The Milky Way Project

The educational technology and digital learning wiki
Revision as of 15:36, 14 November 2013 by Himmelattack (talk | contribs) (Created page with "{{Citizen science project |field_project_name=The Milky Way Project |field_project_access_URL=http://www.milkywayproject.org/ |field_screenshot=Capture d’écran 2013-11-14 ...")
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to navigation Jump to search
Low
Medium
High
Complete

Cs Portal > List of citizen science projects > The Milky Way Project - (2013/11/14)

Capture d’écran 2013-11-14 à 15.26.38.png
Capture d’écran 2013-11-14 à 15.26.38.png
CCLlogo.png
CCLlogo.png


IDENTIFICATION

Participant's homepage
Start date :
  • Beta start date : N/A
  • End date :
Subject

Description We're asking you to help us find and draw circles on infrared image data from the Spitzer Space Telescope. Understanding the material that we see in these images helps scientists to learn how stars form and how our galaxy changes and evolves with time. Purpose The Milky Way Project is currently working with data taken from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) and the Multiband Imaging Photometer for Spitzer Galactic Plane Survey (MIPSGAL). We aim to bring you a host of interesting science problems as time goes by, and to begin with we're looking for bubbles. These bubbles are part of the life cycle of stars. Some bubbles have already been found - by the study that inspired this project - but we want to find more! By finding more, we will build up a comprehensive view of not only these bubbles, but our galaxy as a whole. We're asking you to help us map star formation in our galaxy. ? Research question The bubbles you see in this project are sometimes complete, and round, but often not. There are a great many bubbles that look like they have burst or faded away - or been disrupted by other bubbles. You can help us in this area by identifying bursting or distorted bubbles and figuring out the angle at which they burst or the eccentricity of their shape. This information will allow us to reconstruct bubbles to see how it evolved and grew. Maybe the bubble ran out of material, or maybe there is something stranger afoot!

TEAM

MAIN TEAM LOCATION
Loading map...

University of Oxford

Project team page http://www.milkywayproject.org/team Leader: Institution: University of Oxford Partner institutions: Adler Planetarium, Jeremiah Horrocks, Herschel Institute, Spitzer Space Telescope, HiGal Contact: http://www.milkywayproject.org/contact

USER TASKS

CONTRIBUTION TYPE:
PARTICIPATION TYPOLOGY:


GAMING GENRE NONE
GAMING ELEMENTS: NONE

COMPUTING
THINKING
SENSING
GAMING

Tasks description

Interaction with objects

Interface

  • Data type to manipulate:
  • interface enjoyment:
  • Interface usability:

GUIDANCE

GUIDANCE
  • Tutorial: Somewhat
  • Peer to peer guidance: Somewhat
  • Training sequence: Somewhat
FEEDBACK ON
  • Individual performance: Somewhat
  • Collective performance: Somewhat
  • Research progress: Somewhat

Feedback and guidance description

COMMUNITY

COMMUNITY TOOLS
  • Communication:
  • Social Network: N/A
  • Member profiles:: N/A
  • Member profile elements:
NEWS & EVENTS
  • Main news site:
  • Frequency of project news updates: N/A
  • Type of events:
  • Frequency of events :

Community description

  • Community size (volounteers based)
  • Role:
  • Interaction form:
  • Has official community manager(s): N/A
  • Has team work N/A
  • Other:
  • Community led additions:


Other information

PROJECT

Url:http://www.milkywayproject.org/
Start date:
End date:
Infrastructure: Zooniverse

TEAM

Official team page:http://www.milkywayproject.org/team
Leader:
Institution: University of Oxford
Partner institutions: Adler Planetarium, Jeremiah Horrocks, Herschel Institute, Spitzer Space Telescope, HiGal
Contact: http://www.milkywayproject.org/contact
Main location: University of Oxford

PROJECT DEFINITION


Subject

Natural sciences > astronomy, astrophysics (space)

Description

We're asking you to help us find and draw circles on infrared image data from the Spitzer Space Telescope. Understanding the material that we see in these images helps scientists to learn how stars form and how our galaxy changes and evolves with time.

Purpose.

The Milky Way Project is currently working with data taken from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) and the Multiband Imaging Photometer for Spitzer Galactic Plane Survey (MIPSGAL). We aim to bring you a host of interesting science problems as time goes by, and to begin with we're looking for bubbles. These bubbles are part of the life cycle of stars. Some bubbles have already been found - by the study that inspired this project - but we want to find more! By finding more, we will build up a comprehensive view of not only these bubbles, but our galaxy as a whole. We're asking you to help us map star formation in our galaxy.

Research question.

The bubbles you see in this project are sometimes complete, and round, but often not. There are a great many bubbles that look like they have burst or faded away - or been disrupted by other bubbles. You can help us in this area by identifying bursting or distorted bubbles and figuring out the angle at which they burst or the eccentricity of their shape. This information will allow us to reconstruct bubbles to see how it evolved and grew. Maybe the bubble ran out of material, or maybe there is something stranger afoot!

ABOUT PARTICIPANT TASKS


.

.

Grey typology Participation typology Contribution type:
Computing: NO Thinking: NO
Sensing: NO Gaming: NO
Crowdsourcing Distributed intelligence
Participatory science Extreme citizen science
Science outreach
Data collection
Data analysis
Data interpretation --------
Gaming
Genre: Gaming elements:
Interface
Data type to manipulate: interface enjoyment:
Interface usability:
Member profiles::N/A
Member profile elements:


ABOUT GUIDANCE AND FEEDBACK


Guidance Feedback on
Tutorial and documentation: SOMEWHAT
Training sequence: SOMEWHAT
Peer to peer guidance: SOMEWHAT
individual performance: Somewhat
collective performance: Somewhat
research progress: Somewhat

.

COMMUNITY


Tools News & Events

Communication:
Social Network: N/A

Main news site:
Frequency of project news updates: N/A
Type of events:
Frequency of events :

Community description

Community size (volounteers based):
Role: Interaction form:
Has official community manager(s): N/A
Has team work N/A

Other information about community:
Community led additions:

OTHER PROJECT INFORMATION




Capture d’écran 2013-11-14 à 15.26.38.png No

http://www.milkywayproject.org/team

University of Oxford http://www.milkywayproject.org/contact

No astronomy, astrophysics Natural sciences space The Milky Way Project is currently working with data taken from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) and the Multiband Imaging Photometer for Spitzer Galactic Plane Survey (MIPSGAL). We aim to bring you a host of interesting science problems as time goes by, and to begin with we're looking for bubbles. These bubbles are part of the life cycle of stars. Some bubbles have already been found - by the study that inspired this project - but we want to find more! By finding more, we will build up a comprehensive view of not only these bubbles, but our galaxy as a whole. We're asking you to help us map star formation in our galaxy. The bubbles you see in this project are sometimes complete, and round, but often not. There are a great many bubbles that look like they have burst or faded away - or been disrupted by other bubbles. You can help us in this area by identifying bursting or distorted bubbles and figuring out the angle at which they burst or the eccentricity of their shape. This information will allow us to reconstruct bubbles to see how it evolved and grew. Maybe the bubble ran out of material, or maybe there is something stranger afoot!

The Milky Way Project



, other: Thinking: no Computing: no Sensing: no Gaming: no



N/A N/A N/A N/A N/A N/A

N/A

N/A

N/A



N/A


N/A




Bibliography

BIBLIOGRAPHY