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The Rotation of Venus

Submitted by idfive on
Venus is covered in a thick layer of clouds, one reason that it appears so bright in the sky. Ancient astronomers had a good idea of what (since Copernicus) we know as its orbital period;...

The Nature of Obscured Active Galactic Nuclei

Submitted by idfive on
Most galaxies host a supermassive black hole (SMBH) at their nucleus, one whose mass exceeds a million solar-masses. When material actively accretes onto the SMBH, associated processes ca...

The Hot X-Ray Gas in Giant Elliptical Galaxies

Submitted by idfive on
The oldest known large galactic structures in the universe are giant elliptical galaxies. Unlike our Milky Way and other spiral galaxies, elliptical galaxies have no spiral arms and littl...

Heating the Solar Corona

Submitted by idfive on
The hot outer layer of the sun, the corona, has a temperature of over a million degrees Kelvin, much more than the surface temperature of the Sun which is only about 5500 degrees Kelvin. ...

Bright Galaxy Clusters in the Era of Peak Star Formation

Submitted by idfive on
Galaxies actively engaged in making stars produce many hot massive stars that emit copious amounts of uv radiation. The neutral hydrogen gas in these galaxies (or in the intervening inter...

The Galaxy Cluster Abell 959

Submitted by idfive on
Most galaxies lie in clusters containing from a few to thousands of objects. Our Milky Way, for example, belongs to the Local Group, a cluster of about fifty galaxies whose other large me...

Photosynthesis on Habitable Planets Around Low-Mass Stars

Submitted by idfive on
Life on Earth is dominated by photosynthesis, the process by which green plants and some organisms use sunlight at visible wavelengths to synthesize carbon-based nutrients from carbon dio...
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