EPOXI Mission News Options

[stevesliva]

Looks like the Deep Impact list has been revived. Posting here for others to get back on board:

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EPOXI E-News #1 May 2008
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WELCOME BACK!

Did you know that the Deep Impact Flyby Spacecraft has a new assignment? The
EPOXI mission combines two exciting science investigations in an entirely
new mission that re-uses the Deep Impact spacecraft. The Extrasolar Planet
Observation and Characterization (EPOCh) investigation will observe stars
that have known transiting giant planets. The Deep Impact Extended
Investigation (DIXI) of comets observes comet 103P/Hartley 2 during a close
flyby in October 2010.

The education and public outreach team decided to get back in touch with our
Deep Impact friends and begin sending out newsletters again to keep you
informed of these two exciting investigations! During the two years since
our last newsletter for Deep Impact, the science team has stayed busy
continuing to do more analysis on the data collected in July 2005. The
science team also proposed and was awarded an extended mission teaming up
with a group from Goddard Space Flight Center.
EPOXI website: http://epoxi.umd.edu/
Mission Overview: http://epoxi.umd.edu/1mission/index.shtml
Press Releases: http://epoxi.umd.edu/7press/index.shtml
DI Results: http://deepimpact.umd.edu/results/

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MISSION STATUS

Dr. Deming, Principal Investigator (PI) for the EPOCh portion of the
mission, sends us the latest mission status report in which he tells us
about the current observing target GJ436. “This is an exciting time for
EPOCh, as we search for an exo-Earth orbiting a stellar neighbor of our
Sun!” reports Dr Deming. He also talks about the plans to observe a very
special planet in late May and early June.

Read his status report as well as past reports from other team members at
http://epoxi.umd.edu/1mission/status.shtml

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EPOCh TARGETS

The EPOCh component of the EPOXI mission will carefully study a small number
of stars in order to learn more about planets that we know are orbiting
those stars by watching the planets as they transit (cross in front of) the
star. EPOCh will also search for clues to other planets that might be
orbiting the same stars.

Read more about the EPOCh science targets to find out which stars are being
observed.
http://epoxi.umd.edu/2science/targets.shtml

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PLANET QUEST

Are we alone?
For centuries, human beings have pondered this question. Medieval scholars
speculated that other worlds must exist and that some would harbor other
forms of life. In our time, advances in science and technology have brought
us to the threshold of finding an answer to this timeless question.
The recent discovery of numerous planets around stars other than the sun
confirms that our solar system is not unique. Indeed, these "exoplanets"
appear to be common in our galactic neighborhood.
The EPOCh investigation is part of a larger family of missions studying
extrasolar planets. Learn more at the Jet Propulsion Lab Planet Quest Web site.
http://planetquest.jpl.nasa.gov/index.cfm

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OBSERVING CHALLENGE

The transits that will be studied for EPOCh are extremely difficult to
observe because the change in brightness is very small and requires high
precision photometry that can be accomplished with instruments on the Deep
Impact spacecraft. Observers on Earth can still take a look at the stars in
the night time sky. The selected stars are also pretty dim because we don’t
want them to saturate or over expose the spacecraft instruments but they are
bright enough to be visible in amateur telescopes if the sky conditions are
good and the skies are dark.

Like people, stars have multiple identifiers. EPOCh’s first target was a
star labeled as HAT-P-4 by the scientists observing it. They made their own
list of target stars so that was their shorthand name. But HAT-P-4 has
numerous other names which are more useful in identifying it in other databases.
HAT-P-4 = SAO 64638 = TYC 2569-1599-1 is a magnitude 11, G-class star
located in the constellation Boötes.
Chart: http://epoxi.umd.edu/2science/challenge.shtml

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SUBSCRIPTION INFORMATION

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subscribers may join the EPOXI Mission e-news mailing list on our website
at: http://epoxi.umd.edu/6outreach/newsletter.shtml

[Paolo]

A nice presentation "Remote Detection of Life on Earth ….inferences from EPOXI"

[Paolo]

Hi all,

I just noticed a new article on the EPOXI website by the EPOCh P.I. Drake Deming:

http://epoxi.umd.edu/2science/alienmaps.shtml

Enjoy!

~Rich

The article Alien Maps of an Ocean-Bearing World is now on arxiv

[Paolo]

There is a mission update on the EPOXI site: http://epoxi.umd.edu/1mission/status.shtml

Characterizing Comet Hartley 2
Although the EPOXI mission's spacecraft is in a period of relative inactivity, the team is still actively working on a variety of questions. One of the key areas of investigation is the characterization of the next target, comet Hartley 2. Several investigations have been carried out to characterize the nuclear size and albedo, the large dust, and the rotation of the nucleus. These investigations have been aimed for the period before the nucleus begins outgassing significantly as it approaches the sun.

Observation were taken with the Spitzer Space Telescope in August 2008. The analysis of those data yields a nuclear effective radius of 0.6 km, slightly smaller than, but still comparable to, the size deduced using the European Infrared Space Observatory at the previous apparition. These observations also show that there is a trail of large dust particles released much earlier and still orbiting the sun close to the nucleus. This is a common phenomenon among comets.

The next step was an effort to determine the rotational period in order to design the observing sequence for the approach to the comet. A series of observations with the Hubble Space Telescope in late April were somewhat puzzling. Subsequent observations with a variety of ground-based telescopes, particularly with Gemini-South and Gemini-North on the same night, have suggested a rotational period near 2/3 day, but with narrow minima that were not caught in the HST observations.

[Paolo]

From the latest Discovery and New Frontiers Newsletter

Although the EPOXI mission's spacecraft is in a period of relative inactivity, the team is actively working on a number of areas of interest, including characterizing the next target, comet Hartley 2.
Several investigations have been carried out to characterize the nuclear size and albedo, the large dust, and the rotation of the nucleus. These studies are timed for the period before the nucleus begins outgassing significantly as it approaches the sun. Another effort is to determine the Hartley 2’s rotational period to design the observing sequence for the approach to the comet. A series of observations with the Hubble Space Telescope in late April were somewhat puzzling. Subsequent observations with a variety of groundbased telescopes, particularly with Hawaii’s GeminiSouth and GeminiNorth on the same night, suggest a rotational period near 2/3 day, but with narrow minima that were not caught in the HST observations.
The team is preparing to continue its role in testing software that could lead to improved interplanetary network communications. Last fall, a NASAwide team used DisruptionTolerant Networking, or DTN, software to transmit dozens of space images to and from the Deep Impact spacecraft which was more than 20 million miles from Earth. The test was called DINET (Deep Impact DTN experiment). Computers on the ground at JPL were used to simulate stations on Earth, Mars, and the Martian moon Phobos. The experiment was successful, with all the data transmitted without corruption even as various faults and breakdowns in the system were simulated.
The team was pleased to support this activity that will ultimately lead to much better communications across the solar system. The Preliminary Design Review for DINET2 was conducted on May 13. The current timeline is being reviewed to determine when to begin DINET2 activities on the spacecraft. It may begin following the infrared imaging of Earth at high southern latitudes scheduled for August 17.

[Paolo]

Published at last Spitzer Space Telescope Observations of the Nucleus of Comet 103P/Hartley 2

[dmuller]

There was a somewhat distant Earth flyby of Epoxi on 29 June at some 1.3 million km ... distant yet Epoxi is still closer to Earth than Planck is at the moment. Next close-ish approach at the end of the year

[Paolo]

A very short update on EPOXI's mission page

[Paolo]

Browsing the DSN schedule (http://rapweb.jpl.nasa.gov/Planning/TMODMISS.pdf) I noticed that EPOXI is to conclude in November 2010 after the Hartley flyby, but the document gives a "probable end" date for the mission of 31 October 2011. Any idea what they plan to use the spacecraft for during the intervening year?

[IM4]

Any idea what they plan to use the spacecraft for during the intervening year?

EPOXI trajectory from HORIZONS lasts till February 1, 2012. My program predicts several distant flybys of tiny asteroids and pass through cloud of Schwassmann-Wachmann comets:

CODE

    Object Name              Distance(AU)  Date
73P-BB/Schwassmann-Wachmann    0.15935    2011-May-30
73P-V/Schwassmann-Wachmann3    0.06787    2011-Jun-15
73P-BD/Schwassmann-Wachmann    0.06865    2011-Jun-21
73P-BG/Schwassmann-Wachmann    0.06644    2011-Jun-28
73P-BR/Schwassmann-Wachmann    0.07153    2011-Jul-02
73P-BF/Schwassmann-Wachmann    0.09753    2011-Jul-23
73P-AT/Schwassmann-Wachmann    0.11083    2011-Aug-27

I guess they could tweak spacecraft's trajectory and study some of these objects.

[Paolo]

I wrote to EPOXI PI to ask for some clarifications and he tells me that

Oct 2011 is the official end of our contract from NASA for EPOXI, but that includes the preliminary analysis phase. Our current plan is that spacecraft operations will end in Dec 2010.

[Paolo]

On ArXiv today A Search for Additional Planets in the NASA EPOXI Observations of the Exoplanet System GJ 436

[elakdawalla]

I'm pretty sure the answer is "no" but I thought I'd check here...has there been a PDS release of any of the Deep Impact / EPOXI data from after the Tempel 1 encounter? Specifically, have any of the MRI or HRI images of Earth and/or Moon hit the PDS?

--Emily

[djellison]

http://pdssbn.astro.umd.edu/missions/epoxi/index.html

Nothing.

[Rich]

Hi all:

Just a quick update. EPOXI scientists have discovered water absorption features on the moon. The data was obtained from the IR spectrometer calibrations taken in December and twice in June. Chandryaan's M3 instrument also observed similar absorption features. This was published in Science yesterday. Read more here:
http://epoxi.umd.edu/2science/hydratedmoon.shtml

~Rich

[Paolo]

Yet another EPOXI-related paper on arXiv:
Studying the atmosphere of the exoplanet HAT-P-7b via secondary eclipse measurements with EPOXI, Spitzer and Kepler