A MAGNETIC disturbance has been directly observed
on a brown dwarf for the first time.
Not exact matches
I studied
brown dwarfs for a while when I was working
on Hubble; at the time we didn't know much about them but I found them fascinating.
Adding up all the dark forms of ordinary matter (gas clouds,
brown dwarfs, black holes, and so
on) still leaves 95 percent of the mass in the universe unaccounted
for.
In the 1980s,
for example, researchers proposed that an unseen
brown dwarf star could cause periodic extinctions
on Earth by triggering fusillades of comets.
«
Brown dwarfs are strikingly similar to Jupiter so we study their atmospheres in order to look at what weather
on other worlds might look like,» said Jonathan Gagné, a Backyard Worlds team member from the Carnegie Institution
for Science.
For the moment, data on brown dwarfs can be used as a stand - in for contemplating extrasolar worlds we hope to study with future instruments like the James Webb Space Telesco
For the moment, data
on brown dwarfs can be used as a stand - in
for contemplating extrasolar worlds we hope to study with future instruments like the James Webb Space Telesco
for contemplating extrasolar worlds we hope to study with future instruments like the James Webb Space Telescope.
Although the nature of the electromagnetic engine powering
brown -
dwarf aurorae is still to be determined, the scenario of the subcorotation of magnetospheric plasma
on closed field lines, powering in turn magnetosphere - ionosphere coupling currents, has been suggested as a plausible model
for this case (Schrijver 2009; Nichols et al. 2012).
For more information
on Sedna and other
dwarf planets check out Mike
Brown's
dwarf planet website.
We present here our search methods and spectroscopic follow - up of our high - priority c... ▽ More We are conducting a proper - motion survey
for young
brown dwarfs in the Taurus - Auriga molecular cloud based
on the Pan-STARRS1 3 $ \ pi $ Survey.
For more information
on the known
dwarf planets in the Kuiper belt check out my thesis advisor Mike
Brown's
dwarf planet website.
In 2010, a new study (which included better model atmosphere fitting) argued that the system is around six billion years old, even older than estimates of 3.7 to 4.3 billion years derived from a 2009 study based
on mass and evolutionary models
for the two
brown dwarf companions Ba and Bb (Liu et al, 2010; and King et al, 2009), which are much older than an earlier age estimate of between 0.8 and 2.0 billion years based
on the star's rotational speed (press release; Scholz et al, 2003; and Lachaume et al, 1999).
They find that much depends
on how we set limits
on the habitable zone, but in general habitability durations of a billion years are possible
for planets within 2 - 3 Roche radii
for brown dwarfs above 0.03 solar masses.
Note: Special thanks to Ken Croswell
on studies revising previous estimates of the system's age based
on analyses of its
brown dwarf companions and to Mike Stevens
for notifying us of the discovery of Epsilon Indi bb.
Using the revised stellar properties, we recalculate the radii
for 107 planet candidates in our sample, and comment
on candidates
for which the radii change from a previously giant - planet /
brown -
dwarf / stellar regime to a sub-Jupiter size, or vice versa.
DID N'T LIKE: Thorin's attitude, the rudeness of the
dwarves when they first entered the house, Bilbo's leaving
on his own (Gandalf didn't come back
for him), Radagast the
Brown (too goofy, I always pictured a more St. Francis - like character), the way the scene at the end - with Gandalf and the
dwarves up in the trees, was totally ruined, and the loss of Bilbo's progression as a character (did he really kill several creatures all ready?