The Caulbearer-"born behind the veil"
link to; http://www.caulbearer.org/
Note from Enk; the below referencing tthe "Caulbearer" is an interesting site that describes a natural phenomenon, not known by the majority further identified below by a Wikipedia reference source cited below;Caul
From Wikipedia, the free encyclopedia
For other uses, see Caul (disambiguation).
A caul or cowl (Latin: Caput galeatum, literally, "helmeted head") is a piece of membrane that can cover a newborn's head and face.[1] Birth with a caul is rare, occurring in fewer than 1 in 80,000 births. The caul is harmless and is immediately removed by the physician or midwife upon delivery of the child.
The "en-caul" birth, not to be confused with the "caul" birth, occurs when the infant is born inside the entire amniotic sac. The sac balloons out at birth, with the amniotic fluid and child remaining inside the unbroken or partially broken membrane.
My connection on this for future reference originates with Ceres... see below;
Ceres (dwarf planet)
From Wikipedia, the free encyclopedia
Ceres as seen by Hubble Space Telescope(ACS).[1] The contrast has been enhanced to reveal surface details.
| |||||||||
| Discovery[2] | |||||||||
|---|---|---|---|---|---|---|---|---|---|
| Discovered by | Giuseppe Piazzi | ||||||||
| Discovery date | 1 January 1801 | ||||||||
| Designations | |||||||||
| MPC designation | 1 Ceres | ||||||||
| Pronunciation | /ˈsɪəriːz/ seer-eez | ||||||||
Named after
| Cerēs | ||||||||
| A899 OF; 1943 XB | |||||||||
| Minor planet category | dwarf planet main belt | ||||||||
| Adjectives | Cererian /sɨˈrɪəri.ən/ or Cererean /sɛrɨˈriːən/[3] | ||||||||
| Orbital characteristics[5] | |||||||||
| Epoch 2013-Nov-04 (JD 2456600.5) | |||||||||
| Aphelion | 445280000 km (2.9765 AU) | ||||||||
| Perihelion | 382520000 km (2.5570 AU) | ||||||||
| 413910000 km (2.7668 AU) | |||||||||
| Eccentricity | 0.075797 | ||||||||
| 4.60 yr 1680.99 d | |||||||||
| 466.7 d 1.278 yr | |||||||||
Average orbital speed
| 17.882 km/s | ||||||||
| 10.557° | |||||||||
| Inclination | 10.593° to Ecliptic 9.20° to Invariable plane[4] | ||||||||
| 80.3276° | |||||||||
| 72.2921° | |||||||||
| Satellites | None | ||||||||
| Proper orbital elements[6] | |||||||||
Proper semi-major axis
| 2.7670962 AU | ||||||||
Propereccentricity
| 0.1161977 | ||||||||
Proper inclination
| 9.6474122° | ||||||||
Proper mean motion
| 78.193318 deg / yr | ||||||||
Proper orbital period
| 4.60397 yr (1681.601 d) | ||||||||
Precession ofperihelion
| 54.070272 arcsec / yr | ||||||||
Precession of theascending node
| −59.170034 arcsec / yr | ||||||||
| Physical characteristics | |||||||||
Mean radius
| 476.2 ± ?? km[7] | ||||||||
Equatorial radius
| 487.3±1.8 km[8] | ||||||||
Polar radius
| 454.7±1.6 km[8] | ||||||||
| 2850000 km2 | |||||||||
| Mass |
0.00015 Earths 0.0128 Moons | ||||||||
Mean density
| 2.077±0.036 g/cm3,[8]2.09±??[7] | ||||||||
| 0.28 m/s2[7] 0.029 g | |||||||||
| 0.51 km/s[10] | |||||||||
Sidereal rotation period
| 0.3781 d 9.074170±0.000002 h[11] | ||||||||
| ≈ 3°[8] | |||||||||
North poleright ascension
| 19h 24m 291°[8] | ||||||||
North poledeclination
| 59°[8] | ||||||||
| Albedo | 0.090±0.0033 (V-band geometric)[12] | ||||||||
| |||||||||
Spectral type
| C[13] | ||||||||
| 6.64[14] to 9.34[15] | |||||||||
| 3.36±0.02[12] | |||||||||
| 0.854″ to 0.339″ | |||||||||
Ceres (minor-planet designation 1 Ceres) /ˈsɪəriːz/ (seer-eez)[18] is the largest object in the asteroid belt, which lies between the orbits of Mars and Jupiter. It is a ball of rock and ice 950 km (590 mi) in diameter, containing a third of the mass of the asteroid belt. It is the largest asteroid, and the only dwarf planet in the inner Solar System.
As uncanny as it may seem,, Ceres, described above connects directly to the below "The Caulbearer",, via
Nicholas Louis de Lacaille (March 15, 1713 - March 21, 1762)
Lacaille was honored by naming Moon crater La Caille (23.8S, 1.1 E, 67 km diameter) in 1961. Asteroid (9135) Lacaille was discovered on October 17, 1960 by C.J. van Houten, I. van Houten-Groeneveld, and T. Gehrels at Palomar Observatory, and provisionally designated 7609 P-L; it was later designated 1994 EK6 on an independent observation.
Links
- Lacaille's "Catalog of Nebulae of the Southern Sky"
- Nicolas-Louis de Lacaille images, NGC/IC observers page
- Some Abbe Lacaille info, Yann Pothier
- Asteroid 9135 Lacaille (7609 P-L) (NEO/JPL)
- Nicholas Louis de la Caille, 1755. Sur les étoiles nébuleuses du Ciel Austral [On the nebulous stars of the Southern Sky]. Memoirs of the Royal Academy for 1755 (Paris), pp. 194-199.
- Nicholas Louis de Lacaille, 1763. Coelum Australe Stelliferum; seu Ovservationes ad Construendum Stellarum Australium Catalogum Institutae, in Africa ad Caput Bonae-Spei. Hipp. Lud. Guerin & Lud. Fr. Delatour, Paris, 1763. In Latin.
- F. Boquet, 1913. Bicentenaiere de La Caille. Bull. Soc. Ast. France, 27th year, p. 457.
- Jean Baptiste Joseph Delambre, 1827. Histoire de l'Astronomie au dix-huitièmme siècle [History of Astronomy in the Eighteenth Century]. Bachelier (Successor of Mme. Ve. Courcier), Paris. P. xxx, 457-542.
- David S. Evans, 1992. Lacaille: Astronomer, Traveler. Pachart History of Astronomy Series, Vol. 9, Series Editor: A.G. Pacholczyk. Pachart Publishing House, Tucson, Arizona.
- Owen Gingerich, 1960. Abbé Lacaille's List of Clusters and Nebulae. Sky and Telescope, February 1960, pp. 207-208 [ADS: 1960S&T....19..207G].
- Kenneth Glyn Jones, 1969. The Search for the Nebulae -- VI. Journal of the British Astronomical Association, Vol. 79, No. 3 (1969), pp. 213-222. Section on Lacaille: p. 213-218. Reprinted in: The Search for the Nebulae. Chalfont St. Giles, 1975.
- Kenneth Glyn Jones, 1991. Messier's Nebulae and Star Clusters. 2nd ed, Cambridge University Press, pp. 328-9.
- Rolf Sauermost, Doris Freudig & Sabine Ganter (eds.), 1996. Lexikon der Naturwissenschaftler. Spektrum Akademischer Verlag, Heidelberg, Berlin. Here article on Lacaille, p. 256.
- direct connection to a seer by birth, so to speak. Enk;
Star names their lore and meaning
http://www.messier.obspm.fr/more/m-jwisn.html| Author: | Richard Hinckley Allen |
|---|---|
| Publisher: | New York Dover Publ. [2000] |
| Edition/Format: |  Book : English : Unabridged and corr. republView all editions and formats |
| Database: | WorldCat |
| Rating: |
The Caulbearer
The correct name for those who are born with a true caul is a Caulbearer. Such people are often referred to as being "born behind the veil", as the caul is also referred to as the veil in many cultures due to it being a face covering.
Introduction
Caulbearer.org has been established as a resource to provide specific insight into the phenomenon of the Caul and Caulbearers. These pages provide information on both headings, so they may be of use to both
- (a) the casual visitor or researcher on the phenomenon of the Caul, also known as the Veil, and;
- (b) those who wish to know more in relation to the Caul in the context of how it relates to the philosophy of The Way, much of whose precepts originated in the teachings of the Caulbearer fraternity known as the Nazarenes, the Brotherhood of Light, and particularly through those of the High Caulbearers, the high teachers of truth, knowledge, logic and reason, collectively known as the Seven Veils.
The name, word, title or office of Caulbearer is the sole intellectual property of Robert George Crosbie and the Brotherhood of Nazarenes, a fraternity of Caulbearers and non-Caulbearers of like mind, known as the followers of The Way. This important fact relating to the use of the word or title of Caulbearer is fully explained in our copyright page. All other use of the word in unauthorised publications or media is considered infringement of copyright.
Should you wish to know more of The Way, please visittheorderoftheway.org.
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