38 AUSTRALIAN SKY & TELESCOPE July 2018
Asalways,yourbeststrategyistoobservetheplanetas
often as possible to maximise the chance of getting a sharp
look during infrequent spells of excellent seeing, when all
drossfallsawayandtheplanetlooksasrealasbeingthere.
Remember to allow your telescope’s optics to cool to the
outside temperature, so they don’t become their own source
of‘boiling’air.Marswon’tbethisclosetoEarthagain
until September 2035, a simple fact that motivates many a
Mars-watcher to put eye to eyepiece every clear night around
opposition.
The Red Planet will remain in Capricornus for the next
fewmonths,makingabriefforaywestintoneighbouring
Sagittarius near the end of its retrograde loop in late August.
Minimum declination of –26° 33′willoccuronAugust15
andbytheendofOctoberstillbearespectable–17°.
What to see
Thesouthpolarcap(SPC)willhighlightthefirsthalfofthe
apparition. Tipped in our direction, this frozen CO 2 button
will appear big and bright as it emerges from its winter hood
of clouds in late April and May. Watch it gradually shrink and
rift as opposition approaches. We’ll also see part of the north
polar hood (NPH), a dull, diffuse cap of clouds shrouding
thenorthpolarcap(NPC).Lookforitalongtheplanet’s
northern limb throughout the winter and early spring. The
NPH is often confused with the much brighter, more distinct
true cap, but that won’t be visible until mid-winter 2019.
Spring in Mars’ southern hemisphere occured on May
22 with the cap at maximum extent. North of the SPC,
keep a wary eye out for another polar cap look-alike, the
2,300-kilometre-wide impact basin Hellas. In June, Hellas
might be still be coated with frost or hidden under a blanket
of clouds, mimicking the appearance of a polar cap, but you
cantellthetwoapart—HellasisdistinctlynorthoftheSPC
and appears duller. Even small scopes should provide great
views of these polar features.
Albedo markings
Like the Moon, Mars readily reveals surface features called
albedo markingsacross its orange globe. Some change shape
with the seasons or from apparition to apparition depending
on how the Martian winds move bright surface dust around.
The most obvious southern hemisphere features include Syrtis
Major, an ancient shield volcano shaped like the subcontinent
India; the ‘chicken drumstick’ combination of Sinus Sabaeus
ARCADIA
UTOPIA MARE BOREUM
IAPYGIA
THARSIS
AMAZONIS
NILIACUS
LACUS
CHRYSE
AURORAE
SINUS
MARGARI-
TIFER
SINUS
SINUS
MERID-
IANI
Deucalionis Regio
Protonilus NILOKERAS
HELLAS MARE ERYTHRAEUM
ELYSIUM SYRTIS MAJORAERIA
ARABIAMOABEDEN
MARE
ACIDALIUM
SINU
SSABAEUS
MARE SERPENTISPANDORAE FRETUM
LIBYA
Hesperia
Tritonis
Sinus
Hyblaeus
Extension
Propontis
Tithonius
Lacus
Noctis
Lacus
Phoenicis
Juventae Lacus
Fons
Solis
Lacus
Claritas
Nix Olympica
(Olympus Mons)
Trivium
Charontis
Gomer
Sinus
Cerberus I
Idaeus
Fons
Achillis
Fons
Sigeus
Portus
Osiridis Pr.
HA
DR
IAT
ICUM
MA
M RE
AR
ET
YRR
HENU
M
Th
aumasia
0°
180° 200° 220° 240° 260° 280° 300° 320° 340° 0° 20° 40° 60° 80° 100° 120° 140° 160° 180°
180° 225° 270° 315° 0° 45° 90° 135° 180°
+20°
+40°
+60°
–20°
–40°
–60°
+90°
Oxia
Palus
Nodus
Alcyonius IsmeniusLacus
0°
+20°
–20°
–40°
–60°
+40°
+60°
+90°
MARE
SIREN
UM
MARE CIMMERIUM
SSOUTHERN ICE The south polar cap, which reaches 3 km deep in
places, is made up of frozen water and carbon dioxide.
SPRACTICE MAKES PERFECT The more often you observe Mars, the easier you’ll ind it to detect albedo markings. Use this map to identify
them. Damian Peach assembled this map from images he took during 2009–10. The globes, tipped correctly for the current apparition, are from
the software program WinJupos. Each globe displays the central meridian longitude that is directly below it on the map. Moderate-aperture
telescopes will show only the darkest, largest regions. South is up.
MARS OPPOSITION