i solved another key feature from the corral castle. Our friend
that is shewn below. add pictures.
related to the crown constellation.
in fact the big dipper itself. looking north.
I had sloven, rather confirming its position an ancient Sumerian glyph. find pic. add confirm, description.:angel::angel:
(enter the age of Aquarius. we have the full moon a gibbis. november 2013.
the question is what is poynting? a vector potential, in fact more then just one. now we follow the tail of the scorpion to the red beating pulsing star in the east before dawn. from my eye i see a streaming tail of matter.
looking directly at this star with the naked eye is not advised. A whole cut in the great pyramids to capture one of these stars light. in theory we are in that position, but for how long it remains is the question.
looking now north to the big dipper, upside down with its handle. 6 stars in enlightenment with the crown stone . this is the point i wish to ponder, and show.
At the headache has come back. and is that of ion passing our bow. this will cause internet, and cell phone problems. in a short time. an ordinary spark gap trigger is assumed. This may bean unbarable situation for some people.
the Orion comes out of the water, he steps onto the earth. at a time of water, as he bears his water.
the pyramidal crown stone has how many points, how many stars.lets see what is said. add movie.
lets discover his history, and greatest discovery.
https://www.youtube.com/watch?v=Ga4d0e0YGC8 now what did we do,? a trail of bread crumbs..
Our friend Mr pool has in deed added a great deal of knowlage. i will recap this for my understanding. yours also.
at one min 15 sec Mr Pool states, this 5 pointed star depicted as a chunk of coral carved. stated spica is the brightest star in Virgo. at 2min 14 sec he states to drop below polaris.
in support we find footnoetes.
Arcturus
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For other uses, see Arcturus (disambiguation).
Arcturus
Bootes constellation map.png
Arcturus in the constellation of Boötes.
Observation data
Epoch J2000 Equinox J2000
Constellation Boötes
Pronunciation /ɑrkˈtjʊərəs/
Right ascension 14h 15m 39.7s[1]
Declination +19° 10′ 56″[1]
Apparent magnitude (V) −0.04[1]
Characteristics
Spectral type K1.5IIIFe-0.5
Apparent magnitude (J) −2.25[1]
U−B color index 1.27
B−V color index 1.23
R−I color index 0.65
Variable type Variable star
Note (category: variability): H and K emission vary.
Astrometry
Radial velocity (Rv) -5 km/s
Proper motion (μ) RA: −1093.45 mas/yr
Dec.: −1999.40 mas/yr
Parallax (π) 88.98 ± 0.68 mas
Distance 36.7 ± 0.3 ly
(11.24 ± 0.09 pc)
Absolute magnitude (MV) −0.30 ± 0.02[2]
Details
Mass 1.10 ± 0.06[3] M☉
Radius 25.7 ± 0.3[4] R☉
Luminosity 170[3] L☉
Surface gravity (log g) 1.76 ± 0.05[3] cgs
Temperature 4,290 ± 43[3] K
Metallicity [Fe/H] −0.37[5] dex
Rotational velocity (v sin i) 2.4 ± 1.0[2] km/s
Other designations
Alramech, Abramech, α Boötis, 16 Boötes, BD+19°2777, GCTP 3242.00, GJ 541, HD 124897, HIP 69673, HR 5340, LHS 48, SAO 100944.
Database references
SIMBAD data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.),
VizieR catalog entry
Arcturus (/ɑrkˈtjʊərəs/; α Boo, α Boötis, Alpha Boötis) of the constellation Boötes is the brightest star in the northern celestial hemisphere. With a visual magnitude of −0.04, it is the fourth brightest star in the night sky, after −1.46 magnitude Sirius, −0.86 magnitude Canopus, and −0.27 magnitude Alpha Centauri. It is a relatively close star at only 36.7 light-years from Earth, and, together with Vega and Sirius, one of the most luminous stars in the Sun's neighborhood.
Arcturus is a type K1.5 IIIpe orange giant star, with an absolute magnitude of −0.30. It has likely exhausted its hydrogen from the core and is currently in its active hydrogen shell burning phase. It will continue to expand before entering horizontal branch stage of its life cycle.
footnote spica the blue kachina?
Spica
From Wikipedia, the free encyclopedia
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For other uses, see Spica (disambiguation).
Alpha Virginis A/B
Location of Spica
Cercle rouge 100%.svg
Location of Spica (circled) in the constellation Virgo
Observation data
Epoch J2000 Equinox J2000
Constellation Virgo
Pronunciation /ˈspaɪkə/
Right ascension 13h 25m 11.5793s[1]
Declination −11° 09′ 40.759″[1]
Apparent magnitude (V) +1.04
Characteristics
Spectral type B1 III-IV/B2 V[2]
U−B color index −0.94[3]
B−V color index −0.24[3]
Variable type β Cep,
Rotating ellipsoid
Astrometry
Radial velocity (Rv) +1.0[4] km/s
Proper motion (μ) RA: −42.50[1] mas/yr
Dec.: −31.73[1] mas/yr
Parallax (π) 12.44 ± 0.86[1] mas
Distance 260 ± 20 ly
(80 ± 6 pc)
Absolute magnitude (MV) −3.55 (−3.5/−1.5)[5]
Orbit[6]
Period (P) 4.0145898 d
Eccentricity (e) 0.067 ± 0.014
Inclination (i) 54 ± 6°
Periastron epoch (T) 2440678.09
Argument of periastron (ω)
(secondary) 140 ± 10°
Details
Primary
Mass 10.25 ± 0.68[6] M☉
Radius 7.40 ± 0.57[6] R☉
Luminosity 12,100[7] L☉
Surface gravity (log g) 3.7 ± 0.1[5] cgs
Temperature 22,400[5] K
Rotational velocity (v sin i) 199 ± 5[6] km/s
Secondary
Mass 6.97 ± 0.4[6] M☉
Radius 3.64 ± 0.28[6] R☉
Luminosity 1,500[7] L☉
Temperature 18,500[7] K
Rotational velocity (v sin i) 87 ± 6[6] km/s
Other designations
Spica, Azimech, 角宿一, Spica Virginis, Alaraph, Dana, α Virginis, 67 Virginis, HR 5056, BD -10°3672, HD 116658, GCTP 18144, FK5 498, CCDM 13252-1109, SAO 157923, HIP 65474.[8]
Spica (α Vir, α Virginis, Alpha Virginis, pronounced /ˈspaɪkə/) is the brightest star in the constellation Virgo, and the 15th brightest star in the night sky. It is a blue giant and a variable star of the Beta Cephei type located 260 light years from Earth.
footnote Polaris
From Wikipedia, the free encyclopedia
Jump to: navigation, search
For other uses, see Polaris (disambiguation).
Alpha Ursae Minoris
Polaris alpha ursae minoris.jpg
Polaris as seen by the Hubble Space Telescope.
Observation data
Epoch J2000 Equinox J2000
Constellation Ursa Minor
Component α UMi Aa α UMi Ab α UMi B
Right ascension 02h 31m 49.09s 02h 30m 41.63s
Declination +89° 15′ 50.8″ +89° 15′ 38.1″
Apparent magnitude (V) 1.98v[1] 9.2[1] 8.7[1]
Characteristics
Spectral type F7Ib F6V F3V
U-B color index 0.38[1] 0.01[2]
B-V color index 0.60[1] 0.42[2]
Variable type Classical Cepheid
Astrometry
Radial velocity (Rv) -17 km/s
Proper motion:
RA (μα cos δ) 44.48±0.11 mas/yr
Dec. (μδ) -11.85±0.13 mas/yr
Parallax (π) 7.54 ± 0.11 mas
Distance 325[3] - 425[4] ly
(99[3] - 129.5[4] pc)
Absolute magnitude (MV) -3.6[1] 3.6[1] 3.1[1]
Details
Mass 4.5[1] M☉ 1.26[1] M☉ 1.39[1] M☉
Radius 46±3[1] R☉ 1.38[2] R☉
Surface gravity (log g) 2.2[5] 4.3[2]
Luminosity (bolometric) 2500[6] L☉ 3[1] L☉ 3.9[2] L☉
Temperature 6015[2] K 6900[2] K
Metallicity 112% solar[7]
Rotation 119 days[8]
Rotational velocity (v sin i) 14[8]km/s 110[2]km/s
Age 7×107[9] years
Orbits[1]
Secondary/primary Ab/Aa B/A
Period (P) 29.59 years ~100,000 years
Semimajor axis (a) 0.133" 32" (0.02 pc)
Eccentricity (e) 0.608
Inclination (i) 128°
Longitude of node (Ω) 19°
Argument of periastron (ω)
(secondary) 303°
Semi-amplitude (K1)
(primary) 3.72km/s
Position (relative to Aa)
Epoch of observation 2005.5880 2005.5880
Angular distance 0.172″ 18.217″
Position angle 231.4° 230.540°
Database references
SIMBAD data data
Other designations
Polaris, North Star, 1 Ursae Minoris, HR 424, BD +88°8, HD 8890, SAO 308, FK5 907, GC 2243, ADS 1477, CCDM 02319+8915, HIP 11767, Cynosura, Alruccabah, Phoenice, Navigatoria, Star of Arcady, Yilduz, Mismar
Polaris (α UMi, α Ursae Minoris, Alpha Ursae Minoris, commonly North Star, Northern Star or Pole Star, also Lodestar, sometimes Guiding star) is the brightest star in the constellation Ursa Minor. It is very close to the north celestial pole, making it the current northern pole star.
It is a multiple star, consisting of the main star α UMi Aa, two smaller companions, α UMi B and α UMi Ab, and two distant components α UMi C and α UMi D. α UMi B was discovered in 1780 by William Herschel.
Many recent papers calculate the distance to Polaris at about 434 light-years (133 parsecs).[4] Some suggest it may be 30% closer which, if correct, is especially notable because Polaris is the closest Cepheid variable to Earth so its physical parameters are of critical importance to the whole astronomical distance scale.[3]
at 7 min 22 seconds we see the corral castle l crown stones. i say
I say they must be unfolded into the big dipper.
if we now drop 10 cents, degrees, or arch seconds below we find something poynting. what star is it?.
lets test this for truth.:angel:
[/size]
I add as a prediction to test for truth
Aug 16 2016 a special note worthy date, perhaps a bell ringer also, ring bell two times. future date.:angel: :sleepy::dodgy:
Test February 5th 2016, for great quake. on anniversary of, feb 5th 2013. kelpers law
M8.0 - 76km W of Lata, Solomon Islands (BETA) 2013-02-06 01:12:27 UTC
PAGER - GREEN ShakeMap - VIII DYFI? - VIII Tsunami Warning Center
Earthquake location 10.738°S, 165.138°EReturn to the EQ List/Map/Search
kml iconGoogle Earth KML
Summary
Location and Magnitude contributed by: USGS National Earthquake Information Center
General
+-
50 km
30 mi
Powered by Leaflet
10.738°S, 165.138°E
Depth: 28.7km (17.8mi)
Event Time
2013-02-06 01:12:27 UTC
2013-02-06 12:12:27 UTC+11:00 at epicenter
2013-02-05 20:12:27 UTC-05:00 system time
Location
10.738°S 165.138°E depth=28.7km (17.8mi)
Nearby Cities
76km (47mi) W of Lata, Solomon Islands
574km (357mi) NNW of Luganville, Vanuatu
586km (364mi) ESE of Honiara, Solomon Islands
846km (526mi) NNW of Port-Vila, Vanuatu
1149km (714mi) NNW of We, New Caledonia