Interstellar spaceship simulator for astronomical education and communications 2007 Jul. 15 Tomonori Nomoto.

Slides:



Advertisements
Similar presentations
Development of a Galaxy HI observation system for the 8m radio telescope at Misato Observatory SATO Naoko, OKYUDO Masami, et al (Wakayama University),
Advertisements

E02 Science Live Show UNIVERSE -management and development- MATSUURA, Kyo (Team Chimons / University of Tsukuba) , 15 th July.
E01 Science Live Show UNIVERSE -history and overview- OGINO, Shino (Team Chimons / Nihon University ) 15 th July 2007 Global Hands-On Universe Conference.
Softwares to expand UNIVERSE liveshow KOIKE, Kuniaki ( The Graduate University for Advanced Studies / Team Chimons ) HANDA, Toshihiro.
Starlight and What it Tells Us. Brightness of Stars Variations in distance and intrinsic brightness Scale based on one by Hipparcos 500 B.C. Magnitude:
P1.5.4 Red-shift AQA GCSE Science A. There are two main pieces of evidence for the Big Bang: 1.The expansion of the universe 2. Cosmic microwave background.
7B Stars … how I wonder what you are.. 7B Goals Tie together some topics from earlier in the semester to learn about stars: How do we know how far away.
They seem to form a picture in the sky. People use them to find their way around the sky like someone using objects to get from place to place.
1. absolute brightness - the brightness a star would have if it were 10 parsecs from Earth.
Exam 1 Next Tuesday Covers chapters 1, 2, S1, 4, 5 and 6 2 essay questions/25 multiple choice Allowed one standard sized sheet of notes, writing on one.
Astronomical Imaging: Overview When you think of a clear, dark night sky, what do you think of? –The human visual system is fine-tuned to focus, detect,
Space Quiz Review – Go to Tomorrow SC.8.E.5.1 SC.8.E.5.2 SC.8.E.5.3 SC.8.E.5.4 SC.8.E.5.5.
Stars Properties: Brightness and Color Reasons for brightness: Proximity Temperature of star.
The Milky Way Galaxy.
Our Galaxy The Milky Way. The Milky Way Almost everything we see in the night sky belongs to the Milky Way We see most of the Milky Way as a faint band.
In this talk we'll see that : We can only see about 1% of the Universe The dark side And ask: What is the Universe made of?
Introduction to Astronomy Mr. Byrd Room D-14 Mr. Byrd Room D-14.
Various Techniques for Measuring Astronomical Distances Alex Blanton 1.
Stars, Galaxies, and the Universe
Science Focus Lesson Week 6 Polk County Public Schools Linda Vendur, Senior Coordinator.
WHAT ASTRONOMERS LEARN ABOUT THE ELECTROMAGNETIC SPECTRUM.
Instructions for using this template. Remember this is Jeopardy, so where I have written “Answer” this is the prompt the students will see, and where.
Stellar Parallax & Electromagnetic Radiation. Stellar Parallax Given p in arcseconds (”), use d=1/p to calculate the distance which will be in units “parsecs”
Exploring Space 1.1 Some space objects are visible to the human eye.
Exploring Space CHAPTER the BIG idea People develop and use technology to explore and study space. Some space objects are visible to the human eye. Telescopes.
Astronomy and the Electromagnetic Spectrum
Star Properties. Where do stars come from? Stars form in a cloud of dust and gas in space called a nebula.
STARS Ball of gases, mostly hydrogen and helium that give off energy A. Color- determined by surface temperature.
Light. Review Question What is light? Review Question How can I create light with a cow magnet?
Donna Kubik PHYS162 Fall, Because of its electric and magnetic properties, light is called electromagnetic radiation. It consists of perpendicular,
Chapter 19 The Stars Distances to stars are measured using parallax.
© 2011 Pearson Education, Inc. Chapter 1 Astronomy Today 7th Edition Chaisson/McMillan.
1 Stars Stars are very far away. The nearest star is over 270,000 AU away! ( Pluto is 39 AU from the Sun ) That is equal to 25 trillion miles! At this.
Chapter 8: Characterizing Stars. As the Earth moves around the Sun in its orbit, nearby stars appear in different apparent locations on the celestial.
PHYS 205 Surveying the Stars PHYS 205 Parallax The apparent change in the direction of the remote object due to a change in the vantage point of the.
Chapter 14 The Milky Way Galaxy What do you think? Where in the Milky Way is the solar system located? How fast is the Sun moving in the Milky Way? How.
The Milky Way Galaxy. HW #9 – MasteringAstro “Stars and Galaxies” Available now Tuesday April 17 th Due BEFORE CLASS Tuesday April 24 th Observing logs.
Stars, Galaxies, and the Universe Section 1 Section 1: Characteristics of Stars Preview Key Ideas Analyzing Starlight Stellar Motion Distances to Stars.
Astronomy Big Idea: The sun is one of billions of stars in one of billions of galaxies in the universe.
Intro to Astronomy Ch 26. Value of Astronomy Astronomy: the scientific study of the universe Scientists who study the universe are called astronomers.
Black Holes in Other Galaxies. The giant elliptical galaxy M87 is located 50 million light-years away in the constellation Virgo. By measuring the rotational.
Exploring Space CHAPTER the BIG idea People develop and use technology to explore and study space. Some space objects are visible to the human eye. Telescopes.
Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.
Hubble’s Law AST 112. Spectra If a light source is moving toward or away from an observer, its spectral lines shift We can use this to measure approaching.
EMS review. 1.Look at the above H-R diagram and list the sequence of stars from greatest to least luminosity. Deneb, Spica, Capella, Sirius B 2.Which.
Part 1: Distances in Space
Measuring the Stars (Part I). 3-D Positions in Space of the Stars Closest to our Sun:
(there’s no place like home) The Milky Way Galaxy.
Add to table of contents:  Pictures of telescopesPg. 82  TelescopesPg. 83.
Monday, November Warm-Up: Grade Content Frame 2. Astronomy Intro.
RADIATION AND SPECTRA Chapter 4 WAVESWAVES l A stone dropped into a pool of water causes an expanding disturbance called a wave.
Characteristics of Stars. What is a galaxy? It is a cluster of stars (hundreds of billions of stars) It is a cluster of stars (hundreds of billions of.
Deep Space and Solar System New Test/New Quiz. Universe Biggest Oldest Galaxy Milky Way Solar System Star Sun PlanetMoon Smallest Youngest.
Chapter 19 Stars, galaxies and the Universe. Section 1 Stars.
The Milky Way Galaxy. What are each of these?
 Pictures of telescopesPg. 96  TelescopesPg. 97.
Telescopes.
Lecture 30- The Structure of the Milky Way Galaxy
EMS review.
Stars, Galaxies, and the Universe
What makes up the universe and how does gravity affect the universe?
Since fusing hydrogen into helium causes a star to be on the main sequence, why do smaller stars stay on the main sequence longer than massive stars that.
Astronomy – A Study of “Our Space”
Radial Velocity and Proper Motion
Unit 11- Characteristics of the Universe
Introduction to Astronomy
Study Guide 3-2 Milky Way Universe Exploration
Chapter 10 Star Cluster.
Chapter 15 – Stars, Galaxies and the Universe
CFA #5 Space Technologies
Presentation transcript:

Interstellar spaceship simulator for astronomical education and communications 2007 Jul. 15 Tomonori Nomoto

Interactive simulation of the interstellar space journeys Hipparcos and Tycho catalogue, 1997 enabled 3D simulation outside of solar system, Mitaka, Partiview, StarStrider, Celestia,… etc. HippLiner… 2001 Originally, Constellation line drawing software for solar system simulator. Constellation line drawing software for solar system simulator.Currently, HippLiner is an Interstellar spaceship simulator HippLiner is an Interstellar spaceship simulator Interstellar jouney in the Science Live Show UNIVERSE Interstellar jouney in the Science Live Show UNIVERSE Free software. Not commercial software. Free software. Not commercial software.

HippLiner … Interstellar spaceship simulator Scientific data included: Stars near the Sun … stars The Hipparcos and Tycho Catalogues, ESA SP-1200, The Hipparcos input catalogue, ESA SP-1136, (radial velocity) Stars near the Sun … stars The Hipparcos and Tycho Catalogues, ESA SP-1200, The Hipparcos input catalogue, ESA SP-1136, (radial velocity) Open clusters … 601 clusters New Catalog of Optically Visible Open Clusters and Candidates, Dias et al, Open clusters … 601 clusters New Catalog of Optically Visible Open Clusters and Candidates, Dias et al, Galaxies … 2365 galaxies Nearby Galaxies Catalogue, Tully, Galaxies … 2365 galaxies Nearby Galaxies Catalogue, Tully, Special Features: 3D stereoscopic view is possible for liveshows. 3D stereoscopic view is possible for liveshows. 3D Constellation line writing function enables drawing your original constellations. 3D Constellation line writing function enables drawing your original constellations. Proper motion simulation under approximation of linear motion. Proper motion simulation under approximation of linear motion.

The Hipparcos and Tycho Catalogues, 1997 The Hipparcos input catalogue, D interstellar journey. 3D interstellar journey. Sky-view observed from outside of the sun. Sky-view observed from outside of the sun. Scientific Data Right Ascension DeclinationParallaxMagnitude B-V color index Radial Velocity Proper Motion stars

New Catalog of Optically Visible Open Clusters and Candidates, 2002 Nearby Galaxies Catalogue, 1988 Position of the open clusters or galaxies are also observable. 601 clusters 2365 galaxies

3D Constellation drawing Constellation drawing 88 constellations of IAU 88 constellations of IAU Chinese constellations Chinese constellations Your original constellations or lines Your original constellations or lines

Proper motion approximation 3D simulation of proper motions under an approximation of linear motion for stars with proper motions and radial velocities. 3D simulation of proper motions under an approximation of linear motion for stars with proper motions and radial velocities.

Recent improvements of HippLiner… Actually, currently working and almost finished. Star color Star color Using black body radiation and CIE XYZ color matching functions Using black body radiation and CIE XYZ color matching functions Relativity theory effect Relativity theory effect Doppler shift Doppler shift Aberration Aberration Proper time Proper time Originally 0 th magnitude.

Data needed for future plan Infrared, radio wave data of the space is needed. For 60 second journey to α Centaur, % of light speed is required For 60 second journey to α Centaur, % of light speed is required With high speed, stars become darker. With high speed, stars become darker. Point light source with originally 0 th magnitude (V) for each temperature.

In science live show, UNIVERSE In science live show, UNIVERSE In the section of Interstellar Cruising e.g. Nightview from α Centaur, or other stars Sirius and Betelgeuse becomes very close Sirius and Betelgeuse becomes very close

In science live show, UNIVERSE In science live show, UNIVERSE In the section of Interstellar Cruising e.g. Nightview from α Centaur, or other stars Sirius and Betelgeuse becomes very close Sirius and Betelgeuse becomes very close

Tanabata (): long distance of lovers A Chinese legend says… Separated cowherd (Altair) and weaving princess (Vega) meet through a bridge of magpies over milky way once in a year on Jul. 7th.

Tanabata (): long distance of lovers A Chinese legend says… Separated cowherd (Altair) and weaving princess (Vega) meet through a bridge of magpies over milky way once in a year on Jul. 7th. Magpies comes from quite far place!!

Summary HippLiner is a interstellar spaceship simulator including, HippLiner is a interstellar spaceship simulator including, stars from Hipparcos cataloge stars from Hipparcos cataloge 601 Open clusters 601 Open clusters 2365 Galaxies 2365 Galaxies 3D Constellation drawing function. 3D Constellation drawing function. Simulations of 3D proper motion Simulations of 3D proper motion Function of Simulating relativity theory effect including doppler shift, aberration and proper time as a real spaceship simulator is to be released near future. Function of Simulating relativity theory effect including doppler shift, aberration and proper time as a real spaceship simulator is to be released near future. HippLiner is a free software. You can download from HippLiner is a free software. You can download from I am happy if you get some inspiration or ideas for teaching or exhibitions by using HippLiner.

Acknowledgement Usage of the live show and basic ideas Dr. Toshihiro Handa Dr. Toshihiro Handa Dr. Toshikazu Ebisuzaki Dr. Toshikazu Ebisuzaki members of Team Chimons members of Team Chimons Extension application Mr. Kuniaki Koike Mr. Kuniaki Koike Drawing IAU and Chinese Constellations Ms. Sachiko Onodera, Mr. Kuniaki Koike, Mr. Kyo Matsuura, Mr. Seiichiro Naitoh, Ms. Akiko Nakano, and Mr. Yasuhide Yodo