PlutonianEmpire wrote:....NGC 5195...
It's there, it's just that they got the distance wrong. it's a lot closer than it should be.
danielj wrote:I thought that NGC 5194 and NGC 5195 was interacting,as seen in the Jim??s texture
Now friends,
let me explain in some detail why both your statements are untenable from a more scientific point of view:
First of all, I challenge you to check carefully all existing measurements about M 51 and NGC 5195, as summarized in Simbad.
The closest is a note about NGC 5195 from 2004, saying:
Simbad wrote:possible companion of NGC 5194
But clearly even the most hires imaging taken from EARTH is intrinsically
2d and
perspective can play all sorts of deceptive games. Apparently the phtographic signatures for the two galaxies being in INTERACTION are suggestive, perhaps even probable, but NOT proven. That's why the official statement in Simbad above is sufficiently careful, despite being recent!
Next, a word about all catalog data that I prepare for Celestia: Being a professional scientist myself, with a thorough understanding of the meaning of
measurement uncertainties, I shall NOWHERE impose personal prejudice. Rather my presented data have to be interpreted as
unmodiified, scientifically published data, in genera,l with unavoidable and
often appreciable measurement uncertainties!
Another important remark has to be made, concerning the value of the
Hubble constant, which has been notoriously uncertain.
Only very recently, we have a VERY accurate value from the WMAP experiment about the cosmic microwave background radiation. That value often differs significantly from the earlier values used in the distance analyses of galaxies.
NOTE:The finally quoted distance values are DIRECTLY proportional to the value of the Hubble constant! It sets the basic distance scale.
I have used the accurate WMAP value throughout, which you have of course to fold in when you compare with other sources!
I have used in my latest deepsky.dsc about the most accurate DIRECT and independent distance measurements of M 51 and NGC 5195:
Code: Select all
M 51 (=NGC 5194): 2.89 10^7 ly (recession velocity in CMB frame)
NGC 5195 : 2.50 10^7 ly (SBF method, accurate!)
-------------------------------------
Now let me tell you, how these distance data MUST be interpreted.
Most optimistically, each of these two measurements has an >= 10% uncertainty attached to its center value, i.e we should better write
Code: Select all
M 51 (=NGC 5194): (2.89 +- 0.29) 10^7 ly
NGC 5195 : (2.50 +- 0.25 )10^7 ly
with average distance being <d> = 2.7 10^7 ly
Clearly, allowing youself to add and subtract the >= 10% uncertainty, the measured distance values are
perfectly compatible with NGC 5194 and NGC 5195 being VERY close-by compagnions at an distance around 2.7 10^7 ly. But they may be also quite a bit further apart with the same probability!
Please: Neither JIM nor any of the superficial science writers that many of you often consult on the WEB, have any more solid knowledge about that issue! If there is any other SERIOUS and MORE accurate source for the distances of these two galaxies of which I am unaware, please let me know!
In any case I hope I managed to illustrate that the issue is much more complex than just stating that I got the distance WRONG
or that something is "seen in JIM's texture" .
Bye Fridger