Astronomical works with students Irina GUSEVA St Petersburg - Central (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences - St Petersburg.

Slides:



Advertisements
Similar presentations
Star catalogue comparison a tool to improve asteroidal prediction accuracy Dave Herald, TTSO4, April 2010, Canberra.
Advertisements

HOU in Russia Irina GUSEVA St Petersburg - Central (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences - St Petersburg State University,
THE TREASURES OF PULKOVO OBSERVATORY
General Astrophysics with TPF-C David Spergel Princeton.
Research Centre of Astronomy and Geophysics Mongolian Academy of Sciences Study of near-earth objects in Mongolia. Space debris, asteroids and comets Outreach.
Observing binaries with GAIA: large gains after much effort... Staffan Söderhjelm Lund Observatory.
Cosmic Ray Using for Monitoring and Forecasting Dangerous Solar Flare Events Lev I. Dorman (1, 2) 1. Israel Cosmic Ray & Space Weather Center and Emilio.
Announcements Test this week (all about stars) Turn in Homework 11 today Pick up Homework 12 Questions on last 3 assignments? Second project is due December.
Basic Principles of X-ray Source Detection Or Who Stole All Our Photons?.....
Binary stellar systems are interesting to study for many reasons. For example, most stars are members of binary systems, and so studies of binary systems.
X Ray Astronomy Presented by:- Mohit Shashwat Ankit.
Science Team Management Claire Max Sept 14, 2006 NGAO Team Meeting.
How to Get Equator Coordinates of Objects from Observation Zhenghong TANG Yale Astrometry Summer Workshop July, 2005.
25 YEARS AFTER THE DISCOVERY: SOME CURRENT TOPICS ON LENSED QSOs Santander (Spain), 15th-17th December 2004 Photometric monitoring of SBS : long-term.
TOPS 2003 Remote Obs 1 Karen Meech Institute for Astronomy TOPS 2003 Image copyright, R. Wainscoat, IfA Image courtesy K. Meech.
The Use of a High School Observatory to study the Metallicity Dependence of the Cepheid Period-Luminosity Relation J. Young, S. Scott, S. M. Kanbur (Physics.
30 March 2006Birmingham workshop1 The Gaia Mission A stereoscopic census of our Galaxy.
Distances. Parallax Near objects appear to move more than far objects against a distant horizon. Trigonometric parallax is used to measure distance to.
Introducing Astronomy Education into High School Physics Curriculum Through the Use of the University of North Dakota Observatory Caitlin Nolby Space Studies.
The Faulkes Telescopes: A Robotic Telescope Network for School Science Students Dr David Frew Department of Physics, Faculty of Science, Macquarie University.
Stars and Cells Kathy Cooksey Astronomy Overview.
Chapter 6: The Tools of the Astronomer. Telescopes come in two general types Refractors use lenses to bend the light to a focus Reflectors use mirrors.
Space Exploration- Tools
Starlab Curriculum at a Glance Baltimore County Public Schools Office of Science, PreK-12.
Amateur Astronomy The Bangalore Astronomical Society ®
Unit 11, Chapter 32 Integrated Science. Unit Eleven: Astronomy 32.1 Stars 32.2 Galaxies and the Universe Chapter 32 The Universe.
Astronomy and the Electromagnetic Spectrum
The B-V colors and photometric variability of Nix and Hydra, Pluto’s two small satellites Max Mutchler (STScI) S. Alan Stern (SwRI) Hal Weaver (JHU/APL)
The Chinese SONG proposal: scientific concerns Jianning Fu (Beijing Normal University) and Chinese SONG team Beijing ─ March 29, 2010 The third workshop.
The Close Binary Central Star of the Young Planetary Nebula HB12 C. H. Hsia a, W. H. Ip a, J.Y. Hu b a Institute of Astronomy, National Central University,
Studying for the Exam Relevant chapters: E, 1, 2 & 3 To prepare for the exam it is helpful to … –review readings –review lecture notes online (esp. concept.
Stellar variability monitoring in open clusters with mini-SONG X.B. Zhang National Astronomical Observatories, Chinese Academy of Sciences.
6/11/2012 Building on NEAT concept - M. Gai - INAF-OATo 1 Building on NEAT concept M. Gai – INAF-OATo (a) Extension of science case (b) Payload implementation.
investigated the nature of light, discovering that sunlight is made of light of different colors; the spectrum is, in order from long to short wavelength:
Galaxies Astronomy 115. First, which of the following is a galaxy? Open cluster Globular cluster Nebula Interstellar medium (gas and dust) Supernova remnant.
2004 January 27Mathematical Challenges of Using Point Spread Function Analysis Algorithms in Astronomical ImagingMighell 1 Mathematical Challenges of Using.
Aldo Dell'Oro INAF- Observatory of Turin Detailed analysis of the signal from asteroids by GAIA and their size estimation Besançon November 6-7, 2003.
What is Astrometry? Definition: To study the universe through positions and motions of celestial objects Acronym: Fund./Classical/Positional Astr. Related.
Observational Astrophysics I
Announcements HW #2 due on Friday Color version of Prob 8, clickable links to the Youtube videos available on Carmen Please turn off all electronic devices.
Introduction to Galaxies 5/23/2013. BR: Milky Way Scale The Milky Way has a diameter of approximately 8.25 x 10 9 AU (8.25 billion AU). 206,265 AU = 3.26.
Introduction4 Data acquisition and analysis8 Results17 Conclusion24 ASTEROID PHOTOMETRY GROUP, VSA
Astronomy Chapter Astronomy People in ancient cultures used the seasonal cycles to determine when they should plant and harvest crops. They built.
Celestial Objects Solar System Objects –Sun, Moon, Planets and Their Moons Galactic Objects –Star Formation Regions –Open Clusters –Globular Clusters –Planetary.
VST ATLAS: Requirements, Operations and Products Tom Shanks, Nigel Metcalfe, Jamie McMillan (Durham Univ.) +CASU.
© Sierra College Astronomy Department 1 Astronomy 10 Elementary Astronomy COURSE GOALS & OBJECTIVES.
Prepare your scantron: Please take a moment to mute your cell phone!
20/04/02 - F.A.DMS/PS organisation 1 Proposal for tasks and schedule -Coordination is needed -Tasks -Tools -Topics -Which areas are not covered -Manpower.
What is Astronomy? An overview..
Binary stellar systems are interesting to study for many reasons. For example, most stars are members of binary systems, and so studies of binary systems.
MMT Observation Database for Light Curve Analysis Vladimir Agapov Presentation for the WG1 session 33rd IADC meeting, Houston.
Astronomical Projects BEYOND NIGHT SKY. General requirements Weekly Night sky observation. Good knowledge of telescope controlling Imaging. Inviting few.
Spotting the life of stars „Pi of the Sky” Project Katarzyna Kwiecińska UKSW-SNŚ on behalf of the Pi of the Sky collaboration.
A black hole: The ultimate space-time warp Ch. 5.4 A black hole is an accumulation of mass so dense that nothing can escape its gravitational force, not.
Aim: Tools of Astronomy Do Now: List 4 tools that a chief may use DO NOW: What is this picture showing you? Notepack 21.
26th October 2005 HST Calibration Workshop 1 The New GSC-II and it’s Use for HST Brian McLean Archive Sciences Branch.
In conclusion the intensity level of the CCD is linear up to the saturation limit, but there is a spilling of charges well before the saturation if.
Before it was seen, it was heard. Brainstorming. Star Clusters Chang, Seo-Won.
Prepare your scantron:
University of Leicester Observatories
Gaia impact on asteroidal occultations
Gaia impact on asteroidal occultations
Unit 2 ASTRONOMY.
Photometric Analysis of Asteroids
Karen Meech Institute for Astronomy TOPS 2003
Integrated Science.
State Test Review Astronomy
Ch 12 Notes Early Astronomy
Presentation transcript:

Astronomical works with students Irina GUSEVA St Petersburg - Central (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences - St Petersburg State University, Faculty of Mathematics and Mechanics, Department of Astronomy

Instrument Double Short Focus Astrograph D = 100 mm F = 712 mm Objective prism UBVRI filters CCD ST-8 (SBIG) 1020 x 1530, 9 x 9 mkm Field Of View - 44' x 67 Scale - 2.6"/pixel

Works with students of St Petersburg State University (astronomers) Short time practice (summer) of CCD-observations: - Short lecture on CCDs - How to work with telescope (coordinates, sidereal time) - How to work with CCDOPS computer program - How to direct telescope to the necessary object on the sky - Taking images a) moving object (asteroid, comet, satellite…) - astrometry a) moving object (asteroid, comet, satellite…) - astrometry b) extensional object (galaxy, nebula,…) – photometry b) extensional object (galaxy, nebula,…) – photometry c) spectrum with objective prism (star, comet…) c) spectrum with objective prism (star, comet…) - Data processing (astrometric reduction, color images of galaxies, etc)

Works with students of St Petersburg State University (astronomers) One semester lectures and practice of astrometrists: - Course of lectures on CCD-astrometry - Practical work on CCD-astrometry a) observations (asteroids, comets, satellites…) a) observations (asteroids, comets, satellites…) b) images processing, astrometric and photometric reduction b) images processing, astrometric and photometric reduction c) programming (language on choice) of different investigations c) programming (language on choice) of different investigations concerning CCDs properties (for example, probability and energy concerning CCDs properties (for example, probability and energy distribution of cosmic rays events, different kind mathematician distribution of cosmic rays events, different kind mathematician filtering of frames, investigation of different sources of noise, etc) filtering of frames, investigation of different sources of noise, etc)

Sample (Pulkovo, Tracker) Results of the frame processing:

Works with students of St Petersburg State University (astronomers) Diploma works of students – astronomers Diploma works of students – astronomers (Russia, Moldavia, Ukraine, Argentina, Bolivia) (Russia, Moldavia, Ukraine, Argentina, Bolivia) Investigations of open clusters on the base of own Investigations of open clusters on the base of own CCD observations CCD observations - How to resolve very close (overlapping) star images on the CCD frame to obtain the most correct astrometry and photometry - Precise astrometric and photometric investigation (catalogues of clusters) - Determination of proper motions and investigation of open cluster kinematics

Comparison with Tycho-2 catalogue

Comparison with GSC catalogue

Works with students of St Petersburg State University (astronomers) Diploma works of students – astronomers Diploma works of students – astronomers (Russia, Moldavia, Ukraine, Argentina, Bolivia) (Russia, Moldavia, Ukraine, Argentina, Bolivia) Investigations of comets kinematics and non-gravitational effects Investigations of comets kinematics and non-gravitational effects on the base of own CCD observations on the base of own CCD observations Disturbances in the comet motion may be caused by different reasons: comet lose mass when approaching the Sun, comet is affected by solar wind and its variation because of the huge size of the comet halo, comet motion is affected by irregular ejection (evaporation and explosion) of the nucleus mass. This is very complicated but interesting problem that need extremely precise observations to detect small irregularities in the comet motion. precise observations to detect small irregularities in the comet motion. On the other side it is very difficult to determine the true coordinates of the comet nucleus because of bright halo of the comet. The problem is complicated by phase effect of illumination.

Works with students of St Petersburg State University (astronomers) Diploma works of students – astronomers Diploma works of students – astronomers (Russia, Moldavia, Ukraine, Argentina, Bolivia) (Russia, Moldavia, Ukraine, Argentina, Bolivia) Investigations of comets kinematics and non-gravitational effects Investigations of comets kinematics and non-gravitational effects on the base of own CCD observations on the base of own CCD observations - How to detect the true position of the comets nucleus, to obtain the most correct astrometry and photometry the most correct astrometry and photometry - Series of precise astrometric and photometric measurements, detection of deviations from the predicted (or mean) orbit. detection of deviations from the predicted (or mean) orbit. Looking for reasons of these deviations Looking for reasons of these deviations - Photometric investigation of the comet tale density by the background stars observations through the comet tale (task for future students)

Works with high/secondary scholars 14 – 16 years old Works that were awarded in local (St Petersburg) (St Petersburg) and Russian competitions Synthesis of color images of different objects from the CCD observations with BVR filters Looking for variable stars (short periods) in the open clusters χ and h Persei Investigation of PL dependence of Cepheids on the base of Hipparcos data and catalogue of variable stars Statistics of the IRAS stars classification Statistics of galaxies morphological types on the base of Deep fields HST images

Works with high/secondary scholars 14 – 16 years old Works that were awarded in ESO Catch a star! Catch a star! competitions The Moon (2003 – 3d prize) The Pleiades (2004 – special prize)

The idea of Pulkovo HOU center - We would like to create the center and tools that will help young men - to start with real work on astronomy in the high/secondary school, in the high/secondary school, - to continue this work at the University - and become the professional astronomers.

Thanks!