Total Solar Eclipse When's the Next One?

Total Page:16

File Type:pdf, Size:1020Kb

Total Solar Eclipse When's the Next One? 25 Amazing Moon Features! STARGAZING GETTING STARTED WITH ASTRONOMY Total Solar Eclipse When's the Next One? P. 7 I Join the Club P. 11 I Up All Night Future Eclipses When’s the Next One? Don’t be surprised if seeing the totally eclipsed Sun is habit-forming. By J. Kelly Beatty but also because you’ll be able to experi- Pacific and Atlantic) and by the impos- ence the glorious stars of the deep- ing ridge of Andean peaks. Some of the very total solar eclipse is different. southern sky (think Southern Cross and very best viewing prospects, statistically E Some are frustratingly short, oth- Alpha Centauri). Moreover, the Andes of speaking, occur in Chile’s picturesque ers luxuriously long. The Sun’s ethereal central Chile boast some of the world’s Elqui Valley, which is a little inland from corona can vary from nearly formless greatest professional observatories. A La Serena, and on the other side of the to astoundingly structured. And the few even lie in the path of totality. Andes in western Argentina. Moon’s umbral shadow, which touches From a climatic viewpoint, it’ll be Having visited La Serena and the Earth about every 18 months on average, the middle of winter in the Southern Elqui Valley in March, I can vouch for can drape itself anywhere on the globe. Hemisphere. But the track crosses South the fact that “eclipse buzz” is already Regardless of the specifics, however, America at subtropical latitudes near 30° building in this area. these celestial spectacles are always south, and the average daytime high in amazing. In fact, a common refrain after La Serena (offering 2m 13s of totality) is DECEMBER 14, 2020: someone’s first full immersion in total- about 60°F. According to eclipse-weather Chile & Argentina Again! ity is, “When’s the next one?!” And so, expert Jay Anderson, this positioning By remarkable coincidence, the Moon’s should you likewise be looking ahead, “takes the sting out of what might other- umbral shadow makes its next return here’s a recap of the circumstances for a wise be a very cloudy environment.” Day- about 17 months later — and again few upcoming total solar eclipses. to-day weather is dominated by ocean- crosses Chile and Argentina in the driven cloudiness offshore (in both the middle of a path that spans the southern JULY 2, 2019: Chile & Argentina There’s no “TSE” in 2018. Instead, nearly two years will pass until your next oppor- North America 19 tunity (after August 21st) to stand in 0 2 the Moon’s shadow. On paper, the solar , North Pacific 2 m s Ocean eclipse of July 2, 2019, offers up to 4 33 ly u of totality, nearly double the maximum J that eclipse goers will witness this year. However, to experience all that you’ll need to be bobbing in a remote stretch of the South Pacific Ocean some 700 South America miles north of Easter Island. And while at least one company is planning to place Path of Totality a ship in totality’s path near the Pitcairn Islands, most veteran eclipse chasers are eyeing locations in the path’s only land- fall: central Chile and Argentina. These are exciting countries to visit, not only because of their welcoming South Pacific populations and amazing natural beauty, Ocean A yellow band marks the path of totality during the next total solar eclipse after the one on August 21st. The path crosses land only in Chile and Argentina. A black dot marks where the duration will be longest. Sets of curved lines Antarctica show the extent of the partial eclipse (in 20% increments). MICHAEL ZEILER / GREATAMERICANECLIPSE.COM / ZEILER MICHAEL 1 America’s 2017 Eclipse Future Eclipses Pacific and Atlantic oceans. However, this year the timing comes in the midst of the Southern Hemisphere’s summer 4 2 — high season for tourism! This means 0 2 chances are good that cruise ships will , 8 il be positioned off the South American r p coast specifically to catch the Moon’s A shadow as it sweeps by. The duration of totality is relatively North America short, a maximum of 2m 10s — but at North Atlantic least this time the point of “greatest Ocean eclipse” occurs on dry land, squarely in North Pacific Ocean the Patagonia region of Argentina. It’s still a bit far off for detailed eclipse-day y weather statistics, but summer months it al ot tend to be much less rainy than winter f T h o months, so on that basis alone there’s Pat cause for optimism. If this eclipse appeals to you, keep an South America eye out for travel packages that provide eclipse-day viewing as part of broader summertime tourism opportunities — such as visits to Chilean wineries or to South Pacific Ocean the Incan citadel of Machu Picchu in neighboring Peru. DECEMBER 4, 2021: Antarctica After going 38 years without being touched by the Moon’s shadow, the mainland U.S. is Truly dedicated eclipse chasers will have getting two total solar eclipses in a 7-year period. The second of these, in 2024, has a path that sweeps up through Mexico before crossing a belt of states from Texas to Maine. the opportunity to demonstrate their mettle one year later, when the Moon’s shadow sweeps over Antarctica and APRIL 8, 2024: What has many early planners excited provides a maximum of 1m 54s of total- United States & Mexico is the possibility of seeing the total solar ity. Xavier Jubier, who almost assuredly If distant travel or being really, really eclipses in both 2017 and 2024 from the will be watching that day, suggests three cold isn’t your thing, take heart. After same location. That’s possible inside a ways — none of them inexpensive — for avoiding the mainland U.S. for 38 years 135-by-85-mile parallelogram of real estate getting into the eclipse track. (1979 to 2017), the Moon’s umbra will just to the southeast of St. Louis. This First, you could hop aboard an make a return pass less than 7 years area includes Carbondale, Illinois, near Ilyushin 76 cargo aircraft that will fly after the total eclipse on August 21st. which is the point of maximum duration from Punta Arenas at the southern tip It’ll be a good one too, with a path for August’s eclipse. So a well-placed of Chile to Union Glacier in Antarctica. that sweeps northeastward from the skywatcher could witness 2m 42s of total- Once there you can stay and observe Pacific and across central Mexico, where ity in 2017 and another 4m 8s in 2024. from the relative comfort of a privately onlookers near Durango are banking on Some of the most dedicated “umbra- owned camp. A second option is to book seeing 4m 28s of totality. The path then philes” have traveled the world to witness a seat on a chartered eclipse flight that climbs through central Texas (Austin dozens of eclipses over their lifetimes. will position you in the Moon’s shadow and Dallas–Fort Worth are in for a treat Will you do likewise? Will totality on high above the Antarctic ice cap (I did that day), and several Midwest states August 21st become the first entry in this in 2003 — it’s a breathtaking way (Indianapolis and Cleveland are like- your personal “life list” of treasured to experience totality). Finally, some wise in the path). Then the track follows moments in the Moon’s shadow? ships are likely to venture into the South the arc of Lake Erie and Lake Ontario, Atlantic from various ports and inter- engulfing Buffalo before moving into J. Kelly Beatty, a senior editor at Sky & cept the shadow shortly after dawn from upstate New York, southern Québec, Telescope, has traveled to 17 total and an- positions off the tip of the Antarctic central Maine (where, with luck, “black- nular eclipses beginning in 1991. On August Peninsula, roughly halfway between the fly season” won’t have started yet), and 21st he’ll be leading a tour of 200+ hopeful Falkland and South Sandwich Islands. Canada’s Maritime provinces. eclipse watchers in Hopkinsville, Kentucky. GREATAMERICANECLIPSE.COM / ZEILER MICHAEL 2 America’s 2017 Eclipse LUNAR SHOWCASE M A R E F R I G O M R I S 8 Endymion Aristoteles Endymion SINUS Platolato 24 Reiner Gamma RORIS 17 Atlastlas 4 Serpentine Ridge ALPS MTSAlpineAlpine SINUS alley Eudoxus Picoico Vvalley Hercules IRIDUMIRIDUM 9 2 Proclus MARE Piton MTS Aristillus MTS IMBRIUM CAUCASUS CAUCASUS Posidonius 21 Archimedes 3 Autolycus MARE Schröter’s Timocharis 10 MARE Cleomedes Valley Cleomedes 22 SERENITATIS Aristarchus 11 1 APENNINE MTSMTS MARE Pliniuslinius CRISIUM OCEANUS Manilius Eratosthenes 18 Kepler Reiner Copernicus MARE Agrippa Reinhold TRANQUILLITATIS PROCELLARUM PROCELLARUM Lansberg MARE Delambre FECUNDITATIS Grimaldi Hipparchusipparchus 25 12 Ptolemaeustolemaeus Langrenus Theophilus 5 Albategniuslbategnius Cyrillus MARE Alphonsuslphonsus MARE Gassendi 23 NUBIUM Catharina NECTARIS StraightStraight WallWall 13 Arzachel Bullialdus Thebit 6 MAREMARE Fracastorius Petavius HUMORUM 14 Purbach Werner Piccolominiiccolomini Walter Fra Mauro Hainzel Altai Scarp 19 Tycho 7 15 Maurolycus Schickard Maginus JannsenJannsen 20 Schiller Pitiscusitiscus Claviuslavius Longomontanus 16 FEATURES APLENTY This composite of Lunar Reconnais- sance Orbiter images reveals the Moon's varied surface features. NASA GODDARD / ARIZONA STATE UNIVERSITY 25 Amazing Moon Features TAKE A TELESCOPIC TOUR OF 4 BILLION YEARS OF SOLAR-SYSTEM HISTORY. By J. KELLY BEATTY Every month we watch the Moon morph And what an interesting face it has! Over time we’ve come through its sequence of phases — from new to full and back to appreciate that the lunar surface preserves geologic events to new.
Recommended publications
  • Glossary Glossary
    Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts.
    [Show full text]
  • Grand Dames of Los Feliz Listed for $4.2 & $4.7 Million Our Relatively
    Los Feliz Ledger Read by 100,000+ Residents and Business Owners in Los Feliz, Silver Lake, Vol 12. No. 11 May 2017 Atwater Village, Echo Park & Hollywood Hills Our Relatively Western/ Safe Streets Franklin Project By Michael Aushenker Delayed, Contributing Writer Appeals Filed The city’s co-called “Vi- By Erin Hickey sion Zero” plan, which aims Ledger Contributing Writer to reduce traffic deaths and injuries to zero by 2025, has An April 27th Los Ange- its work cut out for it in some les City Planning Dept. hear- areas of the city, but not so ing for the controversial 5-sto- much locally. ry development proposed for According to city officials, the intersection of Franklin good portions of Los Feliz, and Western avenues has now East Hollywood, Silver Lake, been postponed until May Echo Park and Atwater Village 25th at the developer’s request, have had a statistically low ra- according to public records. tio of car related fatalities and The project, a mixed-use serious injuries compared to apartment complex, would in- other parts of Los Angeles. clude 96 residential units, and “We’re fortunate in roughly 5,550 square feet of Council District 4 to have had commercial space and would relatively few traffic-related -fa replace an existing gas sta- talities,” said Los Angeles City tion, duplex and single family Councilmember David Ryu, home. who represents those neigh- Thus far, public sentiment borhoods in part, along with on the development has been PROTEST—About 60 people gathered April 15 to protest in advance of the city’s April 18th closure Council District 13 Coun- split, with the project’s sup- of a gate at the end of Beachwood Canyon Drive—per a court order—which had become a favorite cilmember Mitch O’Farrell.
    [Show full text]
  • Three Chumash-Style Pictograph Sites in Fernandeño Territory
    THREE CHUMASH-STYLE PICTOGRAPH SITES IN FERNANDEÑO TERRITORY ALBERT KNIGHT SANTA BARBARA MUSEUM OF NATURAL HISTORY There are three significant archaeology sites in the eastern Simi Hills that have an elaborate polychrome pictograph component. Numerous additional small loci of rock art and major midden deposits that are rich in artifacts also characterize these three sites. One of these sites, the “Burro Flats” site, has the most colorful, elaborate, and well-preserved pictographs in the region south of the Santa Clara River and west of the Los Angeles Basin and the San Fernando Valley. Almost all other painted rock art in this region consists of red-only paintings. During the pre-contact era, the eastern Simi Hills/west San Fernando Valley area was inhabited by a mix of Eastern Coastal Chumash and Fernandeño. The style of the paintings at the three sites (CA-VEN-1072, VEN-149, and LAN-357) is clearly the same as that found in Chumash territory. If the quantity and the quality of rock art are good indicators, then it is probable that these three sites were some of the most important ceremonial sites for the region. An examination of these sites has the potential to help us better understand this area of cultural interaction. This article discusses the polychrome rock art at the Burro Flats site (VEN-1072), the Lake Manor site (VEN-148/149), and the Chatsworth site (LAN-357). All three of these sites are located in rock shelters in the eastern Simi Hills. The Simi Hills are mostly located in southeast Ventura County, although the eastern end is in Los Angeles County (Figure 1).
    [Show full text]
  • General Disclaimer One Or More of the Following Statements May Affect
    https://ntrs.nasa.gov/search.jsp?R=19710025504 2020-03-11T22:36:49+00:00Z View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by NASA Technical Reports Server General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) 6 X t B ICC"m date: July 16, 1971 955 L'Enfant Plaza North, S. W Washington, D. C. 20024 to Distribution B71 07023 from. J. W. Head suhiecf Derivation of Topographic Feature Names in the Apollo 15 Landing Region - Case 340 ABSTRACT The topographic features in the region of the Apollo 15 landing site (Figure 1) are named for a number of philosophers, explorers and scientists (astronomers in particular) representing periods throughout recorded history. It is of particular interest that several of the individuals were responsible for specific discoveries, observations, or inventions which considerably advanced the study and under- standing of the moon (for instance, Hadley designed the first large reflecting telescope; Beer published classic maps and explanations of the moon's surface).
    [Show full text]
  • JPL to Map the Moon on India Mission
    I n s i d e May 19, 2006 Volume 36 Number 10 News Briefs ............... 2 Griffin Visits Lab ............ 3 Special Events Calendar ...... 2 Passings, Letters ........... 4 Spitzer Sees Comet Breakup... 2 Retirees, Classifieds ......... 4 Jet Propulsion Laborator y A JPL state-of-the-art imaging spectrometer that will provide the first high-resolution spectral map of the JPL to entire lunar surface successfully completed its critical design review this week. The Moon Mineralogy Mapper, also known as “M3,” is one of two in- materials across the surface at high spatial resolution. This data map the struments that NASA is contributing to India’s first mission to the moon, will provide a much-needed long-term baseline for future exploration scheduled to launch in late 2007 or early 2008. By mapping the mineral activities. composition of the lunar surface, the mission will both provide clues to The mission’s observations will address several important scientific moon the early development of the solar system and guide future astronauts to issues, including early evolution of the solar system; fundamental stores of precious resources. processes acting on planets that shape their character; assessment of on India Chandrayaan-1 is India’s first deep-space mission as well as its first potential impact hazards to Earth; and assessment of space resources. lunar mission. “The entire M3 team feels honored to be able to partici- From its vantage point in orbit around the moon, the spacecraft will mission pate,” said Project Manager Tom Glavich of JPL. measure the sunlight reflected by all of the rocks and soil over which The instrument is well on its way to being delivered to the Chandray- it passes.
    [Show full text]
  • Vol. 73, No. 1 December 2020
    Published by the Astronomical League Vol. 73, No. 1 December 2020 PUBLIC OUTREACH DURING A PANDEMIC THE ULTIMATE OBSERVING CHALLENGE th 75 GEAR UP FOR SOLAR CYCLE 25 THE ASTRONOMICAL LEAGUE’S 75TH ANNIVERSARY AN EMPLOYEE-OWNED COMPANY NEW FREE SHIPPING on order of $75 or more & INSTALLMENT BILLING on orders over $350 PRODUCTS Standard Shipping. Some exclusions apply. Exclusions apply. Orion® StarShoot™ Compact Astro Orion® StarShoot™ Mini 6.3mp Tracker Imaging Cameras (sold separately) Orion® StarShoot™ G26 APS-C Orion® GiantView™ BT-100 ED #21192 $280 Color #51883 $400 Color Imaging Camera 90-degree Binocular Telescope (Mount not Mono #51884 $430 #51458 $1,800 #51878 $2,600 included) computer not Trust 2019 included Proven reputation for Orion® U-Mount innovation, dependability and and Paragon Plus service… for over 45 years! XHD Package #22115 $600 Superior Value Orion® StarShoot™ Deep Space High quality products at Orion® StarShoot™ G21 Deep Space Imaging Cameras (sold separately) Orion® HDX 12" Truss RC Ultimate affordable prices Color Imaging Camera G10 Color #51452 $1,200 Astro- Imaging Package #54290 $950 G16 Mono #51457 $1,300 #21101 $9,500 Wide Selection Extensive assortment of award winning Orion brand 2019 products and solutions Customer Support Orion products are also available through select Orion® MagneticDobsonian authorized dealers able to Counterweights offer professional advice and Orion® Premium Linear Orion® EON 130mm ED Triplet Orion® 2x54 Ultra Wide Angle 1-Pound #7006 $25 Binoculars post-purchase support BinoViewer
    [Show full text]
  • August 2017 Posidonius P & Luther
    A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: Wayne Bailey [email protected] 17 Autumn Lane, Sewell, NJ 08080 RECENT BACK ISSUES: http://moon.scopesandscapes.com/tlo_back.html FEATURE OF THE MONTH – AUGUST 2017 POSIDONIUS P & LUTHER Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA March 5, 2017 01:28-01:48; UT, 15 cm refl, 170x, seeing 7-8/10. I drew these craters on the evening of March 4/5, 2017 while the moon was hiding some Hyades stars. This area is in northeast Mare Serenitatis west of Posidonius itself. Posidonius P is the largest crater on this sketch. The smaller crater south of P is Posidonius F and Posidonius G is the tiny pit to the north. There is a halo around Posidonius G, but this crater is noticeably north of the halo's center. A very low round swelling is northeast of Posidonius G. Luther is the crater well to the west of Posidonius P. All four of these craters are crisp, symmetric features, differing only in size. There are an assortment of elevations near Luther. The peak Luther alpha is well to the west of Luther, and showed dark shadowing at this time. All of the other features near Luther are more subtle than Luther alpha. One mound is between Luther and Luther alpha. Two more mounds are north of Luther, and a low ridge is just east of this crater. A pair of very low mounds are south of Luther. These are the vaguest features depicted here, and may be too conspicuous on the sketch.
    [Show full text]
  • LA Zoo Vision Plan
    3.14 Recreation 3.14 RECREATION The Zoo is a unique attraction within Griffith Park and the greater Los Angeles area. The proposed Project is expected to increase visitation to the Zoo and surrounding area, creating the potential for additional use and physical deterioration of recreational facilities, including those within the Zoo and Griffith Park. Additionally, proposed expansion to the Zoo and associated recreational facilities could result in physical impacts to the surrounding environment. However, proposed expansion in visitor-serving areas and public parkland would accommodate the projected increase in use, reducing potential for adverse impacts. Therefore, impacts to recreational facilities from the Project would be less than significant. This section addresses recreational facilities that would be affected by the Los Angeles Zoo Vision Plan (Vision Plan) in the City of Los Angeles (City). The analysis describes the regulatory setting, the existing conditions at the Zoo and vicinity, and the potential impact of the implementation of the Vision Plan (Project) on recreational facilities. Impact analysis considers the potential for physical detriment or reduction in access to existing recreational facilities and whether development of new recreational facilities would significantly affect the environment. 3.14.1 Environmental Setting Regulatory Setting State and local laws and regulations have been enacted to ensure adequate provision of recreational facilities in the City. There are no federal regulations that apply to the Project. State Regulations Quimby Act (California Government Code Section 66477) The Quimby Act (California Government Code Section 66477) was established in 1965 by the California Legislature to set forth provisions in the State Subdivision Map Act for the dedication of parkland (e.g., dedication ratio of three acres per 1,000 population) and/or payment of in-lieu fees as a condition of approval of certain types of residential development projects.
    [Show full text]
  • July 2020 in This Issue Online Readers, ALPO Conference November 6-7, 2020 2 Lunar Calendar July 2020 3 Click on Images an Invitation to Join ALPO 3 for Hyperlinks
    A publication of the Lunar Section of ALPO Edited by David Teske: [email protected] 2162 Enon Road, Louisville, Mississippi, USA Recent back issues: http://moon.scopesandscapes.com/tlo_back.html July 2020 In This Issue Online readers, ALPO Conference November 6-7, 2020 2 Lunar Calendar July 2020 3 click on images An Invitation to Join ALPO 3 for hyperlinks. Observations Received 4 By the Numbers 7 Submission Through the ALPO Image Achieve 4 When Submitting Observations to the ALPO Lunar Section 9 Call For Observations Focus-On 9 Focus-On Announcement 10 2020 ALPO The Walter H. Haas Observer’s Award 11 Sirsalis T, R. Hays, Jr. 12 Long Crack, R. Hill 13 Musings on Theophilus, H. Eskildsen 14 Almost Full, R. Hill 16 Northern Moon, H. Eskildsen 17 Northwest Moon and Horrebow, H. Eskildsen 18 A Bit of Thebit, R. Hill 19 Euclides D in the Landscape of the Mare Cognitum (and Two Kipukas?), A. Anunziato 20 On the South Shore, R. Hill 22 Focus On: The Lunar 100, Features 11-20, J. Hubbell 23 Recent Topographic Studies 43 Lunar Geologic Change Detection Program T. Cook 120 Key to Images in this Issue 134 These are the modern Golden Days of lunar studies in a way, with so many new resources available to lu- nar observers. Recently, we have mentioned Robert Garfinkle’s opus Luna Cognita and the new lunar map by the USGS. This month brings us the updated, 7th edition of the Virtual Moon Atlas. These are all wonderful resources for your lunar studies.
    [Show full text]
  • Water on the Moon, III. Volatiles & Activity
    Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere).
    [Show full text]
  • GRAIL Reveals Secrets of the Lunar Interior
    GRAIL Reveals Secrets of the Lunar Interior — Dr. Patrick J. McGovern, Lunar and Planetary Institute A mini-flotilla of spacecraft sent to the Moon in the past few years by several nations has revealed much about the characteristics of the lunar surface via techniques such as imaging, spectroscopy, and laser ranging. While the achievements of these missions have been impressive, only GRAIL has seen deeply enough to reveal inner secrets that the Moon holds. LRecent Lunar Missions Country Name Launch Date Status ESA Small Missions for Advanced September 27, 2003 Ended with lunar surface impact on Research in Technology-1 (SMART-1) September 3, 2006 USA Acceleration, Reconnection, February 27, 2007 Extension of the THEMIS mission; ended Turbulence and Electrodynamics of in 2012 the Moon’s Interaction with the Sun (ARTEMIS) Japan SELENE (Kaguya) September 14, 2007 Ended with lunar surface impact on June 10, 2009 PChina Chang’e-1 October 24, 2007 Taken out of orbit on March 1, 2009 India Chandrayaan-1 October 22, 2008 Two-year mission; ended after 315 days due to malfunction and loss of contact USA Lunar Reconnaissance Orbiter (LRO) June 18, 2009 Completed one-year primary mission; now in five-year extended mission USA Lunar Crater Observation and June 18, 2009 Ended with lunar surface impact on Sensing Satellite (LCROSS) October 9, 2009 China Chang’e-2 October 1, 2010 Primary mission lasted for six months; extended mission completed flyby of asteroid 4179 Toutatis in December 2012 USA Gravity Recovery and Interior September 10, 2011 Ended with lunar surface impact on I Laboratory (GRAIL) December 17, 2012 To probe deeper, NASA launched the Gravity Recovery and Interior Laboratory (GRAIL) mission: twin spacecraft (named “Ebb” and “Flow” by elementary school students from Montana) flying in formation over the lunar surface, tracking each other to within a sensitivity of 50 nanometers per second, or one- twenty-thousandth of the velocity that a snail moves [1], according to GRAIL Principal Investigator Maria Zuber of the Massachusetts Institute of Technology.
    [Show full text]
  • Glossary of Lunar Terminology
    Glossary of Lunar Terminology albedo A measure of the reflectivity of the Moon's gabbro A coarse crystalline rock, often found in the visible surface. The Moon's albedo averages 0.07, which lunar highlands, containing plagioclase and pyroxene. means that its surface reflects, on average, 7% of the Anorthositic gabbros contain 65-78% calcium feldspar. light falling on it. gardening The process by which the Moon's surface is anorthosite A coarse-grained rock, largely composed of mixed with deeper layers, mainly as a result of meteor­ calcium feldspar, common on the Moon. itic bombardment. basalt A type of fine-grained volcanic rock containing ghost crater (ruined crater) The faint outline that remains the minerals pyroxene and plagioclase (calcium of a lunar crater that has been largely erased by some feldspar). Mare basalts are rich in iron and titanium, later action, usually lava flooding. while highland basalts are high in aluminum. glacis A gently sloping bank; an old term for the outer breccia A rock composed of a matrix oflarger, angular slope of a crater's walls. stony fragments and a finer, binding component. graben A sunken area between faults. caldera A type of volcanic crater formed primarily by a highlands The Moon's lighter-colored regions, which sinking of its floor rather than by the ejection of lava. are higher than their surroundings and thus not central peak A mountainous landform at or near the covered by dark lavas. Most highland features are the center of certain lunar craters, possibly formed by an rims or central peaks of impact sites.
    [Show full text]