Astronomical Audio Pronunciation Guide

Some astronomical monikers truly do seem alien, and ensuring correct pronunciation can be hazardous for even the most advanced educator. Starry Night Education is here to help with our Audio Pronunciation Guide for the top 500 most commonly mispronounced astronomical objects, from Acamar through Zubeneschamali.

Choose your category:
asteroids
constellations
planets
meteors
stars

     
Click the name to hear the correct pronunciation.

Asteroids

 
 
Name
Pronunciation
 
ANN-FRANK
 
a-PAW-fis
 
a-STREE-a
 
BACK-us
 
BRAIL
 
SEER-eez
 
e-JEER-ee-a
 
EER-os
 
ewe-NOM-ee-a
 
FLOOR-a
 
for-TUNE-a
 
HEE-bee
 
hy-GEE-a
 
eye-REE-nee
 
EYE-ris
 
JEW-noe
 
ka-LYE-o-pee
 
lew-TEE-sha
 
ma-SALL-ee-a
 
mel-POM-e-nee
 
MEE-tis
 
PAL-as
 
par-THEN-o-pee
 
SYE-kee
 
SIL-vee-a
 
the-LYE-a
 
THEE-tis
 
VES-ta

Constellations

 
 
Name
 
Pronunciation
 
an-DROM-eh-da
 
ANT-lee-uh
 
APE-us
 
ack-KWAIR-ee-us
 
ack-WILL-lah
 
AY-rah
 
AIR-ease
 
or-EYE-gah
 
bow-OH-tease
 
SEE-lum
 
ca-MEL-oh-PAR-dal-iss
 
KAN-surr
 
KAN-es veh-NAT-ih-see
 
KANE-es MAY-jer
 
KANE-es MY-ner
 
CAP-rih-CORN-us
 
car-EE-na
 
KASS-ee-oh-PEE-ah
 
sen-TOR-us
 
SEE-fee-us
 
SEE-tus
 
kah-ME-lee-un
 
SIR-sin-us
 
ko-LUM-ba
 
CO-ma bare-uh-NYE-sees
 
coe-ROW--nah ow-STRAHL-iss
 
coe-ROW--nah BOR-ee-AL-iss
 
CORE-vuss
 
CRAY-ter
 
Kruks
 
SIG-nus
 
del-FYE-nus
 
doh-RAY-doh
 
DRAY-ko
 
eh-KWOO-lee-us
 
eh-RID-uh-nuss
 
FOR-naks
 
GEM-in-eye
 
GROOS
 
HER-kyou-leez
 
hor-uh-LOW-gee-um
 
HY-druh
 
HY-drus
 
IN-dus
 
la-SIR-ta
 
LEE-oh
 
LEE-oh MY-ner
 
LEE-puss
 
LEE-bra
 
LOUP-us
 
links
 
LIE-rah
 
MEN-sa
 
MY-krow-SKOH-pee-em
 
mon-OSS-er-us
 
MUSS-ka
 
NOR-ma
 
OCK-tens
 
Oaf-ih-YOU-kus
 
oh-RYE-un
 
PAY-vo
 
PEG-uh-suss
 
PURR-see-us
 
FEE-nix
 
PICK-tor
 
PIE-sees
 
PIE-sees oss-TREE-nus
 
PUP-iss
 
PICK-sis
 
reh-TICK-yuh-lum
 
suh-JIT-uh
 
sa-jih-TARE-ee-us
 
SKOR-pee-uss
 
SKULP-tor
 
SCOOT-um
 
SIR-pens CAP-ut
 
SIR-pens KAW-dah
 
SEX-tens
 
TOR-us
 
tell-es-SCOPE-ee-um
 
tri-ANG-yuh-lum
 
tri-ANG-yuh-lum aus-TRAY-lee
 
too-KAY-nah
 
URR-sah MAY-jer
 
URR-sah MY-ner
 
VEE-la
 
VER-go
 
VO-lans
 
vul-PECK-yoo-la

Planets & Moons

 
 
Name
Pronunciation
 
ah-DRAHS-tee-ah
 
et-NEE
 
ah-mal-THEE-ah
 
a-NAN-kee
 
AIR-ee-el
 
AT-lus
 
aw-TON-oe-ee
 
be-LIN-dah
 
bee-AHNK-uh
 
KAL-e-ban
 
ka-LIRR-o-ee
 
ka-LIS-toe
 
ka-LIP-soe
 
KAR-mee
 
kal-DEE-nee
 
CARE-en
 
core-DEAL-ya
 
KRESS-e-da
 
DYE-mos
 
DES-de-MOAN-a
 
de-SPEEN-a
 
dye-ON-ee
 
URTH
 
EE-lahr-ah
 
en-SELL-ah-dus
 
EPP-e-ME-thee-us
 
err-IN-o-mee
 
EE-ris
 
ewe-AN-thee
 
ewe-POUR-ee-e
 
you-ROE-pah
 
ewe-RID-o-mee
 
GAB-ree-ell
 
GAL-aTEA-a
 
GAN-eh-meed
 
har-PAL-e-kee
 
he-LEAN
 
her-MIP-ee
 
HIM-ah-lee-ah
 
hye-PER-ee-on
 
ee-AHP-eh-tus
Io
 
EYE-oh
 
EYE-o-KAS-tee
 
eye-SON-oe-ee
 
JAY-nus
 
JEW-lee-ette
 
JEW-pi-ter
 
KAY-lee
 
KAL-e-kee
 
la-RISS-a
 
LEE-dah
 
lis-ih-THEE-ah
 
MARZ
 
MEG-a-KLYE-tee
 
MIRK-you-ree
 
MEE-tis
 
MYE-mus
 
mi-RAN-dah
 
moon
 
NYE-ad
 
NEP-toon
 
NAIR-ee-id
 
OH-ba-ron
 
oh-FEEL-ya
 
or-THOE-see-e
Pan
 
PAN
 
pan-DOOR-ah
 
pa-SIF-ah-ee
 
PAS-e-thee
 
FOE-bos
 
FEE-bee
 
PLOO-toe
 
POR-sha
 
prak-SID-e-kee
 
pro-MEE-thee-us
 
PRO-per-oe
 
PRO-tee-us
 
PUCK
 
KWA-oh-ar
 
REE-a
 
ROS-a-lind
 
SA-turn
 
SET-e-bus
 
se-NO-pee
 
SPON-dee
 
ste-FAA-noe
Sun
 
sun
 
SICK-o-RACKS
 
tay-IJ-e-tee
 
tah-LES-toe
 
TEE-this
 
tha-LASS-a
 
THEE-bee
 
the-MISS-toe
 
Thy-OE-nee
 
TYE-tun
 
tye-TAIN-ee-ah
 
TRING-kew-loe
 
TRY-ton
 
UM-bree-el
 
YOU-rah-nus
 
VEE-nus

Meteor Showers

 
 
Name
Pronunciation
 
AY-tah AK-wa-rids
 
GEM-e-nids
 
LEE-o-nids
 
LYE-rids
 
north TOR-ids
 
o-RYE-o-nids
 
PUR-see-ids
 
kwa-DRAN-tids
 
south DEL-tah AK-wa-rids
 
south TOR-ids

Stars

 
 
Name
Pronunciation
 
AH-kuh-mar
 
AK-er-nar
 
A--krucks
 
ACK-you-benz
 
ad-HAR-a
 
al-KAP-rah
 
all-NAYR
 
all-NEE-yaht
 
all-soo-HAIL
 
al-BAL-dah
 
al-BEE-ri-oh
 
al-CHIH-ba
 
AL-kor
 
all-SYE--o-nee
 
al-DEB-ah ran
 
al-DER-a-min
 
al-da_FER-a
 
All-firk
 
all-JED-ee
 
al-JEN-nib
 
al-GEE-bah
 
al-GEEB-bah
 
AL-gall
 
ALL-gor-ab
 
al-HAY-nah
 
AL-lee-oth
 
AL-kade
 
al-ka-LOOR-ops
 
ALL-maaz
 
ALL-mahk
 
all-NAH-zul
 
ALL-nil-ahm
 
ALL-nit-ahk
 
AL-fard
 
al-FECK-ah, JEM-a
 
AL-fer-rats
 
all-RAH-kiss
 
all-RESH-ah
 
all-SHAIN
 
AL-tair
 
ALL-tays
 
al-TARF
 
al-TERF
 
 
al-UDE-rah
 
a-LOOL-ah ow-STRAH-liss
 
a-LOOLah bor-ee-AH-liss
 
ALL-zirr
 
UNG-ka
 
ANG-kah
 
an-TAIR-ease
 
arc-TOUR-russ
 
AR-kub
 
AR-kub
 
AR-kub PREE-or
 
AHR-neb
 
ah-SELL-a
 
ah-SELL-us ow-STRALICE
 
ah-SELL-us bore-ee-AL-is
 
ah-SELL-us
 
ah-SELL-us
 
ah-SELL-us
 
ass-mid-ISS-kee
 
ass-pid-ISS-kee
 
AH-tik
 
AT-las
 
AH-tree-a
 
 
AV-i-or
 
AH-za
 
ba-HAHM
 
BARN-ards star
 
BUT-en KYE-tos
 
BYED
 
BEL-la-trix
 
BET-el-jooz
 
boh-TAYN
 
can-OH-pus
 
kah-PELL-ah
 
KAF
 
CASS-ter
 
SEB-all-rye
 
ke-LAY-no
 
CHAH-ra
 
KERT-ahn,
 
core-ca-ROLE-ee
 
COOR-sah
 
DAH-bee
 
DEN-ebb
 
DEN-ebb al-JEE-dee
 
DEN-ebb
 
DEN-ebb
 
DEN-ebb KAY-tos
 
de-NEB-oh-la
 
DYE-a-dem
 
JOOB-a
 
DOOB-huh
 
ED-a-sick
 
e-LEK-tra
 
EL-noth
 
EL-ta-nin
 
EEN-if
 
er-RYE
 
e-RAHK-is (mu Draconis)
 
FO-mal-oh
 
fur-ROOD
 
GAK-kruks
 
JAW-sahr
 
JEEN-ah
 
GIRR-tahb
 
go-MAY-sah
 
GRAH-fi-us
 
GROOM-bridge
 
"
 
GROO-mi-um
 
HAH-dahr
 
HAM-al
Han
 
HAN
 
 
 
HEE-dus
 
HEE-dus
 
HOH-mahm
 
EYE-zar
 
JAB-bah
 
KAFF-al-JID-mah
 
KOWSS ow-STRAH-liss
 
KOWSS bor-ee-AH-liss
 
KOWSS me-RID-i-an-AL-is
 
KYED
 
kit-AL-fa
 
KOE-cab
 
core-ne-FOR-uss
 
 
KOOR-hah
 
la su-PURR-ba
 
la-KA-ya
 
la-KA-ya
 
la-LAHND
 
LAY-soth
 
MAH-ya
 
MAR-fick
 
MAR-kab
 
MAH-tahr
 
meb-SOO-tah
 
meg-REZ
 
MAY-sah
 
mek-BOO-dah
 
men-KAH-li-nan
 
men-KAHR
 
men-KENT
 
men-KIB
 
MER-ak
 
MER-o-pee
 
mess-AHR-tim
 
mee--a-PLASS-id-uss
 
mim-OH-sah, BAY-cruks
 
MIN-kar
 
MIN-ta-ka
 
MEE-ra
 
MIRR-ahk
 
MERE-fak
 
MERE-zam
 
MYE-zahr
 
MOOL-if-ayn
 
MOO-frid
 
MUSS-id-a
 
nar-AL-safe
 
NOWSS
 
nah-SHE-rah
 
NECK-ahr
 
nih-HALL
 
NOH-dus
 
NUN-kee
 
noo-SAH-kahn
 
Oaf-ih-YOU-kus
 
FEYE-et
 
FEK-da
 
ferk-AHD
 
PLAY-o-nee
 
poe-LAIR-is
 
POL-lucks
 
pour-EE-mah
 
PRO-see-on
 
PRO-puss, TAY-zhaht PRYE-or
 
RAH-sa-luss
 
rah-sell-GAYTH-ee
 
RAHS-al-haig
 
RAHS-al-MOTH-al-ah
 
REG-you-luss
 
RYE-jel
 
RYE-jel ken-TAW-russ
 
ROH-ta-nev
 
ROOK-baht
 
ROOK-baht
 
SAH-bik
 
sah-DUCK-be-ah
 
sah-dul-BAH-ree
 
sah-dul-MEL-ik
 
sah-dul-su-OOD
 
SADE-der
 
SAFE
 
SAHR-goss
 
SAHR-in
 
SHEE-at
 
SHED-er
 
SEG-in
 
seg-EEN-us
 
SHOWL-a
 
SHEL-ee-yak
 
SHARE-ah-tan
 
SEER-ee-us
 
SKAHT
 
SPEE-ka
 
STER-o-pee
 
swah-LOH-sin
 
soo-HALE-al-MOO-liff
 
SOOL-a-faht
 
SIRM-a
 
TAH-lith-a
 
THA-ni-ya ow-STRAH-liss
 
THA-ni-ya bor-ee-AH-liss
 
TAHR-ah-zed
 
TAY-get-a
 
teg-MEEN-e
 
TAY-zhaht pos-TER-i-o
 
THOO-bahn
 
tra-PEEZ-i-um
 
tra-PEEZ-i-um
 
tra-PEEZ-i-um
 
tra-PEEZ-i-um
 
uh-NOO-kul-lye
 
VEY-ga
 
vin-de-mee-AY-tricks
 
wah-SAHT
 
WUZ-un
Wei
 
 
WEZ-en
 
YED pos-TER-i-or
 
YED PRYE-or
 
zah-NYE-a
 
ZAW-rahk
 
zah-vee-JAH-vah
 
ZOSS-mah
 
zoo-BEN-el-AK-rab
 
zoo-BEN-el-je-NEW-bee
 
zoo-BEN-esh-ah-MAL-ee

If you'd like to follow along with NASA's New Horizons Mission to Pluto and the Kuiper Belt, please download our FREE Pluto Safari app.  It is available for iOS and Android mobile devices. Simulate the July 14, 2015 flyby of Pluto, get regular mission news updates, and learn the history of Pluto.

Simulation Curriculum is the leader in space science curriculum solutions and the makers of Starry Night, SkySafari and Pluto Safari. Follow the mission to Pluto with us on Twitter @SkySafariAstro, Facebook and Instagram

The Lure of Variable Stars

I’m a sucker for action. I love change. My favorite planet is Jupiter because of its rapid rotation, ever-changing moons, and volatile cloud features. I love watching Near Earth Asteroids and comets as they move across star fields. Recently I’ve become addicted to watching solar flares and prominences in rapid action with my solar telescope. But most of all, I love to observe variable stars.

All stars vary in brightness to some degree. Even our Sun, which seems so stable, changes its brightness as more or less of its surface is obscured by sunspots. But there are stars in the sky that undergo vast changes in brightness and color. Many are highly unpredictable in their behavior, and need years of study to uncover the mechanisms that drive them.

The Variable Zoo

The most famous are the novas and supernovas which suddenly shoot up from obscurity to prominence. Supernovas are relatively rare in our neighborhood. The last one was over 400 years ago in 1604. Novas are more common, several being observable in any given year.

Some stars appear to vary for purely mechanical reasons. These are called eclipsing binaries: two stars in a close orbit where one star eclipses the other, as regular as clockwork. Algol in the constellation of Perseus is a famous example of an eclipsing binary.

Other stars expand and contract slowly because of processes going on within them. The most common of these “pulsating variables” are long period variable stars like Mira in the constellation Cetus. Mira is larger in diameter than the orbit of Mars, and changes size, brightness, and color over a period of just under a year. It ranges over nearly six magnitudes in brightness, meaning that at its brightest, it is a hundred times brighter than when it’s at its dimmest. Another group of pulsating variables is called the Cepheids, named after the star Delta Cephei. These have much shorter periods than the Miras, ranging from 1 to 70 days, and their period is closely tied to their luminosity, which has led to their use as measuring sticks to determine the distance of globular clusters and galaxies.

Another group of variable stars is called “cataclysmic variables.” These include novas, supernovas, and the so-called “dwarf novas.” These last are the stars that interest me the most because they show the most action. My favorite is SS Cygni (TCY 3196-723-1), located close to the open cluster Messier 39. This star normally sits around twelfth magnitude, just visible in a small telescope, but every few weeks it shoots up unpredictably to about eighth magnitude. If you’re lucky enough to catch it in outburst, you can actually see it get visibly brighter. Stars like SS Cygni are actually close double stars consisting of a red dwarf and a white dwarf. The white dwarf is surrounded by a disk of gas stolen from the red dwarf which is drawn down into the white dwarf where it ignites, causing the sudden outburst in brightness.

 

Observing Variable Stars

Professional astronomers realized over a century ago that there were more variable stars in need of study than they could handle, so they enlisted the aid of amateur astronomers to monitor the brightness of a number of stars well suited to amateur observation: stars which changed in magnitude over a wide range and which took a long period to complete their cycle of brightness. For many years this work required no more than a telescope and a good set of charts, and such simple visual observations are still useful today, although nowadays amateurs have access to photoelectric photometers and CCD cameras which are capable of studying just about any star. The American Association of Variable Star Observers acts as a central clearing house for all sorts of amateur variable star observations, providing instruction, charts, and other support, and giving amateurs a simple online system for recording their observations.

Why observe variable stars? Mainly because it’s fun! You never know from night to night what you are going to find…remember what I said about action? No special equipment is needed other than a set of star charts which plot the variable star and give the brightness of non-variable stars around it, which are used to estimate the brightness of the variable.

If you are a deep sky observer, you already have one of essential skills of a variable star observer: you know how to locate objects in the sky. It doesn’t matter how you do it. I used traditional starhopping for several years, but now I use my Orion SkyQuest XT6’s IntelliScope setting circles to locate my variables. Once you’ve located the variable, you estimate its brightness as compared to other stars on the chart, and record the time of the observation. With a little practice you can make estimates to within a tenth of a magnitude. You can then log onto the AAVSO’s web site and enter your observation. Within ten minutes it will be moved into their database of over ten million observations, and you can see your observation on a light curve along with those of hundreds of other observers around the world. What could be neater?!

Unlike most of the observations amateur astronomers make, variable star observations have a serious side. By making a numerical estimate of the brightness of a star at a particular point in time, you are logging a piece of scientific data. The AAVSO maintains records online of every observation submitted to them over the past hundred years, keeping the records available to researchers around the world.

On a typical night, I’ll observe about a dozen stars from “my” list of about sixty stars visible at different times of year.

I keep finder charts along with the AAVSO charts in plastic sleeves in a loose-leaf binder, so that everything I need is close at hand. Since you never know ahead of time how bright a variable is going to be, you need to have a complete set of charts for each star; these can be downloaded from the AAVSO web site:

The biggest challenge in finding a variable star is that you’re looking for something that may be quite bright, or may be below the magnitude limit of your telescope, totally invisible to you. So what you look for is the star field, the pattern of stars surrounding the variable. Once you’ve found the field, you then check to see how bright the variable is. You then consult your AAVSO charts to see which stars are closest in brightness to the variable. Comparison stars on the charts are marked with their brightness to the nearest tenth of a magnitude. Because a decimal point might be confused with a faint star, they are left out, so that a 9.7 magnitude star is marked “97” and a 11.4 is marked “114” on the chart. You try to find a couple of stars, one slightly brighter than the variable, one slightly fainter, and then estimate where the variable falls between them.

Equipment for variable star observing

For visual observing as I have described above, the equipment needs are very simple. There are many variable stars within range of a pair of small binoculars, and some that can be observed with the naked eye alone. On the other hand, access to a large telescope lets you follow stars that become very faint at minimum.

I have found it advantageous to use eyepieces with a wide field of view, since they show me more of the sky at any given magnification, and let me see more comparison stars without having to move the telescope about.

My current strategy is to survey “my” variables using my Celestron 6" SCT telescope. I’ve programmed the controller with the coordinates of my variables, so I can quickly move through the list. Any variables which are currently too faint to be observable with the 6”, I revisit the next night with my larger 11” Dobsonian.

Where to start?

If you’re still not sure whether variable star observing is for you, I’d recommend reading Starlight Nights by Leslie Peltier (Sky Publishing). Peltier was the finest variable star observer of the 20th century, and his book is an entertaining introduction to a wonderful man and his love of the stars. It’s probably my very favorite astronomy book.

The AAVSO web site includes everything you need to get started. It has a complete observing manual, a list of good stars to start on, and all the charts you will need, all free of charge. Visit http://www.aavso.org

I’d recommend starting on stars that are easy to find and visible all year round, such as these stars in and around the Big Dipper:

A final warning though: variable star observing is highly addictive. Variable star observers probably spend more time at the eyepiece than any other amateur astronomers because, unlike deep sky or planetary observing, they are not dependent on dark skies or steady seeing. For years I carried out regular variable star observing every clear night from the middle of a large city, even when the Moon was full. The only thing that can stop you is clouds!


If you'd like to follow along with NASA's New Horizons Mission to Pluto and the Kuiper Belt, please download our FREE Pluto Safari app.  It is available for iOS and Android mobile devices. Simulate the July 14, 2015 flyby of Pluto, get regular mission news updates, and learn the history of Pluto.

Simulation Curriculum is the leader in space science curriculum solutions and the makers of Starry Night, SkySafari and Pluto Safari. Follow the mission to Pluto with us on Twitter @SkySafariAstro, Facebook and Instagram

Saturn Through the Ages

On May 23rd, Saturn will reach opposition — the closest it will be to Earth in 2015.

Saturn, the original Load of the Rings.

Saturn can be viewed in the morning sky until May 23, when it moves into the evening sky. From November to the end of the year it will be behind the Sun.

Looking south-east on May 23, 2015 at 11:00 p.m. from mid-northern latitudes.

The rings are now widely open, making them easy to see in any telescope magnifying more than about 30x. Saturn’s largest moon Titan is readily visible in a small telescope, and several more moons may be seen in larger telescopes. At opposition, the planet’s equatorial angular diameter will be 19 arc seconds, its rings being 42 arc seconds across.

As you peer through your eyepiece and ponder the ringed planet with the benefit of our modern understanding of science, consider how perplexing Saturn must have been to ancient people whose instruments and grasp of nature were at their infancy.

Eyepiece view (10 arc minutes) of Saturn on May 23, 2015.  The planet’s equatorial angular diameter will be 19 arc seconds, its rings being 42 arc seconds across.

In our feature article below, “Saturn Through the Ages” — a departure from our usual technical take on the universe — we will be returning to times past to explore a piece of the puzzle that highlights our search for knowledge and meaning.

Saturn Through the Ages  

Throughout human history, we have looked to the light of the heavens to illuminate our role on Earth. Next time you are star gazing, consider all of the people throughout time and across the world who have reflected upon the same celestial bodies, conducting their nightly dance across our sky.

Our study of the celestial sphere has brought us understanding of physical and mathematical principles, models for society and perhaps fundamentally, a comforting sense of order. It is the human imagination however, and our quest to find a meaning behind this order, that led us to create a screenplay of the night sky. For millennia we have told our own tale through the guise of a heavenly cast of characters. Because celestial mythology is common throughout many cultures, these stories reveal our discoveries of the human condition.

In the upcoming month, many of us will be gazing at the planet Saturn in the northeastern sky. Perhaps due to a planet’s slow trek through our heavens, the stories we've told about Saturn often involve the passage of time and inevitable fate. We've expressed through Saturn both our appreciation for life and our fear of time's cruel and inescapable quality.

In ancient Mesopotamia, they prayed to Saturn as the Lord of Death, appealing to him thus:

“O Lord Saturn
whose name is august
whose power is widespread
whose spirit is sublime
O Lord Saturn
the cold, the dry, the dark, the harmful…
crafty sire who knowest all wiles
who are deceitful, sage and understanding
who causest prosperity and ruin
happy or unhappy is he whom thou makest such.”

In ancient Rome, Saturn was an agricultural god, a harvest deity. Controlling our fate through the success of our crop, he was celebrated in times of bounty and appealed to when times were hard. The Golden Age of Saturn, an ideal era of equality and abundance, was memorialized during the mid-winter festival of Saturnalia. A time of feasts and gifts from which we can trace rituals of modern day Christmas. During the celebration, a man chosen to represent the god was attentively fêted, only to be sacrificed on the final day of the festival. Try as we have to sway him however, we are all equally powerless before the forces personified by Saturn. 

In Hindu mythology, Saturn appears as the god Sani, holder of the secrets of fate. One could predict the future through use of a Saturn diagram, which represents the planet’s path through our skies. This god is so malevolent that a single glance from the evil-eyed deity burned off the head of the infant Ganesa, god of good fortune and prosperity. Associated with childhood disease, Sani demonstrates that not even a god’s luck can stand against the inevitability that Saturn represents.

Though we may wish it otherwise, nothing in our human existence remains static; nothing escapes the passage of time. Falcon-headed Horus, Saturnine god of the ancient Egyptians, succeeded his father Osiris when he was dethroned, marking the beginning of a new regime. As all change implies death of the old, we tell our tales of Saturn to reconcile ourselves to the necessity of welcoming the new. 

Cronos, Saturn-god of ancient Greece, whose name may originally have referred to his universal governance (from the verb kreno), became known as Father Time. Cronos not only overthrew and replaced his father, but consumed each of his own children at birth, much as time itself consumes all that it creates. Demonstrating the universality of this principle, Cronos himself was ultimately dethroned by his offspring, making way for a new era.

Through our creation of Saturn mythology, we attempt to explain our relationship to fate, time and death. Our ability to perceive these issues is fundamental to our very humanity. When next gazing at Saturn in the night sky, perhaps you will see not only a wonder of the cosmos, but also the history of humanity’s struggle to find meaning therein.


If you'd like to follow along with NASA's New Horizons Mission to Pluto and the Kuiper Belt, please download our FREE Pluto Safari app.  It is available for iOS and Android mobile devices. Simulate the July 14, 2015 flyby of Pluto, get regular mission news updates, and learn the history of Pluto.

Simulation Curriculum is the leader in space science curriculum solutions and the makers of Starry Night, SkySafari and Pluto Safari. Follow the mission to Pluto with us on Twitter @SkySafariAstro, Facebook and Instagram

Sky Events For May 2015

Moon Phases

Full Moon

Sunday, May 3, 11:42 p.m. EDT

The Full Moon of May is known as the Milk Moon,” “Flower Moon,”  or Corn Planting Moon.It rises around sunset and sets around sunrise; this is the only night in the month when the Moon is in the sky all night long. The rest of the month, the Moon spends at least some time in the daytime sky.

Last Quarter Moon

Monday, May 11, 6:36 a.m. EDT

The Last Quarter Moon rises around 2 a.m. and sets around 1 p.m. It is most easily seen just after sunrise in the southern sky.

New Moon

Sunday, May 18, 12:13 a.m. EDT

The Moon is not visible on the date of New Moon because it is too close to the Sun, but can be seen low in the East as a narrow crescent a morning or two before, just before sunrise. It is visible low in the West an evening or two after New Moon.

First Quarter Moon

Monday, May 25, 1:19 p.m. EDT

The First Quarter Moon rises around 1 p.m. and sets around 2:15 a.m. It dominates the evening sky.

Observing Highlights

Mercury at greatest elongation

Thursday, May 7, evening twilight

This is the best evening apparition of Mercury this year for observers in the northern hemisphere. Use Venus to help you locate it. Mercury is most easily located by sweeping with binoculars, but once youve located it, you should be able to see it with your unaided eyes

Uranus and the Moon

Friday, May 15, dawn

The Moon will pass just south of the Uranus just before sunrise.

Double shadow transit on Jupiter

Wednesday, May 20, 8:068:35 p.m. EDT

The shadows of Io and Ganymede will be on opposite limbs of Jupiter, while the moons Io and Callisto will be central on the disk.

Saturn at opposition

Friday, May 22, 10 p.m. EDT

Saturn will be in opposition to the Sun.

Note how most of Saturns moons are in the same plane as the rings, except for Iapetus, whose orbit is tilted 8.3 degrees. At opposition, Iapetus is close to maximum elongation towards the west, while Tycho is close to maximum elongation towards the east.

Double shadow transit on Jupiter

Wednesday, May 27, 10:01 p.m.12:18 a.m. EDT

The shadow of Io chases the shadow of Ganymede across the face of Jupiter, catching up with it and passing it at 11:48 p.m. EDT. The Great Red Spot will also cross Jupiters disk during this period.

Planets

 Mercury is well placed for northern hemisphere observers in the evening twilight sky for the first three weeks of May.

Venus shines high in the western sky after sunset.

Mars moves from Aries to Taurus on May 3, too close to the Sun to be visible.

Jupiter is well placed in the evening sky all month.

Saturn is just north of Scorpius’ “claws.At opposition on May 22, it is visible all night.

Uranus rises just before the Sun in Pisces.

Neptune is in the eastern morning sky in the constellation Aquarius.


If you'd like to follow along with NASA's New Horizons Mission to Pluto and the Kuiper Belt, please download our FREE Pluto Safari app.  It is available for iOS and Android mobile devices. Simulate the July 14, 2015 flyby of Pluto, get regular mission news updates, and learn the history of Pluto.

Simulation Curriculum is the leader in space science curriculum solutions and the makers of Starry Night, SkySafari and Pluto Safari. Follow the mission to Pluto with us on Twitter @SkySafariAstro, Facebook and Instagram

Pluto Is A Planet, And So Is Eris

Is Pluto a planet?  What is a planet, anyhow?  We hope you’ll agree that the IAU's current answers to these questions are unclear and confusing.  Here, we propose clear and unambiguous answers to these fundamentally unclear problems.  Above all, we hope you have fun with the debate, no matter what side of it your heart may lay on.

The Planet Definition Mess

 As astronomers began to discover objects similar in size to Pluto, culminating with the discovery of Eris in 2005, it quickly became clear that if Pluto was a planet, so should Eris.  And if Eris was a planet why not some of the other newly discovered  objects. Our solar system might have dozens of planets.  One camp felt that a line needed to be drawn somewhere, and another camp felt that the newly discovered objects should be added to the list of solar system planets.

 

Illustration of the relative sizes, albedos, and colours of the largest trans-Neptunian objects.

Illustration of the relative sizes, albedos, and colours of the largest trans-Neptunian objects.

In 2006 the International Astronomical Union (IAU) met with the intention of solving the debate once and for all.  The goal was to come up with a definition for “planet”, which had never been done before.  After many days of contentious debate, the IAU passed the following resolution:

RESOLUTION 5A

The IAU therefore resolves that planets and other bodies in our Solar System, except satellites, be defined into three distinct categories in the following way:

(1) A "planet" is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighbourhood around its orbit.

(2) A "dwarf planet" is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape [2], (c) has not cleared the neighbourhood around its orbit, and 

(d) is not a satellite.

(3) All other objects, except satellites, orbiting the Sun shall be referred to collectively as "Small Solar-System Bodies".

This is a poor definition that has only served to add more confusion.  With resolution 2c,  “has cleared the neighborhood around its orbit”, the IAU is trying to express that a planet should be the dominant gravitational force in its local region of the solar system.  That's not an unreasonable position.  Certainly the Earth and Jupiter are the dominant objects in their local regions.  But have any of these planets actually "cleared the neighborhood" around their orbits?  No.  Pluto is still clearly in Neptune's "neighborhood".  For that matter, Jupiter has two well-known groups of asteroids, the "Trojans", which lead and follow Jupiter along in its orbit.  For that matter, the Earth hasn't quite "cleared the neighborhood" around its orbit, either, as anyone who was near Chebalyink, Russia on Feb 15th, 2013 or Tunguska, Siberia on June 30th, 1908 can attest to.  So are Earth, Jupiter, and Neptune the dominant gravitational objects in their local neighborhoods?  Yes.  Have they "cleared their neighborhoods"?  No.

The Thousand Kilometer Rule

 Here is what the IAU should have resolved in 2006:

 (1) A "planet" [1] is a celestial body that (a) is in orbit around the Sun, (b) has a maximum surface radius greater than 1000 kilometers.

 (2) All other objects orbiting the Sun shall be referred to collectively as "Small Solar-System Bodies".

 "But that's completely unscientific" you say. "Why 1000 kilometers?  Why not 1200, or 750?"  I submit to you that the precise definition of a planet as an object at least 1000 kilometers in radius is no less "scientific" than the definition of a "kilometer" as being a unit of distance equal to 1000 meters, or a "degree" being 1/360th of a circle.

 Here is a list of the largest known objects orbiting the Sun, and their radii in kilometers:

Jupiter - 69,911
Saturn - 58,232
Uranus - 25,362
Neptune - 24,622
Earth - 6,378
Venus - 6,052
Mars - 3,390
Mercury - 2,440
Pluto - 1,184
Eris - 1,163
Makemake - 715
Haumea - 620
Quaoar - 555
Sedna - 498
Ceres - 475
Orcus - 458

By the 1000-kilometer definition, all eight classical planets would remain planets.  As would Pluto, and we add Eris.  The solar system would have exactly ten planets. Those fond of keeping Pluto's planetary status for historical reasons would retain its dignity.  And elevating Eris to a first-class planet would be an honorable nod to the cutting-edge astronomers whose work led to a need for this new definition in the first place.

And as to the "cleared the neighborhood" part of the definition?  This it the most unclear and least popular part o the IAU's 2006 definition.  It's best dealt with by being eliminated entirely.  The end game is to define the term "planet" in a manner that's simple, understandable, and satisfying.  The 1000-kilometer rule does this aptly.


If you'd like to follow along with NASA's New Horizons Mission to Pluto and the Kuiper Belt, please download our FREE Pluto Safari app.  It is available for iOS and Android mobile devices. Simulate the July 14, 2015 flyby of Pluto, get regular mission news updates, and learn the history of Pluto.

Simulation Curriculum is the leader in space science curriculum solutions and the makers of Starry Night, SkySafari and Pluto Safari. Follow the mission to Pluto with us on Twitter @SkySafariAstro, Facebook and Instagram


Mercury at its Best

Now that Pluto has been demoted to a dwarf planet, Mercury is the smallest of the eight planets. With a diameter of 3032 miles (4879 km.), it is slightly more than a third of the diameter of Earth, and smaller than the solar system’s two largest moons, Ganymede and Titan. Because of its tight orbit around the sun, Mercury never strays far into the night sky, peeping tantalizingly over the horizon a few times a year. The next two weeks will be your best chance for seeing Mercury in evening twilight this year.

Timing is the secret for catching sight of Mercury. Try too early, and its tiny speck of light will be lost against the twilight sky. Try too late, and Mercury will be too close to the horizon. Ive found the best time to be about half an hour after sunset. Binoculars are helpful in initially spotting Mercury, but once located in binoculars you should be able to see it with the unaided eye.

Currently Venus is shining brightly in the evening sky, and it can be a helpful guide to spotting Mercury, about two-thirds of the way down towards the horizon, and slightly to your right. Dont confuse it with nearby Aldebaran, which will have a noticeably reddish color and will probably twinkle, while Mercury shines with a more steady light.

On the evening of Thursday, May 7, Mercury will be at its farthest from the Sun, making the next two weeks the best time this year for observers in the northern hemisphere to spot this elusive little planet. Credit: Starry Night software.

On the evening of Thursday, May 7, Mercury will be at its farthest from the Sun, making the next two weeks the best time this year for observers in the northern hemisphere to spot this elusive little planet. Credit: Starry Night software.

In a telescope, Mercury is a disappointing sight. Like Venus, Mercury exhibits phases as it passes between us and the sun. At present it is slightly gibbous. On Saturday, May 2, it will look just like a miniature first quarter moon. After that, it will assume a crescent shape.

Because Mercury is always seen close to the horizon, it is a challenge to see its surface markings, even in a powerful telescope. Serious observers of Mercury prefer to observe it in the daytime sky, now relatively easy to do because of computerized telescopes. But always be very careful when observing with the sun above the horizon, because even the briefest view of the sun in a telescope will do permanent harm to your eyes.


If you'd like to follow along with NASA's New Horizons Mission to Pluto and the Kuiper Belt, please download our FREE Pluto Safari app.  It is available for iOS and Android mobile devices. Simulate the July 14, 2015 flyby of Pluto, get regular mission news updates, and learn the history of Pluto.

Simulation Curriculum is the leader in space science curriculum solutions and the makers of Starry Night, SkySafari and Pluto Safari. Follow the mission to Pluto with us on Twitter @SkySafariAstro, Facebook and Instagram

Starry Night 7, eclipses and ... Elmo

Like most two years olds, my daughter loves Elmo. Something about his high-pitched voice and ever-present smile I guess.

Parents innately learn to tune him out, probably to moderate the risk of going insane listening to that same shrill voice on reruns day after day.

One episode that sticks out in my mind, today more than ever perhaps, puts Elmo in a room with none other than David Beckham. The short ends after Elmo, who pesters Becks to teach him to dribble a soccer ball on his head, learns a new word... Persistence.

Persistence is an extremely important quality, and some might say a disappearing quality these days. It goes hand-in-hand with patience I think, something we can all agree is becoming scarce in this age of on-demand everything.

Persistence, as in the case of Elmo and Becks, often pays off.

Over the past few weeks, I've been involved in an exchange over the accuracy of Starry Night's eclipse predictions. One of our "power users" (who shall remain nameless for now) reported what he believed to be an issue with our calculations. They just didn't match up exactly with what NASA (and other government sites) were reporting.

The discrepancy was small; in fact, the timings were exact, to the sub-second but the sizes of the Earth's shadows (both the umbra and penumbra) were too small by a very small but noticeable fraction.

Normally no-one would even notice this, but in this case it changed our prediction for the April 4th, 2015 eclipse from a Total (as reported by NASA) to a Partial eclipse. That made all the difference to a few people.

I sit down at my 'puter. "I'll figure this out", I say to myself confidently:

  • Were we perhaps using an old or imprecise value for the Earth's diameter? Nope. That was in agreement with the USGS.
  • Were we taking the oblateness of the Earth into account? Yup. A precise calculation there too.
  • Was this somehow rounding or another error in calculation? Nope. Everything seems to check out.

After a few hours of this, I checked with my confrere, Bill (our SkySafari developer) to see if they had the same discord with NASA predictions. They did! And even better (worse, it turns out) both Starry Night, and SkySafari, two completely independently created applications, gave almost exactly the same result!

That sealed it for me. Other matters were more pressing. NASA could be wrong too (note that it's not insane to believe this, the pages we were referring to were intended for the public, maintained by a summer student and weren't necessarily vetted by anyone), or could have used slightly different values for the radius of the Earth. Were THEY accounting for the oblateness? Doubts and lack of information made it difficult.

After presenting my findings to Keiron, our head of support, I let the issue go.

Lots of other stuff to work on.

Again, the power user, and Keiron came back to me. Why were our predictions different? We claim arcsecond precision in our planet and moon positions. How could we make that claim if this discrepancy existed?

Again, I chatted with Bill. He said he had been talking with Keiron too. I Don't know what this annoying user thinks he knows that we don't. What could it be? "The Earth's atmosphere?" Says Bill. I dunno. Does NASA take it into account? It's not clear from their site. How can we compare if they don't say? The discrepancy is so small.

Lots of other stuff to work on.

Again, an email from Keiron. "Aren't you busy?" I think to myself. I open it, a curt reply, ready at my fingertips. This time, the message comes with a link.

"Do you think the Danjon rule explains the difference?" he asks:

http://www.eclipsewise.com/oh/oh-help/LEshadow.html

...

Holy s*&t!

...

Not just a clear explanation of what, how, and by how much the Earth's atmosphere contributes to the shadow, but authored by Fred Espenak himself, The Godfather of eclipse predictions! 

This page on the eclipse, with nicely outlined parameters showed something called "Shadow Enlargement":

http://www.eclipsewise.com/lunar/LEprime/2001-2100/LE2015Apr04Tprime.html

... with a link to a clear explanation of what the Danjon shadow rule is, and its value.

It turns out that the Earth's atmosphere contributes around 1/85 (just over 1%) to the diameter of the Earth's shadow... an effect that we were NOT taking into account in Starry Night or SkySafari... but are now! (SN version 7.1.2+, SkySafari ).

Starry Night has been around for almost 20 years in some form or another, and we have never taken this into account, until now.

We could all learn a little from this power user and Keiron (and Elmo for that matter). It pays to be persistent! 

Thanks for keeping at it guys. Starry Night is that much better for it.

After a few hours of this, I checked with my confrere, Bill (our SkySafari developer) to see if they had the same discord with NASA predictions. They did! And even better (worse, it turns out) both Starry Night, and SkySafari, two completely independently created applications, gave almost exactly the same result!

That sealed it for me. Other matters were more pressing. NASA could be wrong too (note that it's not insane to believe this, the pages we were referring to were intended for the public, maintained by a summer student and weren't necessarily vetted by anyone), or could have used slightly different values for the radius of the Earth. Were THEY accounting for the oblateness? Doubts and lack of information made it difficult.

After presenting my findings to Keiron, our head of support, I let the issue go.

Lots of other stuff to work on.

Again, the power user, and Keiron came back to me. Why were our predictions different? We claim arcsecond precision in our planet and moon positions. How could we make that claim if this discrepancy existed?

Again, I chatted with Bill. He said he had been talking with Keiron too. I Don't know what this annoying user thinks he knows that we don't. What could it be? "The Earth's atmosphere?" Says Bill. I dunno. Does NASA take it into account? It's not clear from their site. How can we compare if they don't say? The discrepancy is so small.

Lots of other stuff to work on.

Again, an email from Keiron. "Aren't you busy?" I think to myself. I open it, a curt reply, ready at my fingertips. This time, the message comes with a link.

"Do you think the Danjon rule explains the difference?" he asks:

http://www.eclipsewise.com/oh/oh-help/LEshadow.html

...

Holy s*&t!

...

Not just a clear explanation of what, how, and by how much the Earth's atmosphere contributes to the shadow, but authored by Fred Espenak himself, The Godfather of eclipse predictions! 

This page on the eclipse, with nicely outlined parameters showed something called "Shadow Enlargement":

http://www.eclipsewise.com/lunar/LEprime/2001-2100/LE2015Apr04Tprime.html

... with a link to a clear explanation of what the Danjon shadow rule is, and its value.

It turns out that the Earth's atmosphere contributes around 1/85 (just over 1%) to the diameter of the Earth's shadow... an effect that we were NOT taking into account in Starry Night or SkySafari... but are now! (SN version 7.1.2+, SkySafari ).

Starry Night has been around for almost 20 years in some form or another, and we have never taken this into account, until now.

We could all learn a little from this power user and Keiron (and Elmo for that matter). It pays to be persistent! 

Thanks for keeping at it guys. Starry Night is that much better for it.

Again, I chatted with Bill. He said he had been talking with Keiron too. I Don't know what this annoying user thinks he knows that we don't. What could it be? "The Earth's atmosphere?" Says Bill. I dunno. Does NASA take it into account? It's not clear from their site. How can we compare if they don't say? The discrepancy is so small.

Lots of other stuff to work on.

Again, an email from Keiron. "Aren't you busy?" I think to myself. I open it, a curt reply, ready at my fingertips. This time, the message comes with a link.

"Do you think the Danjon rule explains the difference?" he asks:

http://www.eclipsewise.com/oh/oh-help/LEshadow.html

...

Holy s*&t!

...

Not just a clear explanation of what, how, and by how much the Earth's atmosphere contributes to the shadow, but authored by Fred Espenak himself, The Godfather of eclipse predictions! 

This page on the eclipse, with nicely outlined parameters showed something called "Shadow Enlargement":

http://www.eclipsewise.com/lunar/LEprime/2001-2100/LE2015Apr04Tprime.html

... with a link to a clear explanation of what the Danjon shadow rule is, and its value.

It turns out that the Earth's atmosphere contributes around 1/85 (just over 1%) to the diameter of the Earth's shadow... an effect that we were NOT taking into account in Starry Night or SkySafari... but are now! (SN version 7.1.2+, SkySafari ).

Starry Night has been around for almost 20 years in some form or another, and we have never taken this into account, until now.

We could all learn a little from this power user and Keiron (and Elmo for that matter). It pays to be persistent! 

Thanks for keeping at it guys. Starry Night is that much better for it.

Partial solar eclipse on October 23rd

On the evening of October 23rd a partial solar eclipse takes place, ideally timed for North Americans to observe in the evening. The Moon's first contact with the Sun takes place at 4:25 PM CDT, and the moment of greatest eclipse is at 5:31 PM. These times are for an observer located in Minneapolis, MN; for other parts of the US, the times will vary slightly. Anyone wishing to view the eclipse should view it through special solar observing filters or by projecting the Sun's image. Don't ever stare directly at the Sun, even with sunglasses, and especially not through a telescope!

To simulate the partial solar eclipse in Starry Night 7 look in the Find Panel (the right sidebar) under "Today's Sky" and click on the listing for "Partial Solar Eclipse". Enjoy SN7!

Will you be viewing the partial solar eclipse today?

Double Stars around Boötes

On a May evening many years ago, I made my first exploration of the night sky. The only star pattern I could recognize was the Big Dipper, but with a star chart in a book, I used that to discover the bright star Arcturus in the constellation Boötes.

The curve of the Big Dipper's handle leads to Arcturus, the brightest star in the kite-shaped constellation of Boötes. Surrounding Boötes is an amazing variety of double stars. Credit: Starry Night software

The trick to learning the constellations is to begin with the stars you know, and use them to identify their neighbors. This same technique, known as "starhopping" is the key to discovering all the wonders hidden amongst the stars.

Start, as I did, with the Big Dipper, high overhead as the sky gets dark at this time of year. The stars that form the Dipper’s handle fall in a gentle arc, and if you project that arc away from the Dipper’s bowl, you come to a bright star. This is Arcturus, the third brightest star in the night sky, and the brightest star in the northern sky. Only Sirius and Canopus, far to the south, are brighter.

Arcturus is bright in our sky for two reasons, first because it is relatively close to us, 38 light years away, and secondly because it is inherently a bright star, much brighter than our Sun. Though larger and brighter, it is a slightly cooler star than our Sun, so appears orange to our eyes.

Although Boötes is supposed to be a ploughman in mythology, its pattern of stars most resembles a kite, with Arcturus marking the bottom of the kite where the tail attaches. Notice the little dots over the second "o" in Boötes: this indicates that the two "o"s are supposed to be pronounced separately, as "bow-oo’-tees," not "boo’-tees."

Once you have identified Boötes, you can use its stars to identify a number of constellations surrounding it. Between it and the Big Dipper are two small constellations, Canes Venatici (the hunting dogs) and Coma Berenices (Bernice's hair). To Boötes left (towards the eastern horizon) is the distinctive keystone of Hercules. Between Hercules and Boötes is Corona Borealis (the northern crown) with Serpens Caput, the head of the serpent, poking up from the south.

Although most stars appear to our unaided eyes as single points of light, anyone with access to binoculars or a telescope soon discovers that nearly half the stars in the sky are either double or multiple stars. Some of these are just accidents of perspective, one star happening to appear in the same line of sight as another, but many are true binary stars: two stars in orbit around each other, similar to the stars which shine on the fictional planet Tatooine in Star Wars.

Every star labeled on this map of Hercules, Boötes, and Ursa Major is a double star, worth exploring with a small telescope. Some, like Mizar in the Dipper’s handle, can be split with the naked eye. A closer look with a telescope shows that this is really a triple star. Others require binoculars or a small telescope. Some of the finest are Cor Caroli in Canes Venatici, Izar (Epsilon) in Boötes, Delta Serpentis, and Rho Herculis.

One of the joys of double star observing is the colour contrasts in some pairs. Others are striking for matching colours and brightness. My favorites are stars of very unequal brightness, which look almost like stars with accompanying planets.

Also marked on this chart are three of the finest deep sky objects: the globular clusters Messier 13 in Hercules and Messier 3 in Canes Venatici, and the Whirlpool Galaxy, Messier 51, tucked just under the end of the Big Dipper’s handle. You will probably need to travel to a dark sky site to spot this galaxy. A six-inch or larger telescope will begin to reveal its spiral arms, including the one that stretches out to its satellite galaxy, NGC 5195.

Starry Night 7: High Resolution Planetary Texture Collection

In recent years, NASA has conducted numerous exploratory missions that provided detailed measurements of the visual appearance and physical characteristics of most of the planets and moons in our solar system. These categories include IR/UV/visible imagery, physical, chemical and geological properties of the celestial bodies.

Measurements range from surface features to physical properties to chemical and geological characteristics. Surface features consist of topography, albedo, roughness and age. Fundamental physical properties include gravity, magnetism and temperature. Chemical and geological quantities comprise elemental composition, mineral distributions, geological maps and crustal thickness. 

Starry Night Pro Plus 7 offers a Planetary Science Texture Compilation with over 100 additional maps. Planetary images and data were derived from the latest datasets available. The original, highest quality sources were used to produce maps with maximum fidelity. Gaps and artifacts in individual datasets were corrected with data from older or alternate sources obtained by other exploratory space missions to produce consistent, high quality images that clearly illustrate the parameters of interest.
 

Earth:
Light Pollution Atlas

Jupiter:
Callisto Color
Callisto Gray
Europa Color
Europa Gray
Ganymede Color
Ganymede Gray
Io Color
Io Geology
Io Gray
Jupiter Color
Shoemaker-Levy

Mars:
Mars Albedo Color
Mars Albedo Gray
Mars Elemental Abundance Set
Mars Geoid
Mars Geological Map
Mars Gravity
Mars Magnetic Field
Mars MDIM
Mars Roughness
Mars Surface Dust Index
Mars Thermal Inertia
Mars Topo Jade
Mars Topo Spectrum
Mars Viking Color
Mars Viking MDIM Merged
Mars Viking Shaded
MOC color
MOC gray

Mercury:
Messenger Color
Messenger Gray
Mercury Messenger Color
Mercury Messenger Gray

Moon:
Clementine Color
Clementine False Color
Clementine Gray
Clementine Iron
Clementine Mineral Ratio
Clementine Optical Maturity
Lunar Gravity
Moon Crustal Thickness
Moon Elemental Abundance Set
Moon Geoid
Moon LROC Gray
Moon Roughness
Moon Temperature
Moon Topo
Moon Illusion Beetle
Moon Illusion Lady
Moon Illusion Lady Reading Book
Moon Illusion Man In Moon
Moon Illusion Rabbit
Moon Illusion St. George

Saturn:
Dione Gray
Enceladus Color
Enceladus Gray
Iapetus Color
Iapetus Gray
Mimas Gray
Phoebe Gray
Rhea Gray
Saturn Bjorn Jonsson
Saturn Hubble
Tethys Gray
Titan Color
Titan Gray
Titan IR
Titan Lakes
Titan Topo
Titan Topo scale

Sun:
Ca II 3933A
FeIX-FeX 171A
FeIX-FeX 171APNG Tiles
FeVII 195A
H-alpha
He II 304A

Venus:
Venus Geoid
Venus Gravity
Venus Magellan Color
Venus Magellan Gray
Venus Topo

Vesta:
Vesta Gray
Vesta Rock Types
Vesta Topo