Will Alexander, Exobiology As Goddess
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CONSTELLATION TRIANGULUM, the TRIANGLE Triangulum Is a Small Constellation in the Northern Sky
CONSTELLATION TRIANGULUM, THE TRIANGLE Triangulum is a small constellation in the northern sky. Its name is Latin for "triangle", derived from its three brightest stars, which form a long and narrow triangle. Known to the ancient Babylonians and Greeks, Triangulum was one of the 48 constellations listed by the 2nd century astronomer Ptolemy. The celestial cartographers Johann Bayer and John Flamsteed catalogued the constellation's stars, giving six of them Bayer designations. The white stars Beta and Gamma Trianguli, of apparent magnitudes 3.00 and 4.00, respectively, form the base of the triangle and the yellow-white Alpha Trianguli, of magnitude 3.41, the apex. Iota Trianguli is a notable double star system, and there are three star systems with planets located in Triangulum. The constellation contains several galaxies, the brightest and nearest of which is the Triangulum Galaxy or Messier 33—a member of the Local Group. The first quasar ever observed, 3C 48, also lies within Triangulum's boundaries. HISTORY AND MYTHOLOGY In the Babylonian star catalogues, Triangulum, together with Gamma Andromedae, formed the constellation known as MULAPIN "The Plough". It is notable as the first constellation presented on (and giving its name to) a pair of tablets containing canonical star lists that were compiled around 1000 BC, the MUL.APIN. The Plough was the first constellation of the "Way of Enlil"—that is, the northernmost quarter of the Sun's path, which corresponds to the 45 days on either side of summer solstice. Its first appearance in the pre-dawn sky (heliacal rising) in February marked the time to begin spring ploughing in Mesopotamia. -
Wynyard Planetarium & Observatory a Autumn Observing Notes
Wynyard Planetarium & Observatory A Autumn Observing Notes Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn Tour of the Sky with the Naked Eye CASSIOPEIA Look for the ‘W’ 4 shape 3 Polaris URSA MINOR Notice how the constellations swing around Polaris during the night Pherkad Kochab Is Kochab orange compared 2 to Polaris? Pointers Is Dubhe Dubhe yellowish compared to Merak? 1 Merak THE PLOUGH Figure 1: Sketch of the northern sky in autumn. © Rob Peeling, CaDAS, 2007 version 1.2 Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn North 1. On leaving the planetarium, turn around and look northwards over the roof of the building. Close to the horizon is a group of stars like the outline of a saucepan with the handle stretching to your left. This is the Plough (also called the Big Dipper) and is part of the constellation Ursa Major, the Great Bear. The two right-hand stars are called the Pointers. Can you tell that the higher of the two, Dubhe is slightly yellowish compared to the lower, Merak? Check with binoculars. Not all stars are white. The colour shows that Dubhe is cooler than Merak in the same way that red-hot is cooler than white- hot. 2. Use the Pointers to guide you upwards to the next bright star. This is Polaris, the Pole (or North) Star. Note that it is not the brightest star in the sky, a common misconception. Below and to the left are two prominent but fainter stars. These are Kochab and Pherkad, the Guardians of the Pole. Look carefully and you will notice that Kochab is slightly orange when compared to Polaris. -
Winter Observing Notes
Wynyard Planetarium & Observatory Winter Observing Notes Wynyard Planetarium & Observatory PUBLIC OBSERVING – Winter Tour of the Sky with the Naked Eye NGC 457 CASSIOPEIA eta Cas Look for Notice how the constellations 5 the ‘W’ swing around Polaris during shape the night Is Dubhe yellowish compared 2 Polaris to Merak? Dubhe 3 Merak URSA MINOR Kochab 1 Is Kochab orange Pherkad compared to Polaris? THE PLOUGH 4 Mizar Alcor Figure 1: Sketch of the northern sky in winter. North 1. On leaving the planetarium, turn around and look northwards over the roof of the building. To your right is a group of stars like the outline of a saucepan standing up on it’s handle. This is the Plough (also called the Big Dipper) and is part of the constellation Ursa Major, the Great Bear. The top two stars are called the Pointers. Check with binoculars. Not all stars are white. The colour shows that Dubhe is cooler than Merak in the same way that red-hot is cooler than white-hot. 2. Use the Pointers to guide you to the left, to the next bright star. This is Polaris, the Pole (or North) Star. Note that it is not the brightest star in the sky, a common misconception. Below and to the right are two prominent but fainter stars. These are Kochab and Pherkad, the Guardians of the Pole. Look carefully and you will notice that Kochab is slightly orange when compared to Polaris. Check with binoculars. © Rob Peeling, CaDAS, 2007 version 2.0 Wynyard Planetarium & Observatory PUBLIC OBSERVING – Winter Polaris, Kochab and Pherkad mark the constellation Ursa Minor, the Little Bear. -
List of Easy Double Stars for Winter and Spring = Easy = Not Too Difficult = Difficult but Possible
List of Easy Double Stars for Winter and Spring = easy = not too difficult = difficult but possible 1. Sigma Cassiopeiae (STF 3049). 23 hr 59.0 min +55 deg 45 min This system is tight but very beautiful. Use a high magnification (150x or more). Primary: 5.2, yellow or white Seconary: 7.2 (3.0″), blue 2. Eta Cassiopeiae (Achird, STF 60). 00 hr 49.1 min +57 deg 49 min This is a multiple system with many stars, but I will restrict myself to the brightest one here. Primary: 3.5, yellow. Secondary: 7.4 (13.2″), purple or brown 3. 65 Piscium (STF 61). 00 hr 49.9 min +27 deg 43 min Primary: 6.3, yellow Secondary: 6.3 (4.1″), yellow 4. Psi-1 Piscium (STF 88). 01 hr 05.7 min +21 deg 28 min This double forms a T-shaped asterism with Psi-2, Psi-3 and Chi Piscium. Psi-1 is the uppermost of the four. Primary: 5.3, yellow or white Secondary: 5.5 (29.7), yellow or white 5. Zeta Piscium (STF 100). 01 hr 13.7 min +07 deg 35 min Primary: 5.2, white or yellow Secondary: 6.3, white or lilac (or blue) 6. Gamma Arietis (Mesarthim, STF 180). 01 hr 53.5 min +19 deg 18 min “The Ram’s Eyes” Primary: 4.5, white Secondary: 4.6 (7.5″), white 7. Lambda Arietis (H 5 12). 01 hr 57.9 min +23 deg 36 min Primary: 4.8, white or yellow Secondary: 6.7 (37.1″), silver-white or blue 8. -
UNSC Science and Technology Command
UNSC Science and Technology Command Earth Survey Catalogue: Official Name/(Common) Star System Distance Coordinates Remarks/Status 18 Scorpii {TCP:p351} 18 Scorpii {Fact} 45.7 LY 16h 15m 37s Diameter: 1,654,100km (1.02R*) {Fact} -08° 22' 06" {Fact} Spectral Class: G2 Va {Fact} Surface Temp.: 5,800K {Fact} 18 Scorpii ?? (Falaknuma) 18 Scorpii {Fact} 45.7 LY 16h 15m 37s UNSC HQ base on world. UNSC {TCP:p351} {Fact} -08° 22' 06" recruitment center in the city of Halkia. {TCP:p355} Constellation: Scorpio 111 Tauri 111 Tauri {Fact} 47.8 LY 05h:24m:25.46s Diameter: 1,654,100km (1.19R*) {Fact} +17° 23' 00.72" {Fact} Spectral Class: F8 V {Fact} Surface Temp.: 6,200K {Fact} Constellation: Taurus 111 Tauri ?? (Victoria) 111 Tauri {Fact} 47.8 LY 05:24:25.4634 UNSC colony. {GoO:p31} {Fact} +17° 23' 00.72" Constellation: Taurus Location of a rebel cell at Camp New Hope in 2531. {GoO:p31} 51 Pegasi {Fact} 51 Pegasi {Fact} 50.1 LY 22h:57m:28s Diameter: 1,668,000km (1.2R*) {Fact} +20° 46' 7.8" {Fact} Spectral Class: G4 (yellow- orange) {Fact} Surface Temp.: Constellation: Pegasus 51 Pegasi-B (Bellerophon) 51 Pegasi 50.1 LY 22h:57m:28s Gas giant planet in the 51 Pegasi {Fact} +20° 46' 7.8" system informally named Bellerophon. Diameter: 196,000km. {Fact} Located on the edge of UNSC territory. {GoO:p15} Its moon, Pegasi Delta, contained a Covenant deuterium/tritium refinery destroyed by covert UNSC forces in 2545. {GoO:p13} Constellation: Pegasus 51 Pegasi-B-1 (Pegasi 51 Pegasi 50.1 LY 22h:57m:28s Moon of the gas giant planet 51 Delta) {GoO:p13} +20° 46' 7.8" Pegasi-B in the 51 Pegasi star Constellation: Pegasus system; a Covenant stronghold on the edge of UNSC territory. -
Interpreting the Sky
INTERPRETING THE SKY . by. _ Von Del Chamberlain ~ational Ai~ and Space Museum Smithsonian Institution INTERPRETING THE SKY ~ Von Del Chamberlain Smithsonian Institution "Two things fill ~y mind with ever new and ever greater wonder and reverence, the oftener and the longer I allc~ my nind to dwell on them-- The starry heavens above a~d the moral law within me." Kant SKY !~--:'ERPRETATION is the art in process of coupling direct observation with skilled comrnunicatio~ for the pur- pose of informing people abou~ the sky, its objects and phenomena, with special emphasis upon relationships of these to Earth and its occupants. This paper is intended to introduce you to a realm of natural interpretation which has been · generally neglected in interpretative work . It will not be possible ·here to give detailed instruction about sky pheno~ena, but only to start you thinking about the importance of the sky in natural history interpretation and to make you aware of some useful procedures and materials. Suggestions will be offered which, if followed will start yo~ on your way to become an effective sky interpreter, 2 adding to your comprehensive ability as a naturalist. You will find a study guide and selected reference at the end of the_ paper . These will guide you in your study of selected sources of up~to-date information needed to become knowledgeable of the sky and its extremely interesting objects and events. I. WHY INTERPRET THE SKY? "To a person uninstructed in natural history, his country or seaside stroll is a walk through a gallery filled with wonderful works of art, nine-tenths of which have their faces turned to the wall." Thomas Henry Huxley Interpreters seldom, if ever, question the relevance of biology, geology and ecology in their work. -
The Stars Education
The Stars Student activities 5-10 Student activities Activity 5: Make your own planisphere Background information Star observations With the naked eye, we are able to see about 3000 stars on a clear night (with minimum light pollution). Through a small telescope we are able to see about 6000 stars. A planisphere is a flat map of the stars that can be used as a guide to help identify constellations and individual stars in the night sky. Planispheres can be used for any time of night throughout the year, but are made for use in a particular location (eg. Melbourne/central Victoria). On a clear night, the colour of different stars may become more apparent. The colour of a star can tell you something about its temperature. If you put a piece of metal into a fire, it will first glow a faint red colour, then as it gets hotter, it becomes redder and, if it doesn’t melt, it will turn yellow, then white, then blue/white. In the same way, the blue flame from a Bunsen burner is hotter and more dangerous than a red/yellow flame. The metal rod and the gas in the Bunsen burner have no colour of their own but change colour depending on their temperature. This is the same with stars. Cooler stars (with temperatures around 3,000K) glow red, while hotter stars (with temperatures around 10,000K) glow blue/white. Our Sun is a yellow star because it has a temperature of 5,800K. Stars to look out for Betelgeuse is a red supergiant star in the constellation of Orion. -
Tổ Chức Sinh Hoạt Tập
TỔ CHỨC SINH HOẠT TẬP THỂ Sinh hoạt tập thể là một yếu tố chính để duy trì và phát triển các phong trào và đoàn thể thanh thiếu niên, nhưng ít anh chị Phụ trách nào nắm bắt được cốt lõi của những sự việc hay phải làm gì khi tổ chức sinh hoạt tập thể. Các em đã quá mệt mỏi với những bài vở, lý thuyết ở trong nhà trường rồi, nếu khi đến sinh hoạt mà gặp một anh chị Phụ trách cứ thao thao bất tuyệt hay một anh chị Phụ trách độc diễn suốt buổi sinh hoạt, chúng tôi tin rằng khó tồn tại lâu dài. Để cho các em có thể “tiêu hóa” được những bài học về đạo đức, nhân bản, luân lý... chúng ta nên biến những bài học đó thành những bài ca, điệu múa, vở kịch hay trò chơi. Những hoạt động này không những giúp cho các em tiếp thu bài học một cách thoải mái, tự nhiên, mà còn giúp cho các em được vui chơi thư giãn. Nhưng làm thế nào để cho những hoạt động như: ca hát, nhảy múa, vui chơi... đạt được hiệu quả cao? Chúng tôi xin mời các bạn tham khảo các phần sau đây: Ca hát Trong sinh hoạt của các phong trào thanh thiếu niên, ca hát là một hoạt động chủ lực không thể thiếu, vì nó nói lên được sức mạnh, sự đoàn kết, vui tươi và trẻ trung của đoàn thể đó. Ca hát là giáo dục bằng truyền cảm, là bộc lộ tâm tình của mình bằng ngôn ngữ của âm thanh và nhịp điệu. -
Annualreport
2 17 ANNUALREPORT 17 20 TABLEOFCONTENTS 1 Trustee’s Update 2 Director’s Update 3 Science Highlights 30 Technical Support Highlights 34 Development Highlights 37 Public Program Highlights 40 Putnam Collection Center Highlights 41 Communication Highlights 43 Peer-Reviewed Publications 49 Conference Proceedings & Abstracts 59 Statement of Financial Position TRUSTEE’SUPDATE By W. Lowell Putnam About a decade ago the phrase, unique, enriching and transformative “The transformational effect of the as well. We are committed to building DCT”, started being used around the on that in all that we are doing going Observatory. We were just beginning forward. to understand that a 4 meter class We are not the only growing entity telescope was going to be more in the Flagstaff area. There has seen impactful than our original, and naïve, substantial growth at NAU, at our other concept of “2x the Perkins”. Little did we partner institutions and in the number know then, and we are still learning just of high technology, for-profit business in how transforming the DCT has been. the region. This collective growth is now As you read Jeff’s report and look creating opportunities for collaboration through the rest of this report you can and partnerships that did not exist a begin to see the results in terms of decade ago. We have the potential scientific capability and productivity. to do things that we would not have The greater awareness of Lowell on considered even a few years ago. The the regional and national level has challenge will be doing them in ways also lead to the increases in the public that keep the Observatory the collegial program, and the natural progression and collaborative haven that it has to building a better visitor program and always been. -
A Directory of Otherkin Writings and Other Works, Organized by Topic
A Directory of Otherkin Writings and other works, organized by topic Collected by O. Scribner Version 0.6 – Updated 2012-09-08 Project created 2011-05-07 This free eBook is RATED PG-13 for occasional profanity and references to adult concepts. This document is safe for work, but some links lead to web-sites that are not. (cc by-nc-sa) 2011 by O. Scribner Creative Commons license: Attribution, Non-Commercial, Share Alike (cc by-nc-sa) This means that you have permission to download, share, and print this free e-book, so long as you credit O. Scribner as the original author, and don’t sell it or make money off it. You can even modify this e-book, on the condition that you share it under identical terms. Original file location: http://orion.kitsunet.net By O. Scribner – 2 Summary This document serves as a guide for finding writings or artwork in many websites and books about a variety of topics related to otherkin, therianthropes, and similar peoples. This directory cites or links to works by over 500 different authors and artists, who come from inside as well as outside the community. These aren’t limited to English. This directory also lists translations and original works in 15 other languages. If you’re wondering about any topic that any otherkin or therians have ever discussed, you will probably find several essays on that topic here, each offering a different answer. Use these references to support your own original writings. If you don’t find an essay there, then you’ve found a niche to write new things into. -
Observing List
day month year Epoch 2000 local clock time: 2.00 Observing List for 17 11 2019 RA DEC alt az Constellation object mag A mag B Separation description hr min deg min 58 286 Andromeda Gamma Andromedae (*266) 2.3 5.5 9.8 yellow & blue green double star 2 3.9 42 19 40 283 Andromeda Pi Andromedae 4.4 8.6 35.9 bright white & faint blue 0 36.9 33 43 48 295 Andromeda STF 79 (Struve) 6 7 7.8 bluish pair 1 0.1 44 42 59 279 Andromeda 59 Andromedae 6.5 7 16.6 neat pair, both greenish blue 2 10.9 39 2 32 301 Andromeda NGC 7662 (The Blue Snowball) planetary nebula, fairly bright & slightly elongated 23 25.9 42 32.1 44 292 Andromeda M31 (Andromeda Galaxy) large sprial arm galaxy like the Milky Way 0 42.7 41 16 44 291 Andromeda M32 satellite galaxy of Andromeda Galaxy 0 42.7 40 52 44 293 Andromeda M110 (NGC205) satellite galaxy of Andromeda Galaxy 0 40.4 41 41 56 279 Andromeda NGC752 large open cluster of 60 stars 1 57.8 37 41 62 285 Andromeda NGC891 edge on galaxy, needle-like in appearance 2 22.6 42 21 30 300 Andromeda NGC7640 elongated galaxy with mottled halo 23 22.1 40 51 35 308 Andromeda NGC7686 open cluster of 20 stars 23 30.2 49 8 47 258 Aries 1 Arietis 6.2 7.2 2.8 fine yellow & pale blue pair 1 50.1 22 17 57 250 Aries 30 Arietis 6.6 7.4 38.6 pleasing yellow pair 2 37 24 39 59 253 Aries 33 Arietis 5.5 8.4 28.6 yellowish-white & blue pair 2 40.7 27 4 59 239 Aries 48, Epsilon Arietis 5.2 5.5 1.5 white pair, splittable @ 150x 2 59.2 21 20 46 254 Aries 5, Gamma Arietis (*262) 4.8 4.8 7.8 nice bluish-white pair 1 53.5 19 18 49 258 Aries 9, Lambda Arietis -
The Sky Tonight April
horse. Sources differ on which centaur the APRIL PAENGA-WHĀ WHĀ HIGHLIGHTS constellation represents, but most consider it to be Chiron, who mentored many Greek THE SKY TONIGHT heroes. Centaurus was one of the 48 - - - constellations described in the 2nd century TE AHUA O TE RAKI I TENEI PO by astronomer Ptolemy, and it remains one Omega Centauri of the 88 modern constellations. Originally thought to be a single star, in 1677, this fuzzy spot was identified to High in the southeast, you will find two be a cluster that actually contains around bright stars that appear close together, 10 million individual stars. Pictured on called Alpha Centauri and Beta Centauri. the cover, Omega Centauri is a globular These stars mark the two front legs of the cluster: a collection of stars that orbits a centaur, and also act as the pointer stars galactic core. This is the largest of these in to help find the Southern Cross. the Milky Way, with light taking 150 years to travel from one edge to the other. Omega Centauri has a mass four million times that of our Sun, making it also the Image: Johannes Hevelius – Wikimedia Commons most massive cluster in our galaxy. The light coming from the millions of stars in the cluster has travelled for 15 800 years to reach us here on Earth. As this cluster is most easily seen from April to September, now is the time to start looking for it. Brighter than any other star cluster, Omega Centauri can currently be found high in the southeastern sky, along the back of the constellation Centaurus.