Dr Jeffrey Simpson of the AAO said it takes about an hour to collect
enough photons of light for each star, but «Thankfully, we can observe 360 stars at the same time using fibre optics,» he added.
Not exact matches
4) then
photons erupted from this energy 4) let there be
LIGHT (1 - 4 all the first day) cloud (detectable today as the microwave background radiation) 5)
photons and other particles form the 5) God next creates the heavens (what we call the sky) above bodies
of the early universe (atoms, (2nd day) molecules, stars, planets, galaxies) 6) it rained on the early earth until it was 6) dry land appears as the oceans form (3rd day) cool
enough for oceans to form 7) the first life form was blue green bacteria.
If even a small amount
of energy from phonons (the sound units that carry the energy through the germanium or silicon, much as
photons are the units
of light) hit the detector, it can be
enough to make the device lose superconductivity and register a potential dark matter event through a device called a superconducting quantum interference device, or SQUID.
It pumps 20 liters (about 5.3 gallons)
of seawater and plankton per second through a «
light tight» collection chamber large
enough to capture even fast swimmers and keep them inside long
enough for the device's fiber - optic instruments to record and measure, in
photons per liter, the size, duration, and number
of an organism's flashes.
She assembles sensors keen
enough to detect a single
photon of light.
«You need a lot
of silicon to stop all
of the
photons, but you can't have
enough silicon in the line
of sight to absorb all
of the
light.»
A team
of researchers has built an array
of light detectors sensitive
enough to register the arrival
of individual
light particles, or
photons, and mounted them on a silicon optical chip.
In five minutes, the scope collected a mere 11
photons of light from the glow — tiny but
enough for Swift's sensitive instruments to track the detonation with accuracy.
The ripples are so large that by the time the
photons detected by COBE were emitted, the Universe was simply not old
enough for a
light signal to have crossed from one side
of a COBE ripple to the other.
«In really dim
light, our cones don't receive
enough photons to work, but they continue to emit a low - level baseline signal to the rest
of the retina that is independent
of light,» he explains.
Green -
light photons hold 240 kJ / mole
of energy, which is
enough to bend (but not break) the rhodopsin molecules in our retinas that trigger our photosensitive rod cells to fire.
Deborah Jackson, a senior member
of the quantum computing technologies group at the Jet Propulsion Laboratory (JPL) in Pasadena, California, assembles sensors keen
enough to detect a single
photon of light.
Within that plane,
photons are so concentrated that they interact with the dye in pairs, each
of which has
enough energy to
light up the dye molecules.