From: rabid_fan on
In contrast to the useless spectacle that will be any manned
flight to the moon or Mars, NASA is considering a sound investment
in fundamental science:

http://www.physorg.com/news191777544.html

From: bert on
On Apr 29, 10:59 pm, rabid_fan <r...(a)righthere.net> wrote:
> In contrast to the useless spectacle that will be any manned
> flight to the moon or Mars, NASA is considering a sound investment
> in fundamental science:
>
> http://www.physorg.com/news191777544.html

Mafia NASA spent $25,000,000 on each ot the shuttles toilets(5) They
stole billions and billions so reality is the toilets were dirt cheap.
Best to keep in mind you have to go even in free fall. High cost to
these toilets they had a diode so flushing was automatic. O ya
Depends would have been a lot cheaper. TreBert
From: Uncle Al on
rabid_fan wrote:
>
> In contrast to the useless spectacle that will be any manned
> flight to the moon or Mars, NASA is considering a sound investment
> in fundamental science:
>
> http://www.physorg.com/news191777544.html

First, that's hype. Second, NASA is a disaster. Third, how much
additional resolution can be achieved with a third generation CMB
detector? An evolutionary platform will not suck in more
information. A revoltionary platform cannot be justified in a
business plan for lack of precedent.

--
Uncle Al
http://www.mazepath.com/uncleal/
(Toxic URL! Unsafe for children and most mammals)
http://www.mazepath.com/uncleal/qz4.htm
From: rabid_fan on
On Fri, 30 Apr 2010 07:48:47 -0700, Uncle Al wrote:

> Third, how much
> additional resolution can be achieved with a third generation CMB
> detector?

Increased sensitivity (temperature) and resolution (angular) are
not the goals of these CMB detectors. They are designed to detect
the polarization of the microwave background in the hope of detecting
patterns that are consistent with the inflation theory.

> An evolutionary platform will not suck in more information.

These detectors are evolutionary (aka progressive). COBE and WMAP
provided initial results on the polarization of the CMB. These
new detectors (CLASS and PIPER) will explore the polarization
further.