I found this star in the new Software from ESA, the GAIASKY program that recently has been made available. The spectrum was PINK and unlike other stars, the program shows the star as being pink with some wave functions around it, as though there was some LENS function , could be that the PINK stars are the smallest versions of GALACTIC DISCS.
It's the latest data from billions of stars in the milky way, so it should be right. I made an artistic impression of it.
article by Henryk Szubinski.
It's the latest data from billions of stars in the milky way, so it should be right. I made an artistic impression of it.
article by Henryk Szubinski.
Probably one of the few examples in our Milky Way galaxy of PINK STARS.
http://inis.jinr.ru/sl/tcaep/astro/constell/19260119.htm
date 2018
April 30
time, 13:43
Astronomy
Constellations - Aquila - 32nu Aql
Identification Data
Common Name
ConstellationAquila
Star Name32nu Aql
Skymap Number19260119
Henry Draper (HD) Number182835
Harvard Revised (HR) Number7387
SAO Number124628
Durchmusterung (DM) NumberBD+00 4206
Washington Double Stars (WDS) Number
19265+0020
Positional Data
Position and Proper Motion (PPM) Number167857
Right Ascension (RA) J200019h 26m 31.089s
Declination (Dec) J2000+0° 20' 18.852"
Position Uncertainty0.0072s
Proper Motion in RA (J2000)/cos(Dec)-0.00006
Proper Motion in Dec (J2000)-0.002366
Radial Velocity-001.0km s-1
Trigonometric Parallax+0.00028s
Trigonometric Parallax Uncertainty0.00087s
GCI Unit Vector in X (J2000)0.368597
GCI Unit Vector in Y (J2000)-0.929570
GCI Unit Vector in Z (J2000)0.005909
Galactic Longitude37.26°
Galactic Latitude
-7.64°
Observational Data
Observed Visual Magnitude (V)4.68
Derived Visual Magnitude
Derived Visual Magnitude or Observed Visual Magnitude Uncertainty0.002
Observed B Magnitude5.24
Observed B-V Colour+0.561
Observed B Magnitude or (B-V) Magnitude Uncertainty0.003
Observed U Magnitude
Observed U-B Colour
Observed U Magnitude or (U-B) Magnitude Uncertainty
Observed Photovisual Magnitude4.9
Observed Photographic Magnitude5.2
Morgan Keenan (MK) Spectral TypeF2Ib
One-Dimensional Spectral ClassF0
Position Angle288
Year of Observation1912. AD
Data Source
SKY2000 - Master Star Catalog - Star Catalog Database, Version 2
Sande C.B., Warren Jr. W.H., Tracewell D.A., Home A.T., Miller A.C.
(Goddard Space Flight Center, Flight Dynamics Division (1998))
Page compiled: Sun Sep 02 13:15:32 GMT+01:00 2001
Example of the "WHIRLPOOL" galaxy and it's pink spectrum as the collective point focus of the galactic lenses of the billions of galaxies, each having a small number of pink stars. The ability of pink to be the RED SHIFT but also the WHITE SHIFT , means that the LENSES in SPACE are WHITE, while the LENSES may be RED so that the resulting PINK as the mix between RED+WHITE=PINK, as the motion ability of GALACTIC LENSES to DISPLACE around the UNIVERSE at higher speeds and as the FOCUS function of the LENSES in MOTION.
The only lenses in motion would be the STAR SIZED ONES. The fact of LENSES being on the move as REAL AS IT GETS with the LENS being the size of the STAR CIRCUMFERENCE and may be SOURCE related to the center of the galaxy on their way out of the center disc or into it to fuel the larger WHOLE GALAXY.
So then, the image of the WHIRLPOOL GALAXY as having many positions of PINK STAR LENSES that are being COLLECTED together in the many positions seen in the galaxy as the small PINK STAR SIZE LENSES.
http://inis.jinr.ru/sl/tcaep/astro/constell/19260119.htm
date 2018
April 30
time, 13:43
Astronomy
Constellations - Aquila - 32nu Aql
Identification Data
Common Name
ConstellationAquila
Star Name32nu Aql
Skymap Number19260119
Henry Draper (HD) Number182835
Harvard Revised (HR) Number7387
SAO Number124628
Durchmusterung (DM) NumberBD+00 4206
Washington Double Stars (WDS) Number
19265+0020
Positional Data
Position and Proper Motion (PPM) Number167857
Right Ascension (RA) J200019h 26m 31.089s
Declination (Dec) J2000+0° 20' 18.852"
Position Uncertainty0.0072s
Proper Motion in RA (J2000)/cos(Dec)-0.00006
Proper Motion in Dec (J2000)-0.002366
Radial Velocity-001.0km s-1
Trigonometric Parallax+0.00028s
Trigonometric Parallax Uncertainty0.00087s
GCI Unit Vector in X (J2000)0.368597
GCI Unit Vector in Y (J2000)-0.929570
GCI Unit Vector in Z (J2000)0.005909
Galactic Longitude37.26°
Galactic Latitude
-7.64°
Observational Data
Observed Visual Magnitude (V)4.68
Derived Visual Magnitude
Derived Visual Magnitude or Observed Visual Magnitude Uncertainty0.002
Observed B Magnitude5.24
Observed B-V Colour+0.561
Observed B Magnitude or (B-V) Magnitude Uncertainty0.003
Observed U Magnitude
Observed U-B Colour
Observed U Magnitude or (U-B) Magnitude Uncertainty
Observed Photovisual Magnitude4.9
Observed Photographic Magnitude5.2
Morgan Keenan (MK) Spectral TypeF2Ib
One-Dimensional Spectral ClassF0
Position Angle288
Year of Observation1912. AD
Data Source
SKY2000 - Master Star Catalog - Star Catalog Database, Version 2
Sande C.B., Warren Jr. W.H., Tracewell D.A., Home A.T., Miller A.C.
(Goddard Space Flight Center, Flight Dynamics Division (1998))
Page compiled: Sun Sep 02 13:15:32 GMT+01:00 2001
Example of the "WHIRLPOOL" galaxy and it's pink spectrum as the collective point focus of the galactic lenses of the billions of galaxies, each having a small number of pink stars. The ability of pink to be the RED SHIFT but also the WHITE SHIFT , means that the LENSES in SPACE are WHITE, while the LENSES may be RED so that the resulting PINK as the mix between RED+WHITE=PINK, as the motion ability of GALACTIC LENSES to DISPLACE around the UNIVERSE at higher speeds and as the FOCUS function of the LENSES in MOTION.
The only lenses in motion would be the STAR SIZED ONES. The fact of LENSES being on the move as REAL AS IT GETS with the LENS being the size of the STAR CIRCUMFERENCE and may be SOURCE related to the center of the galaxy on their way out of the center disc or into it to fuel the larger WHOLE GALAXY.
So then, the image of the WHIRLPOOL GALAXY as having many positions of PINK STAR LENSES that are being COLLECTED together in the many positions seen in the galaxy as the small PINK STAR SIZE LENSES.
Here we see then HUBBLE DEEP FIELD and it's GIGANTIC LENSES related to Galaxies of very large sizes.
The fact that they are Yellow and that their alternate side of the color spectrum =violet, may indicate the relationships
of the smaller PINK DISCS and LENSES that are also complementary to the color spectrum of ORANGE as the
SUBTLE alternations of spectrum in opposite directions.
In the deep field the PINK LENSES no longer seem to exist, as the UNIVERSE has taken over their "NON FUNCTIONS"
due to their size being larger than the PINK LENSES that indicate the existance of "another point of view"=the smaller the
lens , the greater the chances of interactions on the levels of alien beings or human type beings and peaceful contact of
their ability to PROJECT into the FUTURE with the LENS functions.
The fact that they are Yellow and that their alternate side of the color spectrum =violet, may indicate the relationships
of the smaller PINK DISCS and LENSES that are also complementary to the color spectrum of ORANGE as the
SUBTLE alternations of spectrum in opposite directions.
In the deep field the PINK LENSES no longer seem to exist, as the UNIVERSE has taken over their "NON FUNCTIONS"
due to their size being larger than the PINK LENSES that indicate the existance of "another point of view"=the smaller the
lens , the greater the chances of interactions on the levels of alien beings or human type beings and peaceful contact of
their ability to PROJECT into the FUTURE with the LENS functions.