«Spitzer allowed us to see really
faint objects so that we could do a census of all the star - forming regions out to 3,000 light - years.
«The discovery is telling us that galaxies as faint as this one exist, and we should continue looking for them and even
fainter objects so that we can understand how galaxies and the universe have evolved over time.»
Not exact matches
As our mental fields succeed one another, each has its centre of interest, around which the
objects of which we are less and less attentively conscious fade to a margin
so faint that its limits are unassignable.
Doing
so would make it possible to detect gravitational waves,
faint ripples in space - time that, according to Einstein, emanate from interactions between massive
objects like neutron stars and supermassive black holes.
Doing
so would make it possible to detect gravitational waves,
faint ripples in space - time that, according to Einstein, emanate from interactions between massive
objects such as neutron stars and supermassive black holes.
So Anita Cochran of the University of Texas and her colleagues turned to the Hubble telescope's Wide Field / Planetary Camera, which can spot much
fainter objects.
All of the thousands of brown dwarfs found
so far are relatively close to the Sun, the overwhelming majority within 1500 light years, simply because these
objects are
faint and therefore difficult to observe.
There are many smaller,
fainter brown dwarfs too,
so this could be a significant underestimate, and the survey confirms these dim
objects are ubiquitous.
One such
object, A1689 - zD1, is located in the box — although it is still
so faint that it is barely seen in this picture.
So Jewitt and Luu carried out two parallel surveys: they used the Palomar Observatory's Schmidt telescope equipped with conventional glass photographic plates to scan large areas of the sky for the very
faintest objects, while also watching a narrow field of view in the plane of the planets for rare but slightly brighter
objects using MIT's 1.3 - metre telescope fitted with a CCD.
Once more massive and brighter than Gacrux and
so burnt out much faster, it is now probably a few hundred times
fainter than Sol, with 0.6 to 1.4 times its mass and less than one percent of its diameter — a very dense
object at planetary size.
The stars in the stream are incredibly
faint,
so it was necessary to use a proxy technique to measure the speeds of brighter tracer
objects moving along with the stream stars.
A new analysis of galaxy colors, however, indicates that the farthest
objects in the deep fields must be extremely intense, unexpectedly bright knots of blue - white, hot newborn stars embedded in primordial proto - galaxies that are too
faint to be seen even by Hubble's far vision — as if only the lights on a distant Christmas tree were seen and
so one must infer the presence of the whole tree (more discussion at: STScI; and Lanzetta et al, 2002).
This is because many of the inner Oort cloud
objects are
so distant that even very large ones would be too
faint to detect with current technology,» says Sheppard.