Bright, hot, blue main-sequence stars high mass are very rare. From Wordnik.com. [Learn: Identify constellations, stars, planets and how to navigate at night] Reference
Now we had five new main-sequence suns ahead within six months 'range. From Wordnik.com. [Greylorn] Reference
Low-mass star seeking main-sequence type for gravitational interaction. From Wordnik.com. [Archive 2006-01-01] Reference
IX Cerulia, being a main-sequence star, did not need vastly more mass than Sol to shine more fiercely. From Wordnik.com. [Agent Of The Terran Empire]
It is a typical main-sequence star and is by far the largest and most massive object in our Solar System. From Wordnik.com. [SciFi, Fantasy & Horror Collectibles - Part 1067] Reference
Telescopically, this main-sequence gem is dazzling white, tinged with blue and diffracts a rainbow of colors. From Wordnik.com. [Weekend SkyWatcher's Forecast: January 29-31, 2010 | Universe Today] Reference
The essence of it, Jake realized, was that almost fifteen hundred years ago—and 7,000 light-years from Earth—a main-sequence star had gone supernova. From Wordnik.com. [THE WAR OF THE PROPHETS] Reference
Yet there are signs that we may be looking at the brief, jubilant flare of the middle-age main-sequence star that is the culture of science as we know it today. From Wordnik.com. [Opening Night Celebration: Reaching into the Future] Reference
His sun is a fairly hot main-sequence star, of spectral class somewhere around F, and it's probably more or less variable, because there was quite a distinct implication of change. From Wordnik.com. [Children of the Lens]
Astronomers are not sure about the cause of its peculiar shape, but the current hypothesis is that the primary component of this binary is the hot core of a star that reached the end of its main-sequence life cycle, ejected most of its outer layers and then became a red giant, and is now contracting into a white dwarf. From Wordnik.com. ["X" Marks Puzzling Galactic Bulge | Universe Today] Reference
And if you want to cast that out as being perhaps incorrect, then you are casting out our entire present understanding of how stars evolve, which is derived only in very small part from those 20-30 yaars of observations, but in much larger part from our understanding of nuclear fusion reactions, and from observations of many, many, many main-sequence stars in the universe. From Wordnik.com. [A few inconvenient truths « Climate Audit] Reference
Greg, As with any main-sequence star, the Sun has gotten significantly brighter as it has aged. From Wordnik.com. [RealClimate] Reference
The Sun is a main-sequence star, and like all main-sequence stars it is slowly burning hotter as it ages. From Wordnik.com. [AMERICAN DIGEST] Reference
They are thought to derive from normal main-sequence stars that have undergone a recent increase in mass. From Wordnik.com. [Naturejobs - All Jobs] Reference
Moreover, these stars are rotating faster than normal main-sequence stars of the same surface temperatures. From Wordnik.com. [Naturejobs - All Jobs] Reference
We can't do experiments with supernovae or the geomagnetic field of main-sequence stars, and yet we have a pretty good idea how they work. From Wordnik.com. [RealClimate] Reference
One of the best ways to remedy this problem is to find resolved physical companions to the CSPN and measure their distances by photometric main-sequence fitting. From Wordnik.com. [SpaceRef Top Stories] Reference
Models of rotation in early-B stars predict that rotationally driven mixing should deplete surface boron abundances during the main-sequence lifetime of many stars. From Wordnik.com. [SpaceRef Top Stories] Reference
We propose to place the mass-loss scenario on a firm observational footing (or otherwise) by using WFC3 imaging to measure the main-sequence stellar mass functions of two of the lowest-mass lowest-concentration globular clusters in the. From Wordnik.com. [SpaceRef Top Stories] Reference
He knew from Diane's expression that there was no sound in the headphones except the frying noise all main-sequence stars give out, and the infrequent thumping noises that come from gas-giant planets 'lower atmospheres, and the Jansky-radiation hiss which comes from everywhere. From Wordnik.com. [The Aliens] Reference
Based on what we’ve seen most recently, and on data from the induction that followed the pursuit of Enterprise, Intrepid, and Bloodwing by the Romulans on the way out of Levaeri V, we’ve managed to cobble together some suggestions for protecting normal main-sequence stars from such inductions. From Wordnik.com. [Rihannsu: The Bloodwing Voyages] Reference
With a main-sequence star?. From Wordnik.com. [Reap the Whirlwind] Reference
This suggests that at least 1-3\% of main-sequence A and F stars - stars slightly hotter and larger than the Sun - have rocky planets, like Earth, "said Farihi. From Wordnik.com. [YubaNet.com] Reference
2) open cluster NGC 188 are currently in binary systems, a frequency three times that found among normal solar-type main-sequence stars. From Wordnik.com. [Naturejobs - All Jobs] Reference
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