Our new 'Word Of The Day' article update : abase , v :
(transitive) To lower, as in condition in life, office, rank, etc., so as to cause pain or hurt feelings; to degrade, to depress, to humble, to humiliate. (transitive, archaic) To lower physically; to depress; to cast or throw down; to stoop. (transitive, obsolete) To lower in value, in particular by altering the content of alloys in coins; to debase.
(transitive) To lower, as in condition in life, office, rank, etc., so as to cause pain or hurt feelings; to degrade, to depress, to humble, to humiliate. (transitive, archaic) To lower physically; to depress; to cast or throw down; to stoop. (transitive, obsolete) To lower in value, in particular by altering the content of alloys in coins; to debase.
The Strange Tale of the Most Obscure Joke a 90s Cartoon Ever Made via Digg https://ift.tt/2I3J4o3
Hello, Information from NASA Medical students from The University of Texas Health Sciences Center (UTHealth) in Houston will speak with an astronaut aboard the International Space Station next week.
September 21, 2018
from NASA https://ift.tt/2zmy5Du
September 21, 2018
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Astronomy news update from NASA : 
Irregular galaxy NGC 55 is thought to be similar to the Large Magellanic Cloud (LMC). But while the LMC is about 180,000 light-years away and is a well known satellite of our own Milky Way Galaxy, NGC 55 is more like 6 million light-years distant and is a member of the Sculptor Galaxy Group. Classified as an irregular galaxy, in deep exposures the LMC itself resembles a barred disk galaxy. Spanning about 50,000 light-years, NGC 55 is seen nearly edge-on though, presenting a flattened, narrow profile in contrast with our face-on view of the LMC. Just as large star forming regions create emission nebulae in the LMC, NGC 55 is also seen to be producing new stars. This highly detailed galaxy portrait highlights a bright core crossed with dust clouds, telltale pinkish star forming regions, and young blue star clusters in NGC 55.
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Irregular galaxy NGC 55 is thought to be similar to the Large Magellanic Cloud (LMC). But while the LMC is about 180,000 light-years away and is a well known satellite of our own Milky Way Galaxy, NGC 55 is more like 6 million light-years distant and is a member of the Sculptor Galaxy Group. Classified as an irregular galaxy, in deep exposures the LMC itself resembles a barred disk galaxy. Spanning about 50,000 light-years, NGC 55 is seen nearly edge-on though, presenting a flattened, narrow profile in contrast with our face-on view of the LMC. Just as large star forming regions create emission nebulae in the LMC, NGC 55 is also seen to be producing new stars. This highly detailed galaxy portrait highlights a bright core crossed with dust clouds, telltale pinkish star forming regions, and young blue star clusters in NGC 55.
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