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Planetary Research Center Lowell Observatory Flagstaff, Arizona 86002
N 8 4 - °1* R 7 <• PLANETARY RESEARCH CENTER LOWELL OBSERVATORY FLAGSTAFF, ARIZONA 86002 NASA GRANT NSG-7530 POST-MISSION VIKING DATA ANALYSIS FINAL REPORT ; SUBMITTED: 26 APRIL M-A,- BAUM-- ' KARI_LUMME .__ PRINCIPAL-INVESTIGATOR< -? CO-^INVESTIGATOR J, .WTIN -• LAWRENCE H, WASSERMAN CO-INVESTIGATOR CO-INVESTIGATOR Page 2 PERSONNEL—" Averaged over the time interval (3.7 years) that funds were expended under this grant, the following staff devoted the indicated percentages of their time to it: W. A. Baum, Principal Investigator, 18$ time L. J. Martin, Co-Investigator, 52% K. Lumme, Co-Investigator, 19% L. H. Wasserman, Co-Investigator, S% T. J. Kreidl, Computer Programmer, 5% Others (combined), ResearctuAssistants, 7-$ • ~ -> "Others" include H. S. Horstman, M. L. Kantz, and S. E. Jones. In addition, there are several Observatory employees paid through overhead who provide services such as library, bookkeeping, and maintenance. BACKGROUND Work under this grant was a continuation of our participation in the Viking Mission. That participation commenced in 1970 with Baum's membership on the Viking Orbiter Imaging Team and continued through the end of team operations in 1978. This grant then commenced in 1979 at the start of the Mars Data Analysis Program (MDAP). MDAP was planned by NASA as a 5-year program, and our initial MDAP proposal was scaled to that expectation and to a funding level consistent with the Mars research projects in which we were already engaged. As it turned out, there were subsequent reductions in MDAP funds, and we (like many of our colleagues at other institutions) had to adjust the scope of our Mars research projects accordingly. -
Lowell Observatory Communications Office 1400 W. Mars Hill Rd
Lowell Observatory Communications Office 1400 W. Mars Hill Rd. Flagstaff, AZ 86001 www.lowell.edu PRESS RELEASE FOR IMMEDIATE RELEASE MAY 12, 2015 ***Contact details appear below*** Image attached LOWELL OBSERVATORY TO HOST PLUTO AND BEYOND GALA ON JUNE 13 Flagstaff, Az- Lowell Observatory will host its fourth annual fundraising gala, Pluto and Beyond, on June 13. Sponsored by APS, it will take place on the campus of Northern Arizona University in Flagstaff and feature experts sharing the latest Pluto news, auctions showcasing a variety of travel packages and astronomy-themed collectibles, and live music. Proceeds support Lowell’s mission of astronomical research and outreach. Lisa Actor, Lowell’s Deputy Director for Development, said, “This will be an exciting event in this year when we’re celebrating the 85th anniversary of the discovery of Pluto at Lowell Observatory! I’m anxious to meet and personally thank the many Flagstaff area supporters of the observatory.” Pluto and Beyond kicks off with the Kuiper VIP Reception at 5:30 p.m. Presented by Blue Cross Blue Shield of Arizona, this champagne and cocktail gathering will meet in the 1899 Bar & Grill. The main event happens in the High Country Conference Center, with doors opening at 6 p.m. and a sit-down dinner served at 7:30 p.m. Afterward, experts from Lowell Observatory will discuss the astronomy news story of the year—the New Horizons spacecraft’s July approach to Pluto after an incredible nine-year journey. This program will start with a look at Clyde Tombaugh’s improbable discovery of this icy world at Lowell in 1930 and continue with the latest news from New Horizons as it prepares to capture the first-ever close-up images of Pluto’s surface. -
Pluto's Long, Strange History — in Pictures : Nature News & Comment
Pluto's long, strange history — in pictures Nature marks the 85th anniversary of the dwarf planet's discovery. Alexandra Witze 18 February 2015 Even at a distance of 5 billion kilometres, Pluto has entranced scientists and the public back on Earth. Nature looks at the history of this enigmatic world, which in July will get its first close-up visit by a spacecraft. First glimpse Lowell Observatory 18 February 1930: Farmer-turned-astronomer Clyde Tombaugh (pictured), aged 24, discovers Pluto while comparing photographic plates of the night sky at Lowell Observatory in Flagstaff, Arizona. The discovery, announced on 13 March 1930, is the culmination of observatory founder Percival Lowell’s obsessive quest to find a ‘Planet X’, the existence of which was suspected based on perturbations in Neptune’s orbit. Name game Galaxy Picture Library 1 May 1930: The Lowell Observatory announces that its favoured name for the discovery is Pluto, suggested by 11-year-old Venetia Burney (pictured) from Oxford, UK, after the Roman god of the underworld. Venetia later becomes the namesake of a student-built dust counter on NASA's New Horizons spacecraft, which is currently on its way to Pluto. Pair bond US Naval Observatory 22 June 1978: James Christy and Robert Harrington, of the US Naval Observatory's Flagstaff Station, discover Pluto’s largest moon, Charon. It is visible as a bulge (at top in left image) that regularly appears and disappears in observational images as the two bodies orbit their mutual centre of gravity1. The moon is so large relative to Pluto that the two are sometimes referred to as a binary planet. -
TENURE-TRACK Or TENURED ASTRONOMER Lowell Observatory
TENURE-TRACK or TENURED ASTRONOMER Lowell Observatory invites applications for one or more tenure-track or tenured research positions in astronomy or planetary science. We invite applicants at any career level who can build on current strengths or open new areas for Lowell. A Ph.D. in astronomy, planetary science, or a related field is required, as is an outstanding record of research and demonstrated ability or potential to obtain external research funding. Candidates are invited to describe how they would make use of our observational facilities, but we will give equal consideration to all research areas. The start date for this position is flexible but desired by Fall 2016. Lowell Observatory is an independent, non-profit research institution. Our astronomers have access to our new 4.3-meter Discovery Channel Telescope, operated in partnership with Boston University, the University of Toledo, the University of Maryland/GSFC, Northern Arizona University, Yale University, and Discovery Communications. Lowell also maintains 1.8-m, 1.1-m, and 0.9-m telescopes equipped with optical and IR imagers and spectrographs. We partner with the US Naval Observatory and the Naval Research Laboratory in the Navy Precision Optical Interferometer. Lowell offers numerous opportunities for involvement in education and outreach as well. To apply: Send applications electronically to [email protected]. Applications should include (1) a cover letter and CV, (2) a research plan of 3 pages or less, and (3) names and mail/email addresses of three individuals who have agreed to serve as references. Do not ask for reference letters to be sent in advance. -
Planetary Patrol - an International Effort
136 COMMISSIONS 16, 17 AND 40 ments devoted to the passage through the asteroid belt which precedes the Jupiter rendezvous. Emphasis was placed on the anticipated contributions of these three programs to our understanding of the solar system. In discussion Carl Sagan stressed that mission B of the Mariner Mars 1971 program is designed to have an orbital period four-thirds the Martian rotational period so that every four days the space craft observes the same area under the same lighting conditions. In this way intrinsic Martian albedo changes can be distinguished from effects due to the scattering phase function of surface material. He also mentioned the possibility that photographic mapping of Phobos and Deimos by the Mariner Mars 1971 mission would provide cartography of these moons superior to the best groundbased cartography of Mars. PLANETARY PATROL - AN INTERNATIONAL EFFORT W. A. Baum Lowell Observatory Abstract. An international photographic planetary patrol network, consisting of the Mauna Kea Observatory in Hawaii, the Mount Stromlo Observatory in eastern Australia, the Republic Observa tory in South Africa, the Cerro Tololo Inter-American Observatory in northern Chile, and the Lowell Observatory, has been in operation since April 1969. The Magdalena Peak Station of the Mexico State University also participated temporarily. New stations are now being added at the Perth Observatory in western Australia and at the Kavalur Station of the Kodaikanal Observatory in southern India. During 1969 Mars and Jupiter were photographed through blue, green, and red filters; and the network produced more than 11000 fourteen-exposure filmstrips with images of a quality suitable for analysis. -
1400 West Mars Hill Rd | Flagstaff, Arizona 86001-4499 | USA 928.774.3358 | Lowell.Edu
1400 West Mars Hill Rd | Flagstaff, Arizona 86001-4499 | USA 928.774.3358 | lowell.edu POSITION ANNOUNCEMENT Multi-Cultural Outreach Astronomer DUTIES: Serve as a Public Program Educator and act as the “Meet an Astronomer” professional for our observatory several times a month. Develop new educational materials and translate existing educational materials for the Spanish speaking community. Participate directly in the Lowell Observatory Camp for Kids programs. These hands-on day camps offer kids the opportunity to learn about STEM through activities such as science investigations, games, story time, music, engineering, art, and more. Partner with schools each year within the Native American Astronomy Outreach program and participate in expansions of that program to other cultures in the region. Partnerships are sponsored by National Science Foundation and private donors. Develop and deliver informal education talks about astronomy, with an emphasis on the most recent astronomy-related news and events, as well as the current and past research done at Lowell Observatory. Engage with visitors and lead tours of the Lowell Observatory campus including occasional tours in Spanish. Deliver public lectures for historical observatory exhibitions. Operate public telescopes, lead outdoor stargazing programs and special pre-K-12 programs. Other duties as assigned, which may include: lead tours of other Lowell telescopes and facilities, assist with design and delivery of new programs, and assist with exclusive programs both on and off-site. REQUIREMENTS: Master’s degree in Astronomy, Physics, or a closely related field or the foreign academic equivalent, plus 1 year of experience in an astronomy related position. Alternatively, Lowell will also accept Bachelor’s degree, in Astronomy, Physics, or a closely related field, with 6 years of experience in an astronomy related position in lieu of a master’s degree and 1 year of experience. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
New Horizons 2 Alan Stern (Swri), Rick Binzel (MIT), Hal Levison
New Horizons 2 Alan Stern (SwRI), Rick Binzel (MIT), Hal Levison (SwRI), Rosaly Lopes (JPL), Bob Millis (Lowell Observatory), and Jeff Moore (NASA Ames) New Horizons is the inaugural mission in NASA’s New Frontiers program—a series of mid-sized planetary exploration projects. This mission was competitively selected in 2001 after a peer review competition between industry-university teams. The mission is on track toward a planned launch in January 2006—just over 6 months hence. The primary objective of New Horizons (NH) is to make the first reconnaissance of the solar system’s farthest planet, Pluto, its comparably sized satellite Charon. If an extended mission is approved, New Horizons may be able to also flyby a Kuiper Belt Object (KBOs) farther from the Sun. The exploration of the Kuiper Belt and Pluto-Charon was ranked as the highest new start priority for planetary exploration by the National Research Council’s recently completed (2002) Decadal Survey for Planetary Science. In accomplishing its goals, the mission is expected to reveal fundamental new insights into the nature of the outer solar system, the formation history of the planets, the workings of binary worlds, and the ancient repository of water and organic building blocks called the Kuiper Belt. Beyond its scientific ambitions, New Horizons is also breaking ground in lowering the cost of exploration of the outer solar system—for it is being built and launched for what are literally dimes on the dollar compared to deep outer solar system missions like Voyager, Galileo, and Cassini. The New Horizons spacecraft carries a suite of seven advanced, miniaturized instruments to obtain detailed imagery, mapping spectroscopy, thermal mapping, gravitational data, and in situ plasma composition, density, and energy sampling of the exotic, icy Pluto- Charon binary and a modest-sized (~50 km diameter) KBO. -
Lick Observatory Records: Photographs UA.036.Ser.07
http://oac.cdlib.org/findaid/ark:/13030/c81z4932 Online items available Lick Observatory Records: Photographs UA.036.Ser.07 Kate Dundon, Alix Norton, Maureen Carey, Christine Turk, Alex Moore University of California, Santa Cruz 2016 1156 High Street Santa Cruz 95064 [email protected] URL: http://guides.library.ucsc.edu/speccoll Lick Observatory Records: UA.036.Ser.07 1 Photographs UA.036.Ser.07 Contributing Institution: University of California, Santa Cruz Title: Lick Observatory Records: Photographs Creator: Lick Observatory Identifier/Call Number: UA.036.Ser.07 Physical Description: 101.62 Linear Feet127 boxes Date (inclusive): circa 1870-2002 Language of Material: English . https://n2t.net/ark:/38305/f19c6wg4 Conditions Governing Access Collection is open for research. Conditions Governing Use Property rights for this collection reside with the University of California. Literary rights, including copyright, are retained by the creators and their heirs. The publication or use of any work protected by copyright beyond that allowed by fair use for research or educational purposes requires written permission from the copyright owner. Responsibility for obtaining permissions, and for any use rests exclusively with the user. Preferred Citation Lick Observatory Records: Photographs. UA36 Ser.7. Special Collections and Archives, University Library, University of California, Santa Cruz. Alternative Format Available Images from this collection are available through UCSC Library Digital Collections. Historical note These photographs were produced or collected by Lick observatory staff and faculty, as well as UCSC Library personnel. Many of the early photographs of the major instruments and Observatory buildings were taken by Henry E. Matthews, who served as secretary to the Lick Trust during the planning and construction of the Observatory. -
LOWELL OBSERVATORY in Flagstaff Embodies the Legacy of Arizona's VISIONARY ASTRONOMER
dby eSALLY BsENFORtD /iphontographsaby DAVItD Hi. SMoITH n PERCIVAL LOWELL NEVER CONSIDERED 1966, Lowell Observatory was registered as a LOWELL himself a dreamer. A stargazer, perhaps, but National Historic Landmark. Today, professional OBSERVATORY never a dreamer. and amateur stargazers go to the observatory, In the summer of 1894, Lowell thought he one of the world’s largest, privately operated, in Flagstaff had proof that intelligent life existed on Mars. nonprofit astronomical research observatories. The Harvard-educated mathematician, who Lowell’s 24-inch Clark refractor telescope, Embodies hailed from Boston blue-blooded society, spent which he used for his Mars observations, now the Legacy of night after night perched on a lonely serves as an instrument for public viewing. ponderosa pine-studded mesa above Flagstaff, Even in the 21st century, Lowell seems to Arizona’s gazing through a telescope at Mars, taking oversee the operation as he peers from a large notes and making calculations. By the end of painting that hangs in the observatory’s Steele VISIONARY summer, Lowell decided he had enough Visitor Center lobby. Hand on hip and staring ASTRONOMER information to publish his findings. straight into the future, Lowell stands amid Lowell never proved his theory of life on modern-day and historical space observational Mars, but such theories sparked a firestorm devices. The center serves as the entry point of controversy about Martians, adding a for all observatory programs, telescopes and fascination with space to the developing literary exhibits. People come to learn the observatory’s genre of science fiction. Author H.G. Wells history and for a chance to look through published his novel War of the Worlds in 1898 Lowell’s telescopes. -
January 2010 Malama
SIERRA CLUB Cherish the Earth JOURNAL OF THE SIERRA CLUB, HAWAI`I CHAPTER A Quarterly Newsletter January - March 2010 Planting Native! Bold Policy Proposals Hey Mr. Green! Nate’s Adventures! National Ocean Policy Task Force Guest Entering the new year, Looking for ways to columnist what bold and realistic save the environment? Long-time Sierra Club Rick policy proposals can we Check out our advice volunteer Dave Raney Barbosa promote in order to column on short, easy describes the mission of SAVE A TREE! writes ensure a greener tips that you can use to the National Ocean about the Hawai`i? Learn about help save the Policy Task and some Receive your Malama the issues the Sierra Club environment. This Join Nate Yuen as he of the current electronically by going distribution, care, and is advocating month suggests how to describes a recent hike recommendations to cultural use of the native be green and save some along Wailuku River. being proposed. www.hi.sierraclub.org Ho`awa. Page 5 green! Click the link below Pages 8 - 9 Pages 10 - 11 “Email My Newsletter” Page 3 Page 6 private homes. Sandy areas -- where children build sand castles and Preserving sunbathers get “tan” -- are increasingly scarce and usually quite crowded. Sandy Hawai`i coastlines are dynamic. Beaches erode or accrete depending upon their location on the coast, their Beaches proximity to various things such as piers, sandwalls, the impact of storms, etc. Anyone who buys beachfront A Proposal to Protect Hawai’i’s property is made aware of the fact that Beaches for Our Keiki boundaries between private property and the public easement may shift over by Robert D. -
Arizona-Based Astronomers Characterize One of the Smallest Known Asteroids
PRESS RELEASE FOR IMMEDIATE RELEASE: 30 November 2016 ***Contact details appear below*** Arizona-based Astronomers Characterize One of the Smallest Known Asteroids A team of astronomers have obtained observations of the smallest asteroid –with a diameter of only two meters (six feet)—ever characterized in detail. The asteroid, named 2015 TC25, is also one of the brightest near-Earth asteroids ever discovered, reflecting 60 percent of the sunlight that falls on it. Discovered by the University of Arizona’s Catalina Sky Survey last October, 2015 TC25 was studied extensively by a team led by Vishnu Reddy, an assistant professor at the University of Arizona's Lunar and Planetary Laboratory. Other participating institutions include Lowell Observatory and Northern Arizona University. The team used four Earth-based telescopes for the study, published this month in The Astronomical Journal. Reddy argues that new observations from the NASA Infrared Telescope Facility and Arecibo Planetary Radar show that 2015 TC25's surface is similar to a rare type of highly reflective meteorite called aubrites. Aubrites consist of very bright minerals, mostly silicates, that formed in an oxygen-free, basaltic environment at very high temperatures. Only one out of every 1,000 meteorites that fall to Earth belong to this class. "This is the first time we have optical, infrared, and radar data on such a small asteroid, which is essentially a meteoroid," said Reddy. "You can think of it as a meteorite floating in space that hasn't hit the atmosphere and made it to the ground—yet." “2015 TC25 is one of the five smallest Near-Earth Objects ever observed to measure rotation rate” says Audrey Thirouin from Lowell Observatory.