Stars in the Milky Way appear to be missing some of the element lithium, and new
observations of a distant star cluster confirm that the problem isn't unique to our galaxy.
That's when telescope
observations of distant stars going behind Pluto (known as stellar occultations) showed that it had a methane atmosphere, probably rapidly evaporating to space.
Not exact matches
Observations of distant exploding
stars, or supernovas, indicated that the space between us and them was expanding at an increasing clip.
The space - warping quirks
of relativity that lead to deviations from Newton's earlier theory
of gravity only become obvious on very large scales, but our passive
observations of distant planets,
stars and galaxies have yet to deliver anything...
Some research has been done to deduce the chemical makeup
of very early galaxies, based on
observations of very bright,
distant galaxies, or
of very old
stars that formed in the early universe and are still around today, Hewitt said.
The new VLBA
observations, made in 2014 and 2015, measured a distance
of more than 66,000 light - years to a
star - forming region called G007.47 +00.05 on the opposite side
of the Milky Way from the Sun, well past the Galaxy's center, some 27,000 light - years
distant.
Discovering a planet requires confirmation
observations to distinguish a true planet orbiting the target
star from a
distant star that happens to sneak into GPI's field
of view — a process that could take years with previous instruments.
These
observations have the power
of penetrating through interstellar dust and so to unveil the
star formation processes in the very
distant, dusty galaxies, that constituted the progenitors
of local ellipticals.
Ultimately, Priest hopes IRIS
observations will bolster studies
of more
distant stars as well.
They are the locations
of bright
stars and other nearby objects that get in the way
of the
observations of more
distant galaxies and are hence masked out in these maps as no weak - lensing signal can be measured in these areas.
These glitches are apparent from astronomical
observations of occultations
of stars by the moon — miniature eclipses that occur when the moon passes in front
of the
distant star.
In the 1990s,
observations of exploding
stars showed that more
distant explosions were dimmer than existing theories predicted.
These first
observations indicated an object was very
distant and glowing brightly in infrared light, meaning that it was extremely dusty and likely going through a burst
of star formation.
Three years ago,
observations of distant, exploding
stars blew to smithereens some
of astronomers» most cherished ideas about the universe.
The results
of follow - up
observations (see Table 2) are a mixture
of results from photometric follow - up (Deeg et al. 2009), which identifies contaminating» diluted EB's that are more than about 2
distant from the third
star - which usually coincides with the observing target -, and from spectroscopic (radial velocity) results, which can only identify signals from sources that fall into the spectrograph's entry slit; that is, they have to be very close (less than 1 - 2) to the target.
u «Three years ago,
observations of distant, exploding
stars blew to smithereens some
of astronomers» most cherished ideas about the universe [the big bang theory].
Some astronomical
observations indicate that a principal source
of cosmic rays is Cygnus X-3, a
distant binary
star system near the edge
of our galaxy.
The famous telescope was named after U.S. astronomer Edwin Hubble, whose
observations of variable
stars in
distant galaxies confirmed that the universe was expanding and gave support to the Big Bang theory.
Unfortunately, however, no single SFR estimator is universally available or even applicable in all circumstances: the numerous galaxies found in deep surveys are often too faint (or too
distant) to yield significant detections with most standard SFR measures, and until now there have been no global, multi-band
observations of nearby galaxies that span all the conditions under which
star - formation is taking place.
Although previous
observations with ALMA have found supporting evidence around a low - mass protostar, there was little compelling evidence around massive protostars because most
of the massive -
star forming regions are rather
distant and difficult to investigate in detail.