Unseen Planet May Lurk Near Solar System's Edge
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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. -
Sirius Astronomer
September 2015 Free to members, subscriptions $12 for 12 issues Volume 42, Number 9 Jeff Horne created this image of the crater Copernicus on September 13, 2005 from his observing site in Irvine. September 19 is International Observe The Moon Night, so get out there and have a look at a source of light pollution we really don’t mind! OCA MEETING STAR PARTIES COMING UP The free and open club meeng will The Black Star Canyon site will open on The next session of the Beginners be held September 18 at 7:30 PM in September 5. The Anza site will be open on Class will be held at the Heritage Mu‐ the Irvine Lecture Hall of the Hashing‐ September 12. Members are encouraged to seum of Orange County at 3101 West er Science Center at Chapman Univer‐ check the website calendar for the latest Harvard Street in Santa Ana on Sep‐ sity in Orange. This month, JPL’s Dr. updates on star pares and other events. tember 4. The following class will be Dave Doody will discuss the Grand held October 2. Finale of the historic Cassini mission to Please check the website calendar for the Saturn in 2017! outreach events this month! Volunteers are GOTO SIG: TBA always welcome! Astro‐Imagers SIG: Sept. 8, Oct. 13 NEXT MEETINGS: October 9, Novem‐ Remote Telescopes: TBA You are also reminded to check the web ber 13 Astrophysics SIG: Sept. 11, Oct. 16 site frequently for updates to the calendar Dark Sky Group: TBA of events and other club news. -
Chaos in the Inert Oort Cloud
EPSC Abstracts Vol. 13, EPSC-DPS2019-1303-1, 2019 EPSC-DPS Joint Meeting 2019 c Author(s) 2019. CC Attribution 4.0 license. Chaos in the inert Oort cloud Melaine Saillenfest (1), Marc Fouchard (1), and Arika Higuchi (2) (1) IMCCE, Observatoire de Paris, France, (2) RISE Project Office/NAOJ, Mitaka, Tokyo, Japan e-mail: [email protected] µ 16 Abstract 2 εP − εG ÝÖ 14 2 We investigate the orbital dynamics of small bodies in aÙ 9 12 the intermediate regime between the Kuiper belt and − 10 the Oort cloud, i.e. where the planetary perturbations ´ 10 and the galactic tides have the same order of magni- 8 tude. We show that this region is far less inert than it could appear at first sight, despite very weak orbital 6 perturbations. Ô eÖØÙÖbaØiÓÒ 4 Øhe Óf 2 1. Introduction ×iÞe 0 0 500 1000 1500 2000 2500 3000 aÜi× ´aÙµ The orbits of distant trans-Neptunian objects are sub- ×eÑi¹Ña jÓÖ a ject to internal perturbations from the planets, and ex- ternal perturbations from the galactic tides. A distinc- Figure 1: Size of the small parameters appearing in tion is generally made between the Kuiper belt and the the Hamiltonian function (Eq. 1) with respect to the Oort cloud, which are thought to have been initially semi-major axis of the small body. The red curve rep- populated through distinct mechanisms (see e.g. the resents the planetary perturbations, and the blue curve recent review by [4]). However, there is no dynamical represents the galactic tides. boundary between the two populations, and numerical simulations show a continuous transfer of objects in 2. -
NOAO Hosts “Colors of Nature” Summer Academy
On the Cover The cover shows an 8 × 9 arcminutes image of a portion of the Milky Way galactic bulge, obtained as part of the Blanco DECam Bulge Survey (BDBS) using the Dark Energy Camera (DECam) on the CTIO Blanco 4-m telescope. In this image, red, green, and blue (RGB) pixels correspond to DECam’s Y, z and i filters, respectively. The inset image shows the 2 × 3 array of monitors at the “observer2” workstation in the Blanco control room. The six chips shown here represent only 10% of the camera’s field of view. For more information about the BDBS and their experiences observing with DECam, see the “The Blanco DECam Bulge Survey (BDBS)” article in the Science Highlights section of this Newsletter. (Image credit: Will Clarkson, University of Michigan-Dearborn; Kathy Vivas, NOAO; R. Michael Rich, UCLA; and the BDBS team.) NOAO Newsletter NATIONAL OPTICAL ASTRONOMY OBSERVATORY ISSUE 110 — SEPTEMBER 2014 Director’s Corner Under Construction: A Revised KPNO Program Emerges ................ 2 CTIO Instruments Available for 2015A ......................................... 18 Gemini Instruments Available for 2015A ..................................... 19 Science Highlights KPNO Instruments Available for 2015A........................................ 20 The Survey of the MAgellanic Stellar History (SMASH) ................... 3 AAT Instruments Available for 2015A .......................................... 21 Two’s Company in the Inner Oort Cloud ......................................... 5 CHARA Instruments Available for 2015 ....................................... -
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. -
Arxiv:1706.07447V1 [Astro-Ph.EP] 22 Jun 2017 Periods
Origin and Evolution of Short-Period Comets David Nesvorn´y1, David Vokrouhlick´y2, Luke Dones1, Harold F. Levison1, Nathan Kaib3, Alessandro Morbidelli4 (1) Department of Space Studies, Southwest Research Institute, 1050 Walnut St., Suite 300, Boulder, CO 80302, USA (2) Institute of Astronomy, Charles University, V Holeˇsoviˇck´ach2, CZ{18000 Prague 8, Czech Republic (3) HL Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA (4) D´epartement Cassiop´ee,University of Nice, CNRS, Observatoire de la C^oted'Azur, Nice, 06304, France ABSTRACT Comets are icy objects that orbitally evolve from the trans-Neptunian region into the inner Solar System, where they are heated by solar radiation and be- come active due to sublimation of water ice. Here we perform simulations in which cometary reservoirs are formed in the early Solar System and evolved over 4.5 Gyr. The gravitational effects of Planet 9 (P9) are included in some sim- ulations. Different models are considered for comets to be active, including a simple assumption that comets remain active for Np(q) perihelion passages with perihelion distance q < 2:5 au. The orbital distribution and number of active comets produced in our model is compared to observations. The orbital distri- bution of ecliptic comets (ECs) is well reproduced in models with Np(2:5) ' 500 and without P9. With P9, the inclination distribution of model ECs is wider than the observed one. We find that the known Halley-type comets (HTCs) have a nearly isotropic inclination distribution. The HTCs appear to be an exten- sion of the population of returning Oort-cloud comets (OCCs) to shorter orbital arXiv:1706.07447v1 [astro-ph.EP] 22 Jun 2017 periods. -
Planet Nine Join the Hunt for a Possible Planet!
Planet Nine Join the Hunt for a Possible Planet! In July 2015, the New Horizons spacecraft gave us our first close look at Pluto, the most famous dwarf planet in the outskirts of our Solar System. The flyby was big news, and the data sent back to Earth revealed a world far more complex than anyone realized. Are there more worlds out there, beyond Pluto? What might such a world be like? Planet Nine tells a tale of the search for another world hidden in the darkness. Planetary scientist-explorers continually make discoveries about conditions "out there". Planet Nine follows Mike Brown and his team at CalTech as they uncover new worlds such as the remarkably bright Eris; tumbling Haumea, an Exploring Farther egg-shaped object rotating incredibly fast; and Sedna, whose High-powered telescopes peer out at the sky each night, orbit takes it deep into the far reaches of the Solar System. searching for faint light from distant worlds. Experience a night at the Subaru Telescope in Hawaii, as Brown describes his Is there a new planet beyond even these distant objects? search for worlds so far away they take thousands of years to orbit the Sun. Orbits Tell The Tale Pluto's own unusual path is a clue to chaotic activities billions of years ago. Could other distant objects "out there" follow equally odd orbits? Throughout this fascinating show, Mike Brown talks about unusual orbits and describes nights of painstaking robotic searches for new planets. His is a story of modern planet- hunting techniques that have uncovered many new worlds out beyond Neptune. -
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. -
Percival Lowell Society: Joe Sims Wanted to Be an Astronomer, Maybe Even Belt Asteroids, and Neos
THE LOWELL EXPANDING OUR UNIVERSE OBSERVER The quarterly newsletter of Lowell Observatory Issue 98 Fall 2013 (Right) Nick Moskovitz poses in front Nick Moskovitz of the SOAR 4-m telescope on Cerro Pachon in Chile, where he was Coming to Lowell observing near-Earth asteroids. The by Tom Vitron figure below illustrates the sheer size of various NEOs. The meteor from the Chelyabinsk event was only slightly smaller than the DCT dome, On February 15th, Earth and more than three times as large witnessed two close-up Near-Earth Object as “Big Red”, Percival Lowell’s 1911 (NEO) events, a predicted nearby pass and Model Y Stevens-Duryea touring the Chelyabinsk, Siberia event. Questions car. The Barringer Meteor created Meteor Crater in Arizona, whereas arose immediately: were the two events the Tunguska Comet explosion was related? What kind of meteor was seen the largest impact event on or near brilliantly exploding in the numerous car Earth in recorded history, occurring dashboard videos from Siberia? When the in 1908 near the Podkamennaya world went looking for answers, one of the Tunguska River in Siberia. leading experts quoted was astronomer Nick Moskovitz of MIT, who will be joining Lowell in 2014. “I was at Kitt Peak [National Observatory near Tucson] to see the flyby as we had one chance to try to see it well,” recounts Dr. Moskovitz. “We had some interviews that night about the flyby and [the interviewers] started asking about Chelyabinsk. I hadn’t heard much yet. We were able to see news about the event more 100m 56.3m 50m 18.9m 17m 12.8m 4.9m closely in the night. -
Lowellobserver
THE ISSUE 105 FALL 2015 LOWELL OBSERVER THE QUARTERLY NEWSLETTER OF LOWELL OBSERVATORY HOME OF PLUTO Just 15 minutes after its closest approach to Pluto on July 14, 2015, NASA’s New Horizons spacecraft looked back toward the Sun and captured a near- sunset view of the rugged, icy mountains and flat ice plains extending to Pluto’s horizon. (NASA/JHUAPL/SwRI) IN THIS SPECIAL EXTENDED ISSUE 2 Director’s Update 2 Trustee’s Update 3 Bound for Chile! New Horizons Unveils Pluto’s Secrets By Will Grundy Astronomers can normally study memes. Importantly, the focus remained distant objects only through their light, so almost entirely on the science, not hare- a unique appeal of solar system science is brained conspiracy theories or umbrage the possibility to send spacecraft to study at off-the-cuff remarks of team members. bodies in ways that could only be done Pluto, the real star of the show, up-close. Such spacecraft exploration isn’t certainly rose to the occasion, revealing 4 Education On Board SOFIA cheap, and competition is fierce over which incredible complexities and stark beauty. missions should be flown. The opportunity But much about the encounter was 5 Pluto Occultation Team to participate in one is a rare and cherished attributable to the hard-working team 6 Lowell Hosts Pluto Palooza opportunity for a planetary scientist like who delivered Pluto to the world. How myself. That’s especially so for a first-ever was this done, and what was it like being encounter with a previously unexplored involved? The key was practice. -
"Planet Nine": Have Astronomers Found a Huge New World Past Pluto? by Scientific American, Adapted by Newsela Staff 01.25.16
Name: ______________________________ Period: ______ Date: _____________ Article of the Week Directions: Read the following article carefully and annotate. You need to include at least 1 annotation per paragraph. Be sure to include all of the following in your total annotations. Annotation = Marking the Text + A Note of Explanation 1. Great Idea or Point – Write why you think it is a good idea or point – ! 2. Confusing Point or Idea – Write a question to ask that might help you understand – ? 3. Unknown Word or Phrase – Circle the unknown word or phrase, then write what you think it might mean based on context clues or your word knowledge – 4. A Question You Have – Write a question you have about something in the text – ?? 5. Summary – In a few sentences, write a summary of the paragraph, section, or passage – # "Planet Nine": Have astronomers found a huge new world past Pluto? By Scientific American, adapted by Newsela staff 01.25.16 Picture and Caption ___________________________ ___________________________ ___________________________ ___________________________ Paragraph #1 This picture is an artist’s depiction of what "Planet Nine" might look like. The planet is thought to be gaseous, similar to Uranus and Neptune, and in our solar system out ___________________________ beyond Pluto. Photo: Caltech/R. Hurt (IPAC) ___________________________ Para #1 In the last 20 years, astronomers have identified about 2,000 new worlds using a telescope in space. These planets ___________________________ orbit stars that lie tens or even hundreds of light-years from Earth. These discoveries are important, but no single planet is likely to ___________________________ be much of a big deal. -
Arxiv:1301.7656V1 [Physics.Hist-Ph]
Origins of the Expanding Universe: 1912-1932 ASP Conference Series, Vol. 471 Michael J. Way and Deidre Hunter, eds. c 2013 Astronomical Society of the Pacific What Else Did V. M. Slipher Do? Joseph S. Tenn Department of Physics & Astronomy, Sonoma State University, Rohnert Park, CA, 94928, USA Abstract. When V. M. Slipher gave the 1933 George Darwin lecture to the Royal Astronomical Society, it was natural that he spoke on spectrographic studies of planets. Less than one–sixth of his published work deals with globular clusters and the objects we now call galaxies. In his most productive years, when he had Percival Lowell to give him direction, Slipher made major discoveries regarding stars, galactic nebulae, and solar system objects. These included the first spectroscopic measurement of the rotation period of Uranus, evidence that Venus’s rotation is very slow, the existence of reflection nebulae and hence interstellar dust, and the stationary lines that prove the existence of interstellar calcium and sodium. After Lowell’s death in 1916 Slipher con- tinued making spectroscopic observations of planets, comets, and the aurora and night sky. He directed the Lowell Observatoryfrom 1916 to 1954, where his greatest achieve- ments were keeping the observatory running despite very limited staff and budget, and initiating and supervising the “successful” search for Lowell’s Planet X. However, he did little science in his last decades, spending most of his time and energy on business endeavors. 1. Introduction Vesto Melvin Slipher, always referred to and addressed as “V. M.” (Giclas 2007; Hoyt 1980b) came to Flagstaff in August 1901, two months after completing his B.A.