The International MarsWatch 2003

Linking Amateur and Professional Mars Observing Communities


Site Index

Breaking News

  • 31 AUG 2004 – Opposition season over; site closed to any further modification and archived.
  • 14 JUL 2004 – Some new images have arrived showing Mars in the ultraviolet and the near infrared. For some information on what you are seeing in them, check out the Non-visible Wavelengths paragraphs on the images page. With the exception of these, it appears the season is officially over. Note that although I am considering the site "close" until 2005, I will still add any images or information contributors may wish to send my way. I'd especially like to hear about more results from any of the professional observers.
  • 20 APR 2004 – Some new images are still coming in and the resolution at this small angular diameter is looking good. We are working on another method to view images, namely by observer instead of by date; that page should roll out soon. My students and I will also soon have some summary images from our NASA IRTF imaging in the near-infrared.

    All spacebourne programs are working wonderfully! The amount of data flooding back to Earth seems almost overwhelming. Both rovers have had their missions extended and there is some strong evidence that liquid water was around to make some of the minerals being seen.

  • 06 JAN 2004 – The images and news from Spirit is coming in fast and furious! To keep up with the latest, go to the following web sites: JPL Mars Rover Mission Home or JPL MER Info Home; The new color pictures are amazing! You can also check out the web site of the rover science team. I will have a newsletter with some summaries once I get all caught up with it.
  • 05 JAN 2004 – MarsWatch website updated with lastest dust activity archives
  • 04 JAN 2004 – Spirit has bounced down, opened and taken its first picture! Keep up to date via NASA TV webcasts.
  • 25 DEC 2003 – Mars Express arrives at Mars and the Beagle has landed! Unfortunately, no contact has yet been made but there is still hope to hear from it
  • 30 NOV 2003 – A possible detection of a duststorm in NW Hellas by Erwin van der Velden; can anyone confirm?
  • 12 NOV 2003 – Added information on non-visible-light observations to the images page; Newsletter 5 is out.
  • 08 OCT 2003 – Newsletter 4 is out.
  • 25 AUG 2003 – Hubble to take images of Mars on 26 Aug 22:30-23:12 UTC and 27 Aug 09:43-10:43 UTC. Images will be available after the observations at their web site
  • 15 AUG 2003 – There is a MarsWatch event in San Diego County, CA
  • 04 AUG 2003 – Newsletter 3 is out. Is everyone getting ready for opposition?
  • 15 JUL 2003 – Mike Smith reports that TES data through 12 July show dust storm in decay. See ASU TES site to see dust storm progress
  • 07 JUL 2003 – Opportunity, MER-B, lifts off from Florida 15:18 UT! Keep track of all currently traveling missions at JPL's MER site
  • 07 JUL 2003 – Newsletter 2 is out. If you are not receiving it via e-mail, subscribe
  • 02 JUL 2003 – Folks are seeing dust activity around Hellas (see early July images)
  • 10 JUN 2003 – Spirit, MER-A, lifts off from Florida 17:58 UT
  • 02 JUN 2003 – Mars Express lifts off from Kazakhstan 17:45 UT
  • 01 JUN 2003 – Monthly newsletters begin
  • 31 MAR 2003 – The Rowan University MarsWatch 2003 web page and ftp site are up and running!
Mars Links

Other Mars Links — Feel free to submit your favorite Mars links to David Klassen for inclusion

MarsWatch Information

Who are we?

The International MarsWatch is a group founded by amateur and professional astronomers more than 30 years ago to facilitate better communication between the amateur and professional Mars observing communities. This network currently consists of over 150 professional and amateur astronomers who are interested in Mars or active in Mars research.

What are we doing?

The primary purpose of this project is frequent CCD imaging of Mars using B,V,R or other standard filters and visual drawings and photos in order to monitor the planet's atmospheric dust and cloud activity.

Secondary goals include imaging or spectroscopic characterization of the surface color and mineralogy, characterization of the growth and retreat of the polar caps, and analysis of atmospheric water vapor content. Because Mars rotates at nearly the same rate as the Earth and it also has a dynamic atmosphere that exhibits hourly, daily, and seasonal changes, frequent observations from observatories spanning the widest possible range of longitudes are desired.

Here you will find images of Mars contributed by amateurs and professional, tools to aid you in planning your own Mars observations, current and past issues of the International Mars Watch Electronic Newsletter, and links to other Mars-relevant sites on the Internet.

When is all this happening?

The next opposition of Mars will be in late August 2003 but the observing season spans a period of about three months before to three months after the opposition date. During this time the apparent size of Mars will increase from about 5" in diameter to about 25"! This means that Mars will be an impressive sight in telescopes of all sizes.

As we all acquire our images of the Red Planet, they can be uploaded to the official MarsWatch FTP site. This site is up and running, ready for your contributions. It will remain open throughout the entirety of 2003 at which point all the images will be collected into a single archive. This archive will be available from this site.

Where...?!

All the information you need will be here at this WWW site. There are links to the MarsWatch sites for the previous oppositions, as well as many other Mars related links. Breaking news will be published here, at the top of the page once things get underway, and in the MarsWatch Electronic Newsletter. If you are interested in receiving the newsletter, please subscribe!

As for where to make Mars observations the answers is: Anywhere! Mars changes on short timescales so it is important to observe it over it throughout the year. Mars also rotates once every 24 hours so having observers spread throughout the world will allow us to monitor Mars at all longitudes throughout a single Mars "day".

Why?

Mars is the subject of intense study by NASA and NASA funded researchers. Although we have learned much about the Red Planet, there is still much to learn — How much water is there on Mars? How does this water move about? What about the possible "warm, wet Mars"? Are the dry river beds from surface or underground flows?

To help answer these questions NASA has put the Mars Global Surveyor (MGS) into Mars obit and has plans on a whole host of spacecraft to visit image the planet. We telescopic observers will be looking at the planet to put MGS images into a global context (MGS is in a solar polar orbit and thus only sees the local 2 p.m. and 2 a.m. Mars surface). We will also identify and track the dust and ice clouds. The MarsWatch program is designed to create a place where all observers can share their knowledge and images throughout the observing season. Our goal will be to create a global view of Mars every day. The images submitted with then be available to the entire observing community (and the public in general) for comparison and interpretation.

How can I participate?

Observe! In order to create the best possible set of comparable images, observations through standard B, V, R, and I filters is encouraged. Once you have your images, and a short description of the image, submit them here for everyone to see. You can get full instructions on the official MarsWatch FTP site.

Prior to observing, if you can, submit your observing plan so others will know what sort of coverage you hope to get so they can plan coordinating observations. You can e-mail your plans, and any other comments, to David Klassen at Rowan University — otherwise known as "he who will maintain this site and publish the MarsWatch Newsletters". Your observing plans, and comments if you wish, will be put into the next Newsletter and on this site.



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