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DIAGRAMA
DE PUNTOS
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| Note las estrellas
extremadament queñas y redondas , inclusive
a la orilla del campo de visión. Sólo
e diseño ótic de un RC Avanzad puede
prducir tal desempeñ fura del eje. Antes
del RCX400 de Meade ls astr´noms seris tenían
que pagar más de tres veces el cosot para
obtener un telescopio que ofreciera este nivel
de desempeño óptico profesional. |
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RCX400
PRICING (All Prices Include Shipping
& Handling in the 50 United
States) | |
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| MEADE RCX400
PRODUCT INNOVATIONS | |
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| Advanced f/8
Ritchey-Chrétien Optics:
The Ritchey-Chrétien or RC optical design is well known
to discerning astrophotographers and is the telescope
optical design in many of the leading professional observatories
of the world. Meade has taken its f/8 RC optical design
to another level by adding a corrector plate to reduce
residual astigmatism that is inherent in the traditional
optical design. In addition many more design features
were added to the RCX400 for the demanding researcher
and imaging enthusiast with telescopes available in
apertures of 10 inches, 12 inches, 14 inches, and 16
inches. |
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Series 5000
24mm 2" O.D.
Ultra Wide Angle Eyepiece:
Standard equipment on all RCX400 telescopes, the Series
5000 24mm 2" O.D. Ultra Wide Angle Eyepiece represents
the ultimate in eyepiece design and technology delivering
extremely high resolution, contrast and full-field sharpness
over an astounding 82° apparent field-of-view. Only
the highest quality materials were selected to create
this extraordinary eyepiece. The designs required several
different types of exotic glass in order to achieve
the highest level of optical performance. |
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New
Carbon Graphite & Kevlar Tube:
The carbon graphite and Kevlar tube is a unique light-weight,
high strength material with ultra-low expansion characteristics
that will maintain the spacing between the optics, so
that focus settings do not change with outside temperature
changes. This is a critical feature to astrophotographers.
Instead of forcing a perfectly round shaped tube assembly,
the tube is shaped around the mechanisms and drive system
of the front focus and collimation assembly, giving
the RCX400 its unique look and style. |
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New
Rear and Front Cell Architecture:
The front and back cells of the RCX400 are designed
to allow the maximum amount of air-flow around the optics,
in order to achieve the quickest "cool down" times.
To accelerate cool-down time, a built-in fan on the
rear cell can be turned on and off through the AutoStar
II handbox. The rear cell additionally incorporates
a multi-port panel with 3 USB ports, a port for an autoguider,
AutoStar II handbox, illuminated reticle, RS232, and
one for future "Smart" accessories. |
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RCX400 Drive Base:
The multi-port panel of the RCX400 drive base includes
a special single High-Speed USB 2.0 input port allowing
simultaneous control over the telescope and either the
Meade LPI or Deep Sky Imager camera through Meade's
AutoStar Suite software. Additionally there are ports
for a power cord input, the AutoStar II handbox, a DB-9
auxiliary port, 12v out power port, and RS-232. Additionally
the RCX400 includes the familiar on/off switch and LED
power light indicator. |
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New Ultra-Stable
Tripod:
Standard equipment for RCX400 10", 12", and 14" telescopes,
the patent pending trigger release leg locks of the
Ultra-Stable tripod are positioned at the top of the
tripod legs for easy access. |
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The RCX Advanced Ritchey-Chrétien Optical
System
It is generally accepted that the Ritchey-Chrétien or Classical
RC system is the premiere optical design for medium to large aperture
astronomical telescopes. The primary benefit of a Classical RC is
the fact that it is an aplanatic design which means it is coma-free.
Coma is an optical aberration that causes star images to appear
comet like with tails that point away from the center of the field
of view. The further from the center, the larger the effect. Fast
Newtonians suffer from this aberration the most, followed by other
reflecting optical systems of various designs. The Schmidt-Cassegrain
or Schmidt-Newtonian design typically has ½ the coma of a Newtonian
of the same focal length. The Classical RC design uses a hyperbolic
primary mirror and a hyperbolic secondary mirror to create an aplanatic
optical system which has no coma. This system produces small round
star images all the way to the edge of the field of view.
Meade’s engineering team recognized the advantages of the Classical
RC design but explored the possibility of using Meade’s unique engineering
and manufacturing expertise to improve on the basic design. The
result is the RCX optical system which is also an aplanatic, coma-free
design with small round star images to the edge of the field. The
RCX design is very similar to the Classical RC and achieves the
same benefits by using a hyperbolic secondary with a new advanced
front corrector plate and primary mirror that together perform as
a hyperbolic primary. This design has several advantages over the
Classical RC design.
- The RCX eliminates the secondary mirror holder
support vanes (spider) that cause diffraction spikes. Because
almost all reflecting telescopes produce diffraction spikes,
many people are used to seeing them and don’t consider them
an aberration. But in reality, they are a large distortion that
reduces image contrast, lowers resolution and presents an unrealistic
view of the sky to the eye or the astro-imager.
- The RCX design reduces the amount of astigmatism
that is inherent in the Classical RC design.
- The RCX, due to the front corrector plate,
is a closed tube design. This keeps the primary optical components
protected from dust, moisture and other contaminates that might
fall on the optical surfaces of the primary and secondary mirrors.
While the RCX optical system is significantly more
expensive to manufacture than a Classical RC, it was chosen because
of its superior performance (i.e., no diffractions spikes, reduced
astigmatism and closed tube). Due to Meade's years of experience
in designing and manufacturing sophisticated corrector plates and
optical systems, we are in a position that very few, if any, other
companies enjoy. Applying this expertise and Meade's resources,
we are able to produce this advanced optical system at a fraction
of the price that other companies would have to charge, if they
could produce it at all. |
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Precision GPS Alignment:
Telescope alignment is accomplished automatically using
signals from the Global Positioning System (GPS), a satellite
system that enables extremely precise communication to the
telescope of the observer's latitude and longitude, as well
as local time. Integrated True-Level and North electronic
sensors in combination with a high-sensitivity Sony GPS
receiver located in the left-hand fork arm result in accurate
telescope alignment to the sky at the touch of a button:
Just press the ENTER button on the Autostar II hand controller
and watch as the telescope measures level, points North,
and slews at 8°/sec. to its first alignment star. Magnetic
declination compensation designed into the telescope software
automatically engages during the alignment process.
Software Downloads and
Satellite Tracking:
The software included in Meade RCX400 telescopes is under
continuous factory review; updates to this software are
published at regular intervals on Meade's website. Importantly,
the latest software version, as well as custom and updated
guided tours, comet and asteroid positions, may be downloaded
in minutes from Meade's website. Additionally, current Earth
satellite orbital data (including the International Space
Station, Space Shuttle, etc.) may be downloaded; the telescope
then automatically acquires and tracks the satellite at
the correct tracking rate. The telescope's flash memory
may be upgraded through one of the RS-232 ports with new
software or data as they become available on Meade's website.
Expanded Database and
Larger User Memory:
The RCX400 database has been expanded over the standard
library of the LX200GPS to include 180,000 objects. In addition
to more stars from the Hipparchos/Tycho catalog, we have
added::
• The popular "Lunar 100" with the finest features to see
and image on the Moon
• A subset of the finest visual doubles from the Washington
Double Star Catalog
• The PK Catalog of Planetary Nebulae
• The Hickson Catalog of Dense Galaxy Clusters
• The Gleason Catalog of Nearby Stars
• The Landolt Catalog of Photometric Standard Stars
• The Sharpless Catalog of HII Regions
Laser Aligned, Fixed Primary Mirror:
The primary mirror is laser aligned to the true optical
path, then float bonded in place. It is fixed, but literally
floats on a layer of adhesive that results in zero stress
to the glass and no distortion to the optics (unlike mirror
cells or floating point pads). There is no mirror movement.
Field Operation:
RCX400 scopes operate from eight C-cells neatly stored inside
the fork arms. Alternately, telescope powering may be effected
from an automobile cigarette lighter plug (using the optional
#607 Power Cord) or from a standard home outlet (using the
new optional AC Adapter).
#929 2" Diagonal with UHTC:
Standard equipment on all RCX400 telescopes, attaches to
the rear cell of and permits the use of wide-field 2" O.D.
eyepieces. Each diagonal includes a Meade optical-flat mirror
of Pyrex glass, UHTC-coated for maximum reflectivity.
Built-In Dew Heater:
Instead of wrapping a heating element around the telescope's
optical tube assembly to send heat through the telescope's
front cell to prevent dew from forming on the corrector
plate, the RCX400 incorporates a nickel-chromium wire heating
element that is in contact with the glass of the corrector
plate that quickly, efficiently, and safely sends heat through
lens using the lowest power drain possible. With two onboard
temperature sensors, one to measure ambient temperature
(placed inside the fork arm) and one to measure the temperature
of the corrector plate, the RCX400 can be set to have the
built-in dew heater keep the corrector plate warmed to a
user-defined setting above ambient temperature. By only
using the dew heater precisely when needed, battery usage
is managed to its optimum. All functions to operate the
dew heater are controlled by the AutoStar II handbox.
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Precision Encoder-Measured
Digital Focusing:
With a laser aligned primary mirror fixed in position, focusing
is performed electronically and digitally by precisely moving
the entire front cell in increments as fine as 1/100 of a
millimeter. Digital readout of the focus position can be read
on the telescope's AutoStar II handbox. There are 4 different
focusing speeds from fine to fast. Since the process is accomplished
without moving the primary mirror, the entire assembly is
virtually free from image shift.
High-Precision Pointing (HP)
Capability:
Meade RCX400 models permit the most accurate pointing capability
ever offered in a commercial telescope. Now you can command
the telescope to GO TO an object located on the opposite side
of the sky (for example, a distance of 120 degrees in sky-angle)
and, in conjunction with the telescope's unique SYNC command,
the RCX400 locates and centers the desired object. HP capability
is accessible in either the altazimuth or equatorial orientations.
Precision Electronic Optical Collimation:
Collimating a Cassegrain telescope has never been
easier. RCX400 owners will make precision collimation adjustments
to the secondary mirror of the telescope by using the arrow
keys of AutoStar II handbox, allowing a single person to simultaneously
make adjustments and see the results. In addition, Meade precision
collimates the optics at the factory and then sets that position
as the default setting. So in the case where one may make
a mistake in making a collimation adjustment, the default
setting can always be used.
Smart Drive Permanent Periodic
Error Correction (PPEC):
Included as standard equipment, the Smart Drive permits a
professional level of drive-rate precision. No longer are
large systems required, worm gear when smaller gears coupled
to Smart Drive software can achieve periodic errors of 5 arc
secs or less-an observatory standard of precision. All worm/worm-gear
combinations, no matter how well made, have minor inaccuracies
that manifest themselves as periodic errors in the telescope
tracking rate, with the period dependent on the worm's rate
of rotation. To program the Smart Drive the observer guides
on an object visually, making corrections with the handbox
controller. The software then remembers these corrections,
stores them in memory, and in the future automatically compensates
for the periodic errors of the gear system. Smart Drive user
programming is stored in the telescope's computer memory forever,
independently of any power source, unlike other periodic error
correctors that must be reprogrammed each time you use the
system. The Smart Drive can be erased, updated, or even averaged
with future programming at the user's option. The significant
value of the Smart Drive is immediately appreciated during
long-exposure astrophotography, where the resulting low periodic
error of the system enables relaxed guiding with a minimum
of handbox corrections. In CCD imaging, where short exposures
of deep-space objects are often all that is required for stunning
results, the Smart Drive often permits imaging without any
guiding requirements at all.
Heavy-Duty Fork Mounts:
RCX400 fork mounts are the strongest, most rigid mountings
ever made available for telescopes of these apertures. Fork
arms, are both longer and stronger. This allows the 10", 12"
and 14" scopes to go all the way to 90 degrees declination
on a wedge, allowing you to reach the horizon. The increased
fork size also gives more back clearance to allow imaging
all the way to the pole with most cameras. DC-servo-motor-controlled
(12v DC) worm gear drives with almost two hundred selectable
drive speeds, combined with the Meade Smart Drive on both
telescope axes, permit observatory-level precision in tracking,
guiding, and slewing. Photo-guide speeds are selectable from
0.01x to 1.0x sidereal, in increments of 0.01x; fast-slew
speeds are selectable from 1°/sec. to 8°/sec. in 0.1°/sec.
increments. Use the 8°/sec. speed for rapid motion of the
telescope across the skies; once near the target, switch instantly
to a speed of 1.5°/sec. or 3°/sec. for centering in the viewfinder.
Observing in the main telescope, use the 16x or 64x sidereal
speed to place the object in the center of the field.
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Computer Optimized
Internal Baffling: Unlike
traditional Schmidt-Cassegrain designs, the primary mirror
moves along a baffle tube in order to achieve focus, Meade's
RCX400 primary mirror is mounted independent of the baffle
tube. This allowed Meade's engineers to take full advantage
of the baffle design to create full stray light cut-off
performance, in order to produce the maximum contrast. Additionally
the secondary baffle, machined of aluminum with its distinctive
outer knife-edges further minimizes stray light in the optical
path.
RCX400 Balanced Drives:
The drive mechanisms of many telescopes can be compared
to the movements of fine chronometer watches. First utilized
on the 14" LX200GPS, the RCX worm block design incorporates
a unique balanced loading system to the keep worm and worm
gear in the optimum contact position, regardless of the
load stress that is normally encountered as the telescope
is moved from one position of the sky to the next. The result
is improved drive performance, with superior centering and
slewing characteristics. RCX400 Balanced Drive assemblies
are on both the RA and Dec. axes.
Focus Position Presets:
By setting up to 9 focus positions, RCX400 owners can customize
perfect focus from observer to observer with different eyesight
(similar to the custom settings in luxury cars to change
the mirror, seat, and steering wheel settings from one driver
to another). The feature is also very useful when using
switching to various eyepiece and Barlow lens combinations
or from a visual setup to a camera setup.
UHTC Coatings:
Standard on all RCX400 telescopes, the importance of Meade's
proprietary UHTC group becomes apparent when comparing total
telescope light transmission, or throughput, caused by the
multiplier, or compounding, effect of the four optical surfaces.
With each optical surface contributing significantly to
telescope light throughput, the effect of all four surfaces
combined is indeed dramatic. At the H-a wavelength of 656nm.,
total transmission increases from 76.7% to 88.5%, an increase
of 15.4%; at the helium wavelengths of 588nm. and 469nm.
- strong emission lines in hot planetary nebulae - total
telescope transmission increases by 13.8% and 16.8%, respectively;
at the two nitrogen II lines of 655nm. and 658nm. and at
the sulfur II line of 673nm., transmission is increased
by 16%. Averaged over the entire visible spectrum (450nm.
to 700nm.), total light transmission to the telescope focus
increases by about 15%.
More Info
about UHTC
Smart Mount:
Revolutionary Smart Mount technology is standard equipment
on all RCX400 telescopes. Smart Mount improves the pointing
accuracy of your RCX400's telescope's "Go To" system with
the following features:
• Constantly improved pointing accuracy with every object
centered and sync'ed.
• Works with both equatorial and altazimuth configurations.
• Simple routine to refine pointing accuracy for the entire
sky with your equipment configuration and alignment.
• Refined pointing data can be saved and reused for permanent
and portable setups.
Altazimuth and Equatorial Operation:
For all visual observing applications, for lunar and planetary
photography, and for many CCD imaging applications, Meade
RCX400 may be set up in the altazimuth mode - just attach
the telescope's drive base directly to the tripod, use the
GPS alignment procedure, and the telescope's computer actuates
2-axis tracking that keeps objects precisely centered in
the field, even at high powers, during the entire observing
session. For long-exposure astrophotography altazimuth-induced
field rotation requires the new Ultrawedge or the #1220
(for 10", 12", and 14" models) or the #1222 (for 16" models)
Field De-rotater, either of which may be purchased separately.
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KEY
FEATURES
GPS & Level-North Alignment
System
Upgraded AutoStar II Controller
Cooling Fan
Smart Mount™
Smart Drive™ (Permanent Periodic Error Correction)
Oversized Primary Mirror
24mm Series 5000™ Ultra Wide Angle Eyepiece
Ultra High Transmission Coatings (UHTC) |
| SPECIFICATIONS |
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| Aperture |
10" |
12" |
14" |
16" |
| Focal Length |
2032mm |
2438mm |
2845mm |
3251mm |
| Focal
Ratio |
f/8 |
f/8 |
f/8 |
f/8 |
| Series 5000™ Eyepiece |
24mm UWA |
24mm UWA |
24mm UWA |
24mm UWA |
| UHTC™ |
Included |
Included |
Included |
Included |
| Accessory Kits |
Click Here |
Click Here |
Click Here |
Click Here |
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Meade, the Meade logo, are trademarks registered with the United
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world. Copyright
© 2005 Meade Instruments Corporation, All Rights Reserved.
This material may not be reproduced in any form without
permission. | |