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	Cancer (Site not responding. Last check: 2007-10-09)
		Zeta Cancri is a notable triple system comprised of a close binary with a period of 59.5 years and a more distant star, component C, with a much longer period of 1115 years.
		Phi Cancri is a binary of two identical white stars (5.5m, 6m): the PA is 217º and separation is 5.1".
		R Cancri is a Mira-type variable with period of 361.6 days and a magnitude change from 6.07 to 11.8.
	www.wingmakers.co.nz /Cancer.html (1124 words)

	Epsilon Cancri - Wikipedia, the free encyclopedia
		Epsilon Cancri (ε Cnc / ε Cancri) is a star in the constellation Cancer.
		ε Cancri is a member of the Beehive Cluster, and the Bayer designation ε Cancri originally referred to the entire cluster.
		ε Cancri is a white A-type main sequence dwarf with an apparent magnitude of +6.29.
	en.wikipedia.org /wiki/Epsilon_Cancri (109 words)

	Extra solar planets: Gas giants, Space Art, 51 Pegasi, 55 Cancri, Tau Bootis, 47 Ursae Majoris, 70 Virginis
		55 Cancri e orbits the star in less than 3 (2.8) days, and the temperature at its' distance (about 5.6 million km.) is about 1 200 degrees Kelvin.
		It orbits the main star at a distance of about 17 million km and the temperature may be around 700 K (this high temperature might have made the planet to swollen up to about 120% of Jupiter's radius), which is similar to that of Mercury.
		Epsilon Eridani b orbits its' star at an average distance of 3.3 AU.
	www.novacelestia.com /space_art_extrasolar_planets/gas_giants.html (2592 words)

	Epsilon Cancri \| Sigma Alpha Epsilon Eugene Oregon (Site not responding. Last check: 2007-10-09)
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	crkh.info /epsilon-cancri.htm (271 words)

	Tau Kappa Epsilon Texas State \| Epsilon Zeta Theta Chi (Site not responding. Last check: 2007-10-09)
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	crkh.info /tau-kappa-epsilon-texas-state.htm (483 words)

	AstroAlert
		A good northern-limit dark-limb graze of epsilon Cancri will be visible from southern Hokkaido, and a graze of 6.8-mag.
		A good northern-limit dark-limb graze of epsilon Cancri will be visible from Ireland, central U.K., southern Sweden, and southern Finland, with grazes of some 7th-mag.
		The epsilon Cancri northern limit is too far north; the southern limit crosses southern Virginia, but the graze will not be observable since it will occur on the sunlit side of the Moon.
	www.xs4all.nl /~carlkop/astalert.html (992 words)

	Canberra Astronomical Society - Southern Cross - April 1997
		Epsilon Cancri, a white star; other bright stars are yellowish or yellow-orange.
		It appeared as a rich group of completely resolved faint stars, the brightest (on the N side) being golden yellow.
		In the other direction, 9 degrees N of M44, Iota Cancri (08h 46.7m, +28 46') is an orange-yellow and pale blue binary that rivals Albireo in Cygnus.
	msowww.anu.edu.au /cas/southerncross/sc_199704.html (1320 words)

	Cancer
		Its stars are generally four magnitude, beta Cancri being the brightest at 3.52.
		It has been estimated that over a hundred of its stars are brighter than our Sun, and in fact (as Burnham points out) if the Sun were a member of this group, it would be a very modest member indeed, at about 10.9 magnitude.
		Visually unremarkable, yet this deep sky object is renowned for its venerable age: it is now believed that the cluster is approximately 10 billion years old.
	www.dibonsmith.com /cnc_con.htm (1320 words)

	EXN.ca \| Space
		According to 55 Cancri's wobble, there should be another object orbiting it.
		But its average distance from 55 Cancri would be about 5.5 Astronomical Units - about the same as Jupiter is from our Sun.
		The gas giant planet discovered orbiting Epsilon Eridani also orbits its star at about the same distance as Jupiter orbits the Sun.
	www.exn.ca /Stories/2000/08/08/53.asp (675 words)

	Deepsky observing report 27-02-04: Zeta Cancri, Iota Cancri, Algieba, NGC 2903, M 53, M 3, M 13 and La Superba
		Deepsky observing report 27-02-04: Zeta Cancri, Iota Cancri, Algieba, NGC 2903, M 53, M 3, M 13 and La Superba
		Then you are in the area of Zeta Cancri.
		Again, this object is easy tot locate, because there are some bright stars in the Lion's head that will guide you to NGC 2903.
	www.backyard-astro.com /deepsky/2004_02_27/27feb04.html (825 words)

	Newsletter- Nehru Centre
		Phi Cancri is a binary of two identical white stars.
		The primary is a bright 6.5m, with a 9.0m companion B. To find this group, first locate epsilon Cancri, which is near the centre of the Beehive Cluster and the brightest star in this cluster.
		It has been estimated that over a hundred of its stars are brighter than our Sun, and in fact if the Sun were a member of this group, it would be a very modest member indeed, at about 10.9 magnitude.
	www.nehrucentremumbai.com /newsletter/April03/zodiac_sign.htm (835 words)

	Messier 44
		Praesepe Cancri (M44) is so very loose and straggling that it would only be noticed as a region rich in L [large; bright] stars; - so also described in Sweeps 59 and 63.
		The Praesepe was called by the Arabians al-ma'laf, a stall or den; and also al-nathrah, the fissure between the Lion's whiskers, - a district which formed the VIIIth Lunar Mansion.
		An occult line projected from Spica under Regulus, and about 22deg beyond the latter, rund through Praesepe; or it may be found by a ray from the Pleiades being brought mid-way between Procyon and Castor, which will pass over Epsilon, in Castor's knee.
	www.seds.org /messier/Mdes/dm044.html (761 words)

	Extrasolar Planets (via CobWeb/3.1 planetlab2.cs.umd.edu) (Site not responding. Last check: 2007-10-09)
		Epsilon Eridani is considered to be a star very similiar to our sun.
		It was also determined by the wobble's characteristics that the planet lies approximately 18 million kilometers (0.11 AU) from the star, and has a mass similiar to that of Jupiter (i.e., 87% Jupiter's mass).
		Marsh and Mahoney (1), (2) in a series of papers have suggested gaps in the interstellar dust clouds (circumstellar disks) that may infer the possibility of a planetary body.
	www.public.asu.edu.cob-web.org:8888 /~sciref/exoplnt.htm (15809 words)

	Some Bright Spring Double Stars
		Often forgotten are the beautiful double stars that also inhabit the spring skies.
		iota Cancri mags 4.2 and 6.6, sep 30.5”
		Like the similar pair epsilon Pegasi, this duo displays an illusory oscillating motion when you jiggle the telescope tube back and forth in a direction perpendicular to a line joining them.
	www.theskyscrapers.org /content3490.html (365 words)

	FROM NOTHING TO ETERNITY
		It is a cluster of over 350 stars, with one, Epsilon Cancri, being of absolute magnitude 0.2, and a luminosity of about 70 of our suns.
		The Epsilon star, at the tip of the "sickle", has twin companions making a triangle with the main star, while the Zeta star, Adhafera, has 3 companions which are findable in small amateur telescopes.
		The Epsilon star, Vindemiatrix, is the patron star of vinyardists and winemakers.
	home.att.net /~d.r.fudge/art_bgs/HODGE.htm (1663 words)

	Science Adhara
		also known as Adara and Epsilon Canis Majoris, second brightest star in the constellation Canis Major, the Large Dog.
		The name Adhara is derived from the Arabic phrase Al Adhara, meaning "The Virgins," the name of an archaic Arabic constellation that included several other brilliant blue stars in the celestial vicinity, including Wezen (Delta Canis Majoris) and Aludra (Eta Canis Majoris).
		Adhara is classified as a blue giant star, meaning that it has used up much of the hydrogen in its core, which has caused it to undergo changes that have increased its size.
	www.latifm.com /look/Science_Adhara.htm (370 words)

	Beehive Cluster - Encyclopedia, History, Geography and Biography
		Messier 44's age is estimated at about 730 million years.
		One of the brighter components of the Beehive Cluster is Epsilon Cancri, which is also known as 41 Cancri.
		Originally, the Bayer designation ε Cancri was applied to the entire cluster.
	www.arikah.com /encyclopedia/NGC_2632 (213 words)

	Dr. William Cochran's Outreach Lecture Information
		An illustration of a Jupiter-like planet and its hypothetical moon (blue orb) circling the star 55 Cancri.
		In addition to Gamma Cephei, the team has found planets orbiting the stars 16 Cygni B and Epsilon Eridani.
		His research interests include the search for extrasolar planetary systems, high-precision measurements of stellar radial velocity variations, variable stars, asteroids, planetary atmospheres, and comets.
	www.esi.utexas.edu /outreach/ols/lectures/Cochran/index.html (282 words)

	Randy Muller; Assault on the Beehive
		The wide double is epsilon Cancri (aka Tycho 1395-2733-1, Hipparcos 42556 and SAO 98024 for those keeping score at home).
		Finally, I observed a faint galaxy (UGC 4526 = PGC 24400) about 13 arcminutes to the south east of epsilon Cancri, anchoring my starhop once again on the house asterism.
		This turned out to be a very rewarding, entertaining and spontaneous project, borne of idle conversion during bad atmospheric conditions.
	observers.org /reports/2002.02.09.7.html (1187 words)

	Identifying star clusters
		Known also as Praesepe (Latin for manger), it's Messier No. is M44.
		When observing it, look for the eclipsing binary star TX Cancri.
		Epsilon Cancri is also an eye catcher and worth spending some time to find.
	www.astronomytoday.com /astronomy/clusters.html (462 words)

	Beehive (Site not responding. Last check: 2007-10-09)
		The orange color of the giant stars shows nicely.
		"Epsilon Cancri" was initially appled to the whole cluster.
		The giants within the cluster are labelled with their Flamsteed and (longer) HD numbers, the latter coming from the spectroscopic Henry Draper Catalogue.
	www.astro.uiuc.edu /~kaler/sow/beehive-t.html (101 words)

	cancer_(constellation)
		{{Infobox Constellationname = Cancer abbreviation = Cnc genitive = Cancri symbology = the Crab RA = 9 dec= +20 areatotal = 506 arearank = 31st numberstars = 0 starname = Î² Cnc (Altarf) starmagnitude = 3.5 meteorshowers = *Delta Cancrids bordering =
		Cancer is best noted among stargazers as the home of Praesepe (M44), an open cluster also called the Beehive Cluster or the Gate of Men, which contains the star Îµ Cancri.
		The smaller, denser open cluster M67 can be found here as well.
	www.pokerpiratesforum.com /wiki/?title=Cancer_(constellation) (1054 words)

	Star Coordinates - Ultronomicon
		832.2 893.4 Alpha Hyades 837.5 895.8 Beta Hyades 837.5 904.1 Gamma Hyades 824.9 895.8 Delta Hyades 850.0 912.5 Epsilon Hyades 850.0 937.2 Zeta Hyades 845.8 939.3 Eta Hyades 829.6 954.8 Theta Hyades 800.0 950.5 Iota Hyades 766.4 958.9 Kappa Hyades 725.5 937.4 Lambda Hyades
		190.2 606.5 Alpha Orionis 197.8 596.8 Beta Orionis 192.3 587.8 Gamma Orionis 171.4 592.6 Delta Orionis 154.5 581.8 Epsilon Orionis 155.8 605.8 Zeta Orionis 179.5 632.9 Eta Orionis 188.1 630.8 Theta Orionis 211.8 637.9 Iota Orionis 220.0 617.6 Kappa Orionis 215.9 607.3 Lambda Orionis 222.8 603.8 Mu Orionis
		491.1 018.0 Alpha Serpentis 486.1 026.2 Beta Serpentis 492.3 029.4 Gamma Serpentis 474.7 022.1 Delta Serpentis 487.2 040.8 Epsilon Serpentis 500.7 003.5 Zeta Serpentis 474.1 007.8 Eta Serpentis 452.9 016.9 Theta Serpentis 459.6 042.9 Iota Serpentis
	uqm.stack.nl /wiki/Star_Coordinates (1872 words)

	University of Pittsburgh - Physics & Astronomy Department (Site not responding. Last check: 2007-10-09)
		Han, I. and Gatewood, G. An Upper Limit to the Mass of the Radial Velocity Companion of rho1 Cancri", ApJ 564,L27-L30.
		2003, "HST Fine Guidance Sensor Astrometry of the Extrasolar Planet Candidates Epsilon Eri and Upsilon And, A Progress Report", Bulletin of the American Astronomical Society, 35, #4, G.F.Benedict, B.E. McArthur, A Hatzes, E.Nelan, W.D. Cochran.
		2003, Update to "An Upper Limit to the Mass of the Radial Velocity Companion of rho1 Cancri", Scientific Frontiers in Research on Extrasolar Planets, ASP Conference Series (ed D.Deming and S.Seager).
	www.phyast.pitt.edu /People/Faculty/GD_Gatewood.htm (298 words)

	NGC (Site not responding. Last check: 2007-10-09)
		I counted approximately 50 stars and noted one very colorful golden, more yellowish than orange, star: 39 Cancri which was coupled with a brilliant white SAO 80336.
		Forming the slightly distorted square of the base of the house were: SAO 98030, SAO 98032, SAO 98021, and Epsilon 41 Cancri.
		Forming the triangular roof of the house were SAO 98021 and Epsilon 41 Cancri which marked the top of the square and the base of the triangle.
	delaneys.home.att.net /a/dso.html (14485 words)

	First part of a novel - Hatrack River Writers Workshop (Site not responding. Last check: 2007-10-09)
		A better choice perhaps would be Delta Pavonis or Epsilon Eridani...do some research on near-Terra stars.
		Also, is this a multi-generational ship that they're on?
		Personally, I'm a fan of Procyon and Epsilon Eridani.
	www.hatrack.com /forums/writers/forum/Forum11/HTML/002026.html (4326 words)

	astrobiology, astrobiologia, cemistry of life (via CobWeb/3.1 planetlab2.cs.umd.edu) (Site not responding. Last check: 2007-10-09)
		Descubierto y fotografiado un objeto de tan sólo 25 veces la masa de
		Evidence for a Long-period Planet Orbiting Epsilon Eridani
		Detection of a spectroscopic transit by the planet orbiting the star HD209458
	astrobionet.rediris.es.cob-web.org:8888 /extrasolar.html (439 words)

	Extrasolar Visions (via CobWeb/3.1 planetlab2.cs.umd.edu) (Site not responding. Last check: 2007-10-09)
		EV: Updates and images now available for 55 Cancri e, b, and c
		Space.com: Small Planet inferred in epsilon Eridani dust disk
		CNN: Disk of 55 Cancri resembles Kuiper Belt
	www.thyrenacia.com.cob-web.org:8888 /news.asp (804 words)

	Ask John Harper (Site not responding. Last check: 2007-10-09)
		Alpha Cancri is Acubens, Beta is Ai Tarf, Gamma and Delta are known respectively as Asellus Borealis and Asellus australis.
		Epsilon Cancri and the surrounding stars constitute M44 or the Praesepe (Beehive) Galactic Open Cluster, whilst Zeta Cancri, the only other star with a proper name, is Tegmine
		What is the motion and decribe the motion of the earth that makes the stars,moon and sun move westward??
	www.cyberwitch.com /Wychwood/Observatory/askJohnHarper.asp?id=279 (11952 words)

	Astronomical League Double Star Observing Log
		RDF came off scope, lucky to find this one.
		DI:93.91 30 Jan Coyote Lake 80mm f/6 Stellarvue Refractor Seeing 6-7 LM 5.9 4.8mm 100x Elusive, I thought my chart for this and Iota Cancri was messed up.
		Didn't know I was looking for a wide difference in magnitude.
	www.wgg.com /scope/dbl.html (5829 words)

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