 years reflect, as
in the space era, a combination of solar, volcanic, ENSO, and anthropogenic influences, with relative contributions shown
in Figure 6.22 The adopted solar
brightness changes in this scenario are based on a solar surface flux transport model; although long - term
changes are «50 % larger than the 11 - year irradiance cycle, they are significantly smaller than the original estimates based on variations
in Sun - like
stars and geomagnetic activity.