Skywatch Number 67 (New Series) : Two Eyes

Total Page:16

File Type:pdf, Size:1020Kb

Skywatch Number 67 (New Series) : Two Eyes Amateur Astronomy WITH AN ATTITUDE from Chaos Manor South! Rod Mollise’s March-April 2003 Volume 12, Issue 2 “A Newsletter for the Truly Outbound!” Skywatch Number 67 (New Series) : two eyes. Only when it’s time to look <[email protected]> through a telescope do we squint Great, Huge one closed and look at the universe Inside this Issue: through a single peeper. This is SUPERSIZED uncomfortable, and, since our brain is used to getting the input from two eyes, we lose detail. A binoviewer is How I Learned to Stop Issue! the supposed cure. It’s a device that Worrying and Love uses prisms to take the light coming 1 Binoviewers! from your lenses and mirrors, split it, and direct the image into two Lucy Looks Skyward! How I learned to eyepieces. Put one of these on your 2 scope and you can view the Stop Worrying wonders of the heavens through two The EyeOpener! eyes as nature intended. 3 and Love Too bad this idea didn’t seem to MX7C Conversion! work well—at least not for me. Many 4 Binoviewers were the times I’d been offered the Confessions of an Astromart chance to use a binoviewer, given it Junkie! a try, and come away shaking my Denkmeier Optical, Inc. 5 head at the idea anybody could like 100 Pinehurst Road one of these things. Didn’t seem to Berlin, MD 21811 Lunar Software! matter which brand I tried, either, Information:(410)208-6014 Toll-Free 6 including expensive TeleVues and Order Line: (866)340-4578 AP branded units. I just couldn’t 7 Space Place! http://deepskybinoviewer.com/ seem to get one to work for me. I’d look strain, adjust the interocular don’t make any secret of how distance (you can adjust the My Back Pages! much I love astro-gear. separation between a binoviewer’s 78 Anything—telescopes, eyepieces, I eyepieces just as you can with a charts, computer programs, packs pair of binoculars), focus, squint, of lens tissue. I don’t care. But there was one piece of amateur astronomy equipment that I just hadn’t been able to stomach: binoviewers. If you spend any time at star parties, you’ve seen binoviewers. They Skywatch are those binocular 1207 Selma Street viewing attachments Mobile, AL 36604 you’ll often find U.S.A. mounted in the focusers of big dobs or monster SCTs. In theory, it’s a good idea. We normally view our world through . strain some more and always wind impressed by the design of the unit. backyard, and got Saturn in the field up with two separate images. I In order to attach the focus tube to of view. I inserted the Denkmeier couldn’t get my eyes and brain to the binoviewer, TeleVue uses a into my 2” diagonal and popped in merge the pictures into one. And system of fussy adapter rings. two eyepieces (the only identical based on the comments of other These can be a real hassle if you oculars I could find were two 25mm folks who’ve used binoviewers, this have to remove them, as Pat Kellners of dubious heritage). OK, problem, while not common, ain’t Rochford and I discovered one let’s get this over with. I put my eyes exactly unheard of, either. After a evening when we unscrewed the to the eyepieces, focused and… while, I learned just to take a quick adapters from his TV, got ‘em back Yep. Two Saturns. I could feel a look through a BV when offered, on wrong, and basically ruined ‘em headache comin’ on already. I mutter something like, “cool!” or to the tune of 60 bucks (we adjusted the interocular spacing a “nice!” and head back to my single- threaded one ring into the wrong bit (the Denkmeier “folds” in the eyepiece scope as soon as politely part and couldn’t remove it). In middle like a pair of binoculars), possible. contrast, 1.25” and 2” focus tubes focused the big SCT a little and. thread right onto the body of the ALL OF A SUDDEN I WAS SEEING And there things stood for quite a Denkmeier binoviewer, with no ONE, BEAUTIFUL IMAGE! while. I didn’t bother binoviewers, adapters required. There’s plenty of and they didn’t bother me. Until one room in the carrying case for I could hardly believe it! After about day when I got an email from the binoviewer, StarSweeper, focus 5 minutes of use, I even found that I good folks at Denkmeier Optical. tubes and more. This foam-padded couldn’t force myself into seeing two Seems as how they’d heard some case appears to be designed to hold separate images. What a revelation. comments about my problems with a pistol (the eagle embossed on the Why was it so easy with the binoviewing, and wanted me to give case cover makes its sporting goods Denkmeier when I’d had such a one of their “Deep Sky Binoviewers” heritage clear), but it’s a nice touch hard time with other binoviewers? a try. I was a little hesitant. Like I and works great. Maybe because I was able to relax said, I like gear, and being able to and use the BV on my own scope, a give new stuff a try is one of my Was there anything I didn’t like right comfortable SCT rather than a favorite pastimes. But I really wasn’t off the bat? The friction fit eyepiece ladder-equipped dobsonian. But I sure I wanted to bother with tubes. Rather than locks of some don’t think that’s the whole story. I something I knew I wouldn’t like. kind to hold your eyepieces in place, didn’t have any trouble when I tried But, in the end, I just couldn’t resist. the Standard Denkmeier uses the Denkmeier in Pat Rochford’s big I told Russ at Denkmeier to send friction fit tubes that hold both Dobsonian either. Talking to the one on, but not to be disappointed if eyepieces in place with the aid of O folks at Denkmeier, they stated that I hated the Denkmeier as much as I rings. I like my eyepieces to be they take special pains in the design did the rest of the pack. Russ was secure and tight, so I wasn’t overly and alignment of their units to unphased, and pretty much told me happy with this arrangement. It did preclude problems with image that he guaranteed I’d like his baby. seem to work OK, however. The merging. I guess I’ll have o believe Yeah. Right. eyepieces didn’t fall out and I was ‘em, since their binoviewer worked able to slide both in and out of the so well for me! Before I knew it, there was a sizable tubes for differential focus and they box sitting on the dining room table. stayed put. But it still seemed a less But beyond being able to merge Opening this parcel revealed a well- than ideal situration. This is actually images, what did I think? While the packed black-plastic carrying case a non-issue now, as Russ informed Denkmeier is billed as the “Deep containing the Standard Denkmeier me shortly after I received the eval Sky Binoviewer,” it was doing one Binoviewer ($599.00), the unit that all future Standard and heck of a job on Saturn. I’m not sure StarSweeper focal reducer for SCTs Premium Denkmeier BVs would I could see more with the two cheap ($149.00), and all necessary tubes indeed include locking, self- Kellners than I could when I and adapters to allow use of the centering eyepiece holders. switched in my single 22mm binoviewer in 1.25” or 2” focusers Panoptic. But I could easily see as (you’ll need a 2” setup for your SCT Looked nice. Yeah. But I doubted much and without as much effort. in order to use the StarSweeper). I that I’d be able to use this thing, so, And there was the added bonus of was immediately impressed by the so what? A glance out one of Chaos the binoviewer’s pseudo 3-D effect. quality of the Denkmeier’s Manor South’s kitchen revealed that When using this or any binoviewer, construction. It seemed even more the coming evening would be clear, there’s not nearly enough solid than the (more expensive) something that’s been rare this separation between your eyes when TeleVue, which has formerly been Winter, though, so I decided to give viewing a distant object like a planet something of a benchmark in the the blasted thing a try. I grabbed the to produce a real 3-D effect. But world of BVs. I was further binoviewer, set the C11 up in the 2 . Skywatch your brain doesn’t believe this. It’s the help of my buddy, Pat Rochford. binoviewer and OCS. We were very seeing through two eyes, so there Pat, as mentioned earlier, is a curious to see what the effect would must be depth. The way my brain Binoviewer user and is set up with a be on field-edge quality in this fast perceived things, Saturn was in the full range of eyepiece focal lengths. scope. After a little fumbling around midground, Titan was in the When the bubbas at Denkmeier to get the OCS adjusted to the point background, and a couple of the heard that I was takin’ their baby where the scope would come to other little moons were in the over to Pat’s to try under his fairly focus (the OCS barrel is adjustable foreground.
Recommended publications
  • Naming the Extrasolar Planets
    Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named.
    [Show full text]
  • A Basic Requirement for Studying the Heavens Is Determining Where In
    Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun­ damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short).
    [Show full text]
  • Meeting Announcement Astro-Imaging Special Interest
    CVAS Executive Committee Pres – Dell Vance - (435) 938-8328 Loaner Scope Coordinator/NSN Coordinator – [email protected] Garrett Smith – [email protected] Vice Pres- Layne Pedersen – (801) 463-1701 Past President, Webmaster, Librarian – [email protected] Tom Westre – (435) 787-6380 [email protected] Treasurer- Brad Kropp - (435) 755-0877 Public Relations – Lyle Johnson - [email protected] Secretary – Dale Hooper - (435) 563-0608 [email protected] Vol. 5 Number 7 March 2018 www.cvas-utahskies.org Meeting Announcement With that in mind, I was able to travel down to Goblin Valley and Arches National Park during Our March meeting will be held on the fourth February. I took my binoculars and my camera Wednesday, March 28, 2018 at 7pm in room 840 along, because these areas are known for their dark of the main BATC campus. We have room 840 skies. It was a couple of days before a new moon so for the rest of this year. Enter on the east side of the the skies should be great. At Arches NP bookshop, I building located at 1301 North 600 West. found a book titled “Photography NIGHT SKY” by Our featured speaker this month is club member Garrett Smith. He will be sharing with us a presentation about the king of planets, Jupiter. Astro-Imaging Special Interest Group The Astro-Imaging SIG will have a kick-off meeting at the Logan Library in the Temple Fork room at 7pm on March 15th. Please contact Tom at 435-787- 6380 if you are interested. The President’s Corner By Dell Vance, CVAS President Jennifer Wu and James Martin.
    [Show full text]
  • An Aboriginal Australian Record of the Great Eruption of Eta Carinae
    Accepted in the ‘Journal for Astronomical History & Heritage’, 13(3): in press (November 2010) An Aboriginal Australian Record of the Great Eruption of Eta Carinae Duane W. Hamacher Department of Indigenous Studies, Macquarie University, NSW, 2109, Australia [email protected] David J. Frew Department of Physics & Astronomy, Macquarie University, NSW, 2109, Australia [email protected] Abstract We present evidence that the Boorong Aboriginal people of northwestern Victoria observed the Great Eruption of Eta (η) Carinae in the nineteenth century and incorporated the event into their oral traditions. We identify this star, as well as others not specifically identified by name, using descriptive material presented in the 1858 paper by William Edward Stanbridge in conjunction with early southern star catalogues. This identification of a transient astronomical event supports the assertion that Aboriginal oral traditions are dynamic and evolving, and not static. This is the only definitive indigenous record of η Carinae’s outburst identified in the literature to date. Keywords: Historical Astronomy, Ethnoastronomy, Aboriginal Australians, stars: individual (η Carinae). 1 Introduction Aboriginal Australians had a significant understanding of the night sky (Norris & Hamacher, 2009) and frequently incorporated celestial objects and transient celestial phenomena into their oral traditions, including the sun, moon, stars, planets, the Milky Way and Magellanic Clouds, eclipses, comets, meteors, and impact events. While Australia is home to hundreds of Aboriginal groups, each with a distinct language and culture, few of these groups have been studied in depth for their traditional knowledge of the night sky. We refer the interested reader to the following reviews on Australian Aboriginal astronomy: Cairns & Harney (2003), Clarke (1997; 2007/2008), Fredrick (2008), Haynes (1992; 2000), Haynes et al.
    [Show full text]
  • Astronomy 2009 Index
    Astronomy Magazine 2009 Index Subject Index 1RXS J160929.1-210524 (star), 1:24 4C 60.07 (galaxy pair), 2:24 6dFGS (Six Degree Field Galaxy Survey), 8:18 21-centimeter (neutral hydrogen) tomography, 12:10 93 Minerva (asteroid), 12:18 2008 TC3 (asteroid), 1:24 2009 FH (asteroid), 7:19 A Abell 21 (Medusa Nebula), 3:70 Abell 1656 (Coma galaxy cluster), 3:8–9, 6:16 Allen Telescope Array (ATA) radio telescope, 12:10 ALMA (Atacama Large Millimeter/sub-millimeter Array), 4:21, 9:19 Alpha (α) Canis Majoris (Sirius) (star), 2:68, 10:77 Alpha (α) Orionis (star). See Betelgeuse (Alpha [α] Orionis) (star) Alpha Centauri (star), 2:78 amateur astronomy, 10:18, 11:48–53, 12:19, 56 Andromeda Galaxy (M31) merging with Milky Way, 3:51 midpoint between Milky Way Galaxy and, 1:62–63 ultraviolet images of, 12:22 Antarctic Neumayer Station III, 6:19 Anthe (moon of Saturn), 1:21 Aperture Spherical Telescope (FAST), 4:24 APEX (Atacama Pathfinder Experiment) radio telescope, 3:19 Apollo missions, 8:19 AR11005 (sunspot group), 11:79 Arches Cluster, 10:22 Ares launch system, 1:37, 3:19, 9:19 Ariane 5 rocket, 4:21 Arianespace SA, 4:21 Armstrong, Neil A., 2:20 Arp 147 (galaxy pair), 2:20 Arp 194 (galaxy group), 8:21 art, cosmology-inspired, 5:10 ASPERA (Astroparticle European Research Area), 1:26 asteroids. See also names of specific asteroids binary, 1:32–33 close approach to Earth, 6:22, 7:19 collision with Jupiter, 11:20 collisions with Earth, 1:24 composition of, 10:55 discovery of, 5:21 effect of environment on surface of, 8:22 measuring distant, 6:23 moons orbiting,
    [Show full text]
  • HIFISTARS Herschel/HIFI Observations of VY Canis Majoris. Molecular-Line Inventory of the Envelope Around the Largest Known Star
    Chalmers Publication Library HIFISTARS Herschel/HIFI observations of VY Canis Majoris. Molecular-line inventory of the envelope around the largest known star This document has been downloaded from Chalmers Publication Library (CPL). It is the author´s version of a work that was accepted for publication in: Astronomy and Astrophysics (ISSN: 0004-6361) Citation for the published paper: Alcolea, J. ; Bujarrabal, V. ; Planesas, P. (2013) "HIFISTARS Herschel/HIFI observations of VY Canis Majoris. Molecular-line inventory of the envelope around the largest known star". Astronomy and Astrophysics, vol. 559 pp. (article nr.) A93. http://dx.doi.org/10.1051/0004-6361/201321683 Downloaded from: http://publications.lib.chalmers.se/publication/192302 Notice: Changes introduced as a result of publishing processes such as copy-editing and formatting may not be reflected in this document. For a definitive version of this work, please refer to the published source. Please note that access to the published version might require a subscription. Chalmers Publication Library (CPL) offers the possibility of retrieving research publications produced at Chalmers University of Technology. It covers all types of publications: articles, dissertations, licentiate theses, masters theses, conference papers, reports etc. Since 2006 it is the official tool for Chalmers official publication statistics. To ensure that Chalmers research results are disseminated as widely as possible, an Open Access Policy has been adopted. The CPL service is administrated and maintained by Chalmers Library. (article starts on next page) A&A 559, A93 (2013) Astronomy DOI: 10.1051/0004-6361/201321683 & c ESO 2013 Astrophysics HIFISTARS Herschel/HIFI observations of VY Canis Majoris, Molecular-line inventory of the envelope around the largest known star J.
    [Show full text]
  • A Radial Velocity Survey of Low Galactic Latitude Structures: II. the Monoceros Ring Behind the Canis Major Dwarf Galaxy
    Mon. Not. R. Astron. Soc. 000, 1–5 (2005) Printed 15 September 2018 (MN LaTEX style file v2.2) A radial velocity survey of low Galactic latitude structures: II. The Monoceros Ring behind the Canis Major dwarf galaxy Blair C. Conn1, Nicolas F. Martin2,4, Geraint F. Lewis1, Rodrigo A. Ibata2, Michele Bellazzini3 & Mike J. Irwin4 1Institute of Astronomy, School of Physics, A29, University of Sydney, NSW 2006, Australia: Email [email protected], [email protected] 2Observatoire de Strabourg, 11, rue de l’Universit´e, F-67000, Strasbourg, France: Email [email protected], [email protected] 3INAF - Osservatorio Astronomico di Bologna, Via Ranzani 1, 40127, Bologna, Italy: Email [email protected] 4Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, U.K.: Email [email protected] 15 September 2018 ABSTRACT An AAT/2dF Spectrograph Survey of low Galactic latitudes targeting the putative Canis Major dwarf galaxy, and the (possibly) associated tidal debris of stars known as the Monoceros Ring, covering Galactic coordinates 231.5◦ < l < 247.5◦ and -11.8◦ <b<-3.8◦, has revealed the presence of the Monoceros Ring in the background of the Canis Major dwarf galaxy. This detection resides at a galactocentric distance of ∼18.9±0.3kpc (13.5±0.3kpc heliocentric), exhibiting a velocity of ∼132.8±1.3 kms−1 with a dispersion of ∼22.7±1.7 kms−1; both of these comparable with previous measurements of the Monoceros Ring in nearby fields. This detection highlights the increasing complexity of structure being revealed in recent surveys of the Milky Way thick disk and Halo.
    [Show full text]
  • One of the Most Useful Accessories an Amateur Can Possess Is One of the Ubiquitous Optical Filters
    One of the most useful accessories an amateur can possess is one of the ubiquitous optical filters. Having been accessible previously only to the professional astronomer, they came onto the marker relatively recently, and have made a very big impact. They are useful, but don't think they're the whole answer! They can be a mixed blessing. From reading some of the advertisements in astronomy magazines you would be correct in thinking that they will make hitherto faint and indistinct objects burst into vivid observ­ ability. They don't. What the manufacturers do not mention is that regardless of the filter used, you will still need dark and transparent skies for the use of the filter to be worthwhile. Don't make the mistake of thinking that using a filter from an urban location will always make objects become clearer. The first and most immediately apparent item on the downside is that in all cases the use of a filter reduces the amount oflight that reaches the eye, often quite sub­ stantially. The brightness of the field of view and the objects contained therein is reduced. However, what the filter does do is select specific wavelengths of light emitted by an object, which may be swamped by other wavelengths. It does this by suppressing the unwanted wavelengths. This is particularly effective in observing extended objects such as emission nebulae and planetary nebulae. In the former case, use a filter that transmits light around the wavelength of 653.2 nm, which is the spectral line of hydrogen alpha (Ha), and is the wavelength oflight respons­ ible for the spectacular red colour seen in photographs of emission nebulae.
    [Show full text]
  • Deepsky Delights
    deepsky delights Deepsky Delights glow” of the Sun. However, this night by Magda Streicher belonged to Caroline Herschel. [[email protected]] Caroline (1750–1848) although small in stature was more than just a remarkable Caroline Herschel’s woman. Her unselfishness and consist- deepsky discoveries ent assistance enabled her brother Wil- Just before midnight one evening this liam and nephew John, to give the astro- past October I walked out under an ex- nomical world a rich heritage. William ceptionally dark and transparent sky, in turn equipped her with a telescope and filled with starlight. I gazed up and was encouraged her to hunt for comets. With amazed to see a very soft, large glow great perseverance and during freezing between the constellations Aquarius and cold nights in winter she found 8 comets Pisces. This very rare sight later turned and a hand-full of deepsky objects. This out to be the Gegenschein, the “counter surely must have highlighted her lonely world. The first object I turned to was NGC 6633 in Ophui- chus, with the constellation already descending in the West. My first impression revealed a bright grouping of stars of various magni- tudes. The centre exhib- ited a few brighter stars in the shape of a semi-circle, along with a faint uneven string of stars to the east that drapes from North to South. Concluding the ob- servation was a very tight group of six stars to the west. Members of queen Cas- siopeia’s crown can be seen low on the northern hori- Caroline’s Cluster: NGC 2360 in Canis Major was dis- zon where they only bow covered in the late 18th century by Caroline Herschel.
    [Show full text]
  • February 2019 BRAS Newsletter
    Monthly Meeting February 11th at 7PM at HRPO (Monthly meetings are on 2nd Mondays, Highland Road Park Observatory). Speaker: Chris Desselles on Astrophotography What's In This Issue? President’s Message Secretary's Summary Outreach Report Astrophotography Group Asteroid and Comet News Light Pollution Committee Report Recent BRAS Forum Entries Messages from the HRPO Science Academy International Astronomy Day Friday Night Lecture Series Globe at Night Adult Astronomy Courses Nano Days Observing Notes – Canis Major – The Great Dog & Mythology Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society Newsletter of the Baton Rouge Astronomical Society February 2019 © 2019 President’s Message The highlight of January was the Total Lunar Eclipse 20/21 January 2019. There was a great turn out at HRPO, and it was a lot of fun. If any of the members wish to volunteer at HRPO, please speak to Chris Kersey, BRAS Liaison for BREC, to fill out the paperwork. MONTHLY SPEAKERS: One of the club’s needs is speakers for our monthly meetings if you are willing to give a talk or know of a great speaker let us know. UPCOMING BRAS MEETINGS: Light Pollution Committee - HRPO, Wednesday, February 6, 6:15 P.M. Business Meeting – HRPO, Wednesday, February 6, 7 P.M. Monthly Meeting – HRPO, Monday, February 11, 7 P.M. VOLUNTEERS: While BRAS members are not required to volunteer, if we do grow our volunteer core in 2019 we can do more fun activities without wearing out our great volunteers. Volunteering is an excellent opportunity to share what you know while increasing your skills.
    [Show full text]
  • Annual Report 2009 ESO
    ESO European Organisation for Astronomical Research in the Southern Hemisphere Annual Report 2009 ESO European Organisation for Astronomical Research in the Southern Hemisphere Annual Report 2009 presented to the Council by the Director General Prof. Tim de Zeeuw The European Southern Observatory ESO, the European Southern Observa­ tory, is the foremost intergovernmental astronomy organisation in Europe. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. Several other countries have expressed an interest in membership. Created in 1962, ESO carries out an am­ bitious programme focused on the de­ sign, construction and operation of power­ ful ground­based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world­ View of the La Silla Observatory from the site of the One of the most exciting features of the class observing sites in the Atacama 3.6 ­metre telescope, which ESO operates together VLT is the option to use it as a giant opti­ with the New Technology Telescope, and the MPG/ Desert region of Chile: La Silla, Paranal ESO 2.2­metre Telescope. La Silla also hosts national cal interferometer (VLT Interferometer or and Chajnantor. ESO’s first site is at telescopes, such as the Swiss 1.2­metre Leonhard VLTI). This is done by combining the light La Silla, a 2400 m high mountain 600 km Euler Telescope and the Danish 1.54­metre Teles cope.
    [Show full text]
  • Dave Mitsky's Monthly Celestial Calendar
    Dave Mitsky’s Monthly Celestial Calendar January 2010 ( between 4:00 and 6:00 hours of right ascension ) One hundred and five binary and multiple stars for January: Omega Aurigae, 5 Aurigae, Struve 644, 14 Aurigae, Struve 698, Struve 718, 26 Aurigae, Struve 764, Struve 796, Struve 811, Theta Aurigae (Auriga); Struve 485, 1 Camelopardalis, Struve 587, Beta Camelopardalis, 11 & 12 Camelopardalis, Struve 638, Struve 677, 29 Camelopardalis, Struve 780 (Camelopardalis); h3628, Struve 560, Struve 570, Struve 571, Struve 576, 55 Eridani, Struve 596, Struve 631, Struve 636, 66 Eridani, Struve 649 (Eridanus); Kappa Leporis, South 473, South 476, h3750, h3752, h3759, Beta Leporis, Alpha Leporis, h3780, Lallande 1, h3788, Gamma Leporis (Lepus); Struve 627, Struve 630, Struve 652, Phi Orionis, Otto Struve 517, Beta Orionis (Rigel), Struve 664, Tau Orionis, Burnham 189, h697, Struve 701, Eta Orionis, h2268, 31 Orionis, 33 Orionis, Delta Orionis (Mintaka), Struve 734, Struve 747, Lambda Orionis, Theta-1 Orionis (the Trapezium), Theta-2 Orionis, Iota Orionis, Struve 750, Struve 754, Sigma Orionis, Zeta Orionis (Alnitak), Struve 790, 52 Orionis, Struve 816, 59 Orionis, 60 Orionis (Orion); Struve 476, Espin 878, Struve 521, Struve 533, 56 Persei, Struve 552, 57 Persei (Perseus); Struve 479, Otto Struve 70, Struve 495, Otto Struve 72, Struve 510, 47 Tauri, Struve 517, Struve 523, Phi Tauri, Burnham 87, Xi Tauri, 62 Tauri, Kappa & 67 Tauri, Struve 548, Otto Struve 84, Struve 562, 88 Tauri, Struve 572, Tau Tauri, Struve 598, Struve 623, Struve 645, Struve
    [Show full text]