NGC 4,654 is a spiral galaxy with some interesting nuances of stellar formation.
Have you seen an unusually bright object moving through the evening sky recently?
Chances are that it wasn’t one of the mysterious objects that the DoD and NASA are currently studying, but was instead one of the growing number of manmade spacecraft taking up residence in Earth’s orbit.
And this one has astronomers particularly concerned.
The Vela pulsar has claimed the record for emitting the most powerful gamma rays among all known pulsars.
A corpse of a dead star has been found to be emanating the most intense gamma rays ever observed. This unexpected observation was found coming from the Vela pulsar, situated in the constellation Vela.
Astronomers noted that the detected gamma rays had an astonishing energy level of 20 tera-electronvolts (TeV), which is ten trillion times higher than the energy of visible light.
Science Communication Lab for DESY
This unexpected observation was found coming from the Vela pulsar, situated in the constellation Vela.
After decades of searching, scientists have found stars accompanying the gas streaming from two smaller galaxies that orbit our Milky Way.
Our galaxy is so big that astronomers are still exploring its stellar backwaters. Now, new observations have enabled them to map a previously uncharted structure in the Milky Way.
Scientists have found 13 stars that they believe are associated with the Magellanic Stream — a giant ribbon of gas stretching over three-quarters of the way across the sky. The researchers presented their findings on the arXiv astronomy preprint server in June.
The first asteroid sample collected in space by a U.S. spacecraft and brought to Earth is unveiled to the world at NASA’s Johnson Space Center in Houston on…
NASA has issued a request for “lunar freezer” designs that can safely store materials taken from the moon during planned Artemis missions.
According to a request for information (RFI) posted to the federal contracting website SAM.gov, the freezer’s primary use will be transporting scientific and geological samples from the moon to Earth. These samples, the post specifies, will be ones collected during the Artemis program.
Astronomers from the Binary Systems of South and North (BSN) project have conducted photometric observations of a distant binary star known as V0610 Virgo. Results of the observation campaign, published Sept. 23 in a research paper on the pre-print server arXiv, indicate that V0610 Virgo is a low-mass contact binary system.
W Ursae Majoris-type, or W UMa-type binaries (EWs) are eclipsing binaries with a short orbital period (below one day) and continuous light variation during a cycle. They are also known as “contact binaries,” given that these systems are composed of two dwarf stars with similar temperature and luminosity, sharing a common envelope of material and are thus in contact with one another. In general, studies of contact binaries have the potential to reveal many details about the evolution of stars.
Located some 1,560 light years away from the Earth, V0610 Virgo is an EW with an apparent magnitude of 13.3 mag. Although not much is known about this system, previous observations have found that it has an orbital period of approximately eight hours.